Macquarie University ResearchOnline · TOP LEVEL SPECIFICATIONS ... spectrum by illumination a test...

Macquarie University ResearchOnline

This is the published version of: Andrew Sheinis ; Sam Barden ; Michael Birchall ; Daniela Carollo ; Joss Bland-Hawthorn ; Jurek Brzeski ; Scott Case ; Russell Cannon ; Vladimir Churilov ; Warrick Couch ; Robert Dean ; Gayandhi De Silva ; Valentina D'Orazi ; Tony Farrell ; Kristin Fiegert ; Kenneth Freeman ; Gabriella Frost ; Luke Gers ; Michael Goodwin ; Doug Gray ; Ron Heald ; Jeroen Heijmans ; Damien Jones ; Stephan Keller ; Urs Klauser ; Yuriy Kondrat ; Jon Lawrence ; Steve Lee ; Slavko Mali ; Sarah Martell ; Darren Mathews ; Don Mayfield ; Stan Miziarski ; Rolf Muller ; Naveen Pai ; Robert Patterson ; Ed Penny ; David Orr ; Keith Shortridge; Jeffrey Simpson ; Scott Smedley ; Greg Smith ; Darren Stafford ; Nicholas Staszak ; Minh Vuong ; Lewis Waller ; Elizabeth Wylie de Boer ; Pascal Xavier ; Jessica Zheng ; Ross Zhelem and Daniel Zucker " First light results from the Hermes spectrograph at the AAT ", Proc. SPIE 9147, Ground-based and Airborne Instrumentation for Astronomy V, 91470Y (July 8, 2014) Access to the published version: http://dx.doi.org/10.1117/12.2055595 Copyright: Copyright 2014 Society of Photo-Optical Instrumentation Engineers (SPIE). One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.

First Light Results from the Hermes Spectrograph at the AAT Sheinis, Andrew a, d; Barden, Sam c; Birchall, Michael a; Carollo, Daniela g; Bland-Hawthorn, Joss d;

Brzeski, Jurek a; Case, Scott a; Cannon, Russell a; Churilov, Vladimir a; Couch Warrick a; Dean, Robert a; De Silva, Gayandhi a; D'Orazi, Valentina g; Farrell, Tony a; Fiegert, Kristin a; Freeman,

Kenneth b; Frost Gabriella a; Gers, Luke a; Goodwin, Michael a; Gray, Doug a; Heald, Ron a; Heijmans, Jeroenh ; Jones, Damien e; Keller, Stefan b; Klauser, Urs; Kondrat, Yuriy a; Lawrence, Jon

a, g; Lee, Steve a; Mali Slavko a; Martell Sarah a, i; Mathews, Darren a; Mayfield, Don a; Miziarski, Stan a; Muller, Rolf a; Pai, Naveen a; Patterson, Rober a t ; Penny, Ed a; Orr, David a; Shortridge, Keith

a; Simpson, Jeffrey g; Smedley, Scott a; Smith, Greg a; Stafford, Darren a; Staszak, Nicholas a; Vuong, Minh a; Waller, Lewis a; Wylie de Boer, Elisabeth b; Xavier, Pascal a; Zheng, Jessica a; Zhelem, Ross

a; Zucker, Danielg

a Australian Astronomical Observatory (AAO) PO Box 296, Epping NSW 1710, Australia b Australian National University (ANU), Research School of Astronomy & Astrophysics, Mount

Stromlo Observatory, Weston ACT 2611, Australia c Leibniz-Institut für Astrophysik Potsdam (AIP),14482 Potsdam, Germany

d School of Physics, The University of Sydney NSW 2006, Australia; e Prime Optics, Eumundi, QLD 4562, Australia

f Centre for Astrophysics Research (CAR), School of Physics, Astronomy and Mathematics, University of Hertfordshire (Herts), Hatfield, AL10 9AB, UK

g Department of Physics and Astronomy, Macquarie University, NSW 2109, Australia hTNO – Hoofddorp Netherlands

iSchool of Physics, The University of New South Wales, Sydney NSW Australia

ABSTRACT

The High Efficiency and Resolution Multi Element Spectrograph, HERMES is an facility-class optical spectrograph for the AAT. It is designed primarily for Galactic Archeology [21], the first major attempt to create a detailed understanding of galaxy formation and evolution by studying the history of our own galaxy, the Milky Way. The goal of the GALAH survey is to reconstruct the mass assembly history of the of the Milky Way, through a detailed spatially tagged abundance study of one million stars. The spectrograph is based at the Anglo Australian Telescope (AAT) and is fed by the existing 2dF robotic fiber positioning system. The spectrograph uses VPH-gratings to achieve a spectral resolving power of 28,000 in standard mode and also provides a high-resolution mode ranging between 40,000 to 50,000 using a slit mask. The GALAH survey requires a SNR greater than 100 for a star brightness of V=14. The total spectral coverage of the four channels is about 100nm between 370 and 1000nm for up to 392 simultaneous targets within the 2 degree field of view. Hermes has been commissioned over 3 runs, during bright time in October, November and December 2013, in parallel with the beginning of the GALAH Pilot survey starting in November 2013. In this paper we present the first-light results from the commissioning run and the beginning of the GALAH Survey, including performance results such as throughput and resolution, as well as instrument reliability. We compare the abundance calculations from the pilot survey to those in the literature.

Keywords: HERMES, spectrograph, AAT, 2dF, VPH, GALAH, fiber

a

*[email protected]; phone +61 2 93724821; fax +61 2 93724880; www.aao.gov.au

Ground-based and Airborne Instrumentation for Astronomy V, edited by Suzanne K. Ramsay, Ian S. McLean, Hideki Takami, Proc. of SPIE Vol. 9147,

91470Y · © 2014 SPIE · CCC code: 0277-786X/14/$18 · doi: 10.1117/12.2055595

Proc. of SPIE Vol. 9147 91470Y-1

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1. INTRODUCTION The latest in a long history of instruments to be developed by the AAO Instrumentation Group (IG) for the Anglo-Australian Telescope (AAT) is the High Efficiency and Resolution Multi-Object Spectrograph (HERMES) for the AAT. HERMES is a facility instrument, designed to provide high-resolution multi-object spectra in the visible. The primary science driver is Galactic Archeology, in which detailed abundances of up to 20 elements are used to chemically tag stars in order to understand their origin and star formation history. The primary program is the Galactic Archeology with Hermes survey (GALAH), which has begun as a pilot survey in late 2013 and is now in full data gathering operations. GALAH will measure the chemical abundances of 1000,000 stars in the Milky Way. HERMES provides a nominal spectral resolving power of 28,000 for GALAH with a high-resolution mode of about 45,000, over 4 non-contiguous bands within the 370-1000 nm window. The opto-mechanical design of HERMES2 allows for reconfiguration of the bands to enable astronomers to pursue other spectral bands of interest between 370 - 1000 nm. The spectrograph uses four large 500 x 200mm Volume Phase Holographic (VPH) gratings and is fed by the 2dF fiber-positioning robot at the AAT telescope prime focus. There are two slits of 392 science fibers each that allow for one slit to collect science data while the robot configures the other slit for the next observation. Details of the 2dF positioner system are available in [23].

The AAO IG has: completed its assembly, integration and testing of the HERMES spectrograph at the AAO head quarters in Sydney; delivered the instrument to the AAT site in mid 2013; and along with the GALAH team, has fully commissioned the instrument in Oct-Dec 2013.

2. TOP LEVEL SPECIFICATIONS The HERMES spectrograph is required to achieve the following top-level functional performance specifications:

1) The HERMES system should have high spectral resolution (λ/∆λ) of ~50,000 at multiplex of 400 targets. (For Stellar Astrophysics, Interstellar Medium, and Radial Velocity Variability science cases.)

2) The HERMES system shall provide 4 configurable windows located in the wavelength range 370 - 1000 nm. Nominally:

a. 471.8 nm – 490.3 nm b. 564.9 nm – 587.3 nm c. 648.1 nm – 673.9 nm d. 759.0 nm – 789.0 nm

3) The HERMES system shall provide the following sensitivities for brightness, V=14, SNR of 100 in 60 minutes of integration. For galactic archaeology (V=14) this corresponds to a system efficiency of 0.1 Brightness of targets: 10−14 for main galactic archaeology survey; down to 16 – 17 for targeted observation. Typically >14 for stellar astrophysics and radial velocity variability science cases.

3. ASSEMBLY AND INTEGRATION At the end of March 2013, initial integration and testing, in the Epping-Sydney lab, of the HERMES Spectrograph came to a close. Tests were carried out on a fully aligned spectrograph with completed Blue, Green, and Red Channels. The IR Channel, while structurally complete, was not tested as the IR-VPH grating was still being manufactured. Testing in the Epping lab was limited to the use of a test fixture for the slit, which is similar to, but does not perform to the full standard of the slits attached to the 2dF Fiber Cable. Included in the testing was the acquisition, and reduction of a solar spectrum by illumination a test fiber bundle with sunlight and feeding that to HERMES. The testing showed conclusively that all the systems within HERMES were operational and ready for shipment to the AAT at Siding Spring Observatory, but that the optical (image-quality) performance in the green and red channels was not within spec. After



extensive testing it was determined that this was primarily due to wavefront errors (primarily astigmatism) introduced in the green and red gratings. It was decided at the time that this issue should not drive the overall HERMES Schedule and the issue could be resolved in parallel. In addition, the AAO instrumentation group was required to vacate our Epping facility to move and re-establish ourselves in our new facility in North Ryde, some 5 Km from Epping. Our time in Epping had come to a close. In the first week of April 2013 the process of disassembling HERMES, packing, and transporting to site began. During the disassembly process HERMES received its NEXTEL black interior paint work. After 5 weeks, five 20-foot container truck loads, 6 moving van loads, and approximately 10 station wagon trips, HERMES was safely transported to the AAT. On the last week of June 2013, the re-assembly process began at the AAT in Coonabarabran NSW. The aggressive goal was to have a fully operational instrument for the scheduled first commissioning run on October 19th, 2013. This left little over 3 ½ months to take a completely disassembled and packaged HERMES to a fully rebuilt, aligned, working instrument. This was quite a challenge but the team was keen. After a complete design, and fabrication stage at site, the HERMES temperature-controlled room was ready to receive its instrument. The first step was to position the vibration isolators in the correct position on top of the concrete piers. The next step of the rebuild process was to re-assemble the HERMES structure. This main support structure is called the “spine” of HERMES. The spine supports the slit assembly, field lens, collimator mirror, corrector lenses, and beam splitters. Off the spine are four structures that are bolted and pinned to the spine. Each of these structures is for one arm of the spectrograph. These structures support a grating, fold mirror, and light baffling. Cantilevered off each of the four channel structures, is the camera focus drive assemblies and cryostat assemblies. The HERMES structure was designed to be modular to aid in the disassembly and re-assembly process.

Figure 1. HERMES Spine being set to air isolators. Figure 2. HERMES structure nearing final assembly. IR Box removed to allow collimator alignment. Following rebuild of the HERMES structure, the blue, green, and red camera assemblies were re-attached. To save time and schedule the cameras were shipped fully integrated in their structural mount/flexural focus drive mechanism. With the cameras mounted, the 1 meter-diameter HERMES collimator mirror was reassembled into its mount and then reset onto the structure. All the most massive HERMES components were now set to the frame, fully loading the structure, with the exception of the IR channel structure and camera, which was left until later in the assembly to allow alignment access of the collimator down the center of the spine



Figure 3. Green camera assembly being craned into position. Figure 4. Collimator mirror being inserted into its chain mount.

The collimator alignment process was now able to commence with the HERMES collimator mirror first being set to the established optical axis[20]. The collimator mirror was tested interometrically in the assembled condition to ensure no stress was being transferred to the surface and it was still meeting wavefront requirement. Following the collimator mirror alignment the field lens and corrector lens were aligned to the optical axis. The slit assembly was set into position and focus was verified across all fibers of the two slit assemblies, as we looked back through the collimator assembly with a metrology telescope arangement.

Figure 5. Collimator mirror craned on top of the spine mount. Figure 6. View through the spine. Point source microscope in position to align collimator optics.



Figure 7. Corrector lens being lowered into their kinematic mounts within the frame. Figure 8. View of the exchanging slit assembly, field lens, back illuminators, and corrector lens asembly (right). In parallel with the HERMES re-construction was an effort to solve the grating astigmatism issue. As detailed in section 4.3, the plan was to repolish the gratings flat and have them re-coated. This plan went forward and sucessfully brought the gratings to a completed state as they were just needed for the HERMES channel alignment. With the HERMES collimator assembly fully assembled and aligned attention was turned to aligning each of the fold paths. Alignment progressed from Blue, Green, Red and finally the IR path. Using prism setups, alignment telescope and PSM, each of the fold paths were brought into alignment with the previously established optical axis[20]. The beam splitters and gratings were addjusted via shimming on their kinematic mounting arangement. Fold mirrors utilized an integrated precision tip-tilt arangment in the mount driven by high precision 100 pitch screws. Alignment targets to each of the cameras were previously set, and camera alignment to the optical axis was verified to be within specification.

Figure 9. Green channel alignment setup. Figure 10. Beamsplitter being craned into position.



In parallel with the opto-mechanical assembly and alignment the electronics team re-assembled all the electronic control cabinets, ran all the cables to the instrument, and fully re-wired HERMES. Cryostats were remounted after channel alignment. Controllers were assembled to the cryostats. The process of pumping each cryostat and cooling to temperature began. After each cryostat was brought to temperature final alignment of each cryostat to each camera was performed. Cameras were focused utilizing every last minute, but HERMES was ready and saw first light on 47 Tuc on its scheduled commissioing run on Ocotber 19th having been finished with just hours to spare! Since the first commissioning run, HERMES has completed the GALAH pilot survey, and is now taking scientific survey data. The HERMES room is now assembled and complete. Only minor tweaks to the alignment have been implemented. Minor bug fixes have been implemented. No major design changes have been required. The instrument is now fully in the hands of the AAT site staff.

Figure 11. HERMES fully assembled.

4. OPTICAL COMPONENTS



IR Camera

Red CameraFold Mirror

Blue Camera

VPH Grating

Corrector lenses Collimator

BeamSplitters

Fibre Slit

Green Cameraitrrruui

'al ti

There are three main optical assemblies in the HERMES spectrograph that were deemed high risk. While in a spectrograph as large as HERMES all optics are high risk the camera assemblies, collimator assembly, and the especially the volume phase holographic grating (VPH) had the most potential to effect performance and delivery schedule. As a result a series of metrology tests were done to ensure vendors delivered as promised and to minimize for any

unaccounted performance losses in the spectrograph.

Figure 12. Optical layout of the HERMES spectrograph

4.1 Camera optics

Each of the four cameras in the spectrograph is an F/1.67 refractive design with a 380 mm diameter first element, with an entrance pupil of 190 mm located at the grating. The cameras assembly contains a doublet, with an aspheric first surface, and then 3 additional lens elements. The camera assembly does not contain the dewar optics, which consist of 2 windows and a field flattener lens just above the detector. The vendor supplying the cameras relied on a coordinate measuring machine data (CMM) to align each individual lenses of the camera in the lens cell, which was determined to be insufficient to fully verify performance. To ensure the performance of the cameras two tests were conducted by AAO personnel on the cameras; a double pass interferometric test and a lens alignment check with an autocollimating alignment telescope at the vendor facility and again after shipping to the AAO.

Each camera was designed to overlap the previous cameras wavelength coverage for future instrument modifications. While this made the design a little more challenging this did allow a common null lens to be used for the interferometric testing with only slight modifications to the distance between the null lens, the camera, and the interferometer. Due to the weight of the camera, 220 kg, the interferometric testing was designed in such a way that the interferometer and the null lens were brought to the optical axis of the camera. The interferometer was attached to a 250 mm precision linear stage with an F/1.5 reference sphere. The interferometer was aligned iteratively using the returns from camera lens optical surfaces at their respective centers of curvature (COC). By setting the first surface of the of the fourth lens as a reference as well as the last surface on the third the lens, an optical axis was



quickly established with minimal distortion from other elements in the system. Furthermore the inteferometric returns confirmed the lens spacing’s and defined offset positions for the null lens. Using a Monte-Carlo tolerance analysis the upper and lower bounds were predetermined for a number of Zernike polynomials that would provide a Go/No-Go performance evaluation for the cameras, as is typically done for mass produced components. If the inteferometric test proved the performance insufficient then the alignment of each lens could be determined using the autocollimating alignment telescope with the PIP attachment[20]. The second test uses the autocollimating alignment telescope with a fixed point source set at a distance from the optical assembly. The high intensity point source is reimaged by each optical surface. By aligning the alignment telescope to two optical surfaces in the camera the displacement of all the surfaces could be determined using the ‘pip’ returns from surface whether real or virtual. Fortunately, the cameras tested well the first time at the vendor facility and again at the AAO requiring only a quick check using the second test method.

Figure 13. Camera under test with the autocollimating alignment telescope after inferometric testing (left), IR camera

transmitted wavefront using the null lens resulting in a measured wavefront of RMS 0.17 wv and PV 1.88 wv at 632.8 nm (right).

4.2 Collimator assembly

The HERMES spectrograph uses an off-axis Houghton-based collimator design with a slit curved to match the radius of the focal surface as presented to the spectrograph curved again perpendicularly along the surface of the sphere to compensate for the spectral smile. The collimator consists of a relatively small field lens, a 1 meter diameter spherical mirror weighing 500 kg, and two off-axis corrector lenses 620 x 330 mm in diameter in an assembly weighing 250 kg. The collimator optics each had their issues. While each issue was found in testing, some were expected due to good reporting from vendors, and others were uncovered later in the process.

The 1 meter diameter collimator mirror is a standard 6:1 diameter to thickness ratio mirror with enhanced silver coatings to improve throughput at 370 nm. The mirror had two issues. One, the mirror is strap mounted using an invar and stainless steel chain. This made the mirror very sensitive to gravitational loading, created if the mirror was unbalanced with respect to the gravity vector and the face contact pads. This required interferometric testing at the time of integration to qualify the angle of the mirror with respect to gravity so the mounting didn’t inadvertently load the mirror face on the front reference pads. Two, the enhanced silver coating has proved challenging on two fronts. The coating performance proved very challenging to obtain on such a large mirror and the adherence of the coating is proving softer than promised. While witness samples of the coating passed testing for adhesion and abrasion requirements using MIL-C-48497, the coating on the mirror itself has proven soft and uncleanable as it does not conform to MIL-C-48497.

The fabrication and alignment of the collimator corrector lenses proved difficult from the onset. Due to the sheer size of the refractive off-axis element, it was deemed not cost effective and technologically too challenging to make a full-size on-axis parent. Thus, the blank size was restricted to the final as-built size of the lens to reduce costs. This made the fabrication of the second surface on each corrector lens particularly challenging as the surface became a



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tilted/decentered spherical surface with respect the first surface. The alignment by the vendor relied on a large three axis CMM to square each surface in assembly. It was first thought that this would provide an accurate alignment even with the limited number of sampling points at each step in the alignment of the two lenses in a common cell. The long radius of curvature on two of the surfaces, 3813 mm and 1986 mm, proved later the sag difference too small to discern over the error of the machine for a given sampling area, the sampling area too small, and possibly that a mounting flange ground into one of the lenses had the wrong angle. This resulted in an alignment error of the two lenses with respect to each other far above the required tolerance. The error was found using the autocollimating alignment telescope and the PIP attachment to image the centers of curvature of each lens surface. Further analysis in optical design software showed that the error added little change to the performance of the system. Due to time constraints it was deemed a worthy exercise to integrate the corrector lenses into the system as long as the camera optics, collimator mirror, and the gratings induced minimal error. With the errors known for the corrector assembly, the alignment compensated for the errors in order to locate and align the collimator corrector lenses. .

4.3 VPH grating

The VPHG proved not only a challenge to manufacture, but also to qualify the error induced by manufacturing errors. There are four gratings in HERMES, each 550 x 220 x 40 mm in size, with line frequencies from 3827 to 2378 lines/mm working at a 67.2 degree angle of incidence.

As highlighted in earlier papers[1,2,3,4,18,19], the extreme working angle of the grating forced the design of the grating to be optimized for s-polarization. Due to the size, the working angle of the grating, and the high resolution a custom large-aperture metrology system had to be built at the AAO to test the gratings for spectral and wavefront performance. Due to manufacturing processes the deformation of the carrier glass is very hard to control due to the internal stresses from the gelatin and bonding process. As a result the HERMES gratings had to be post polished after manufacturing to remove the deformation from the outer surfaces. What is still not clear is whether the grating surface inside the VPHG is itself bent along the internal surface and how that is contributing to wavefront error in the system due to our limited interferometer aperture. Due to time and budgetary constraints the gratings were integrated into the spectrograph and fortuitously, the maximum amplitude of diffracted wavefront error was lower than extrapolated error from sub-aperture measurements. Making the carrier glass thicker is one way to solve the problem, but due to the size of the grating in HERMES the glass weight quickly becomes unmanageable and would require complete retooling at the manufacturer facilities if the glass diameter to thickness is made on the standard 6:1 ratio with respect to the long axis of the diameter. Another unexpected surprise for future spectrographs of equivalent size to HERMES using large VPH’s is the number of carrier plates needed to in the manufacturing process. The AAO purchased 13 plates for only 4 gratings.

Figure 14. Red VPHG surface profile before repolishing (left), Red VPHG transmitted wavefront at repolish at working

angle of 62 degrees. (right).



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Figure 15. The two curved slit assemblies on the translation stage, right: single V-groove block for lens mounting 40 lens sets

Figure 16. The mounted collimator mirror before coating and its interferogram, P-V=0.1 wave, RMS=0.013wave



5. CRYOSTATS AND DETECTORS The HERMES detector cryostat shell is based on an Infrared Laboratories cryostat with a Polycold PCC cryocooler cold head to which we have fitted a Pfeiffer PKR full range vacuum gauge head. The end plate is replaced by a custom shell extension which encloses the detector and field flattener assembly. Hermetically sealed connectors, one for the detector control and data, another for thermal control, are mounted through the wall of this shell extension. To maintain thermal isolation a G10 fiberglass ‘spider’ is used to locate the detector and field flattener to the wall.

Figure 17. The detector assembly with the mounted field lens mounted, (before blackening) To ensure a good match to the thermal expansion of the CCD detector, a molybdenum mounting plate is used. The thermal control hardware, heaters and a diode sensor are mounted directly on this plate. Three heaters are used to provide an even distribution of the heat input required for temperature trimming to much less than 0.1°C. The mount for the bi-concave field flattener lens is mounted with less than 4mm gap from the detector. Cooling of the detector assembly is implemented by linking the detector mounting plate to the cryocooler head using oxygen-free copper thermal links. To minimize thermal strains and maintain detector alignment these links incorporate corrugated sections which structurally decouple the cryocooler head from the detector assembly. The contamination ‘getter’ is also connected via separate links to the cold head. A radiation shield encloses the detector and field flattener assembly and the thermal link and getter assembly. The cryostat shell is sealed by a front plate which accommodates the plane window, which withstands the atmospheric pressure load and a second thinner window. Dry nitrogen may be flushed between these windows to prevent dewing that might otherwise occur on high-humidity nights. Internal electrical wiring is accomplished using flexible PCBs and the detector controller electronics box is mounted directly on the cryostat shell to minimize noise. Design variations between cryostats result from the different wavelength ranges at which they operate and are limited to different CCDs, field flatteners and window coatings. The detector control electronics includes the CCD controllers and their power supplies for each detector, as well as the computer systems that send commands to and acquire data from the CCD controllers. Each CCD detector in HERMES is controlled with an AAO2 CCD controller5. These controllers are configured for operation with the e2v CCD231-84 detectors to permit readout from one, two or four detector outputs, at various readout rates with windowing and binning. The CCD controller electronics and enclosures have been manufactured and most of the individual boards have been tested. Three of the four HERMES CCDs have been tested and characterised in a test cryostat and the “engineering” grade detector has been installed in the blue camera cryostat and is undergoing performance verification tests prior to the blue science grade detector being installed. At this point the blue cryostat is showing excellent vacuum and thermal performance. The next step will be to swap the blue science grade detector into the cryostat.



6. FIBER CABLE FEED The HERMES/AAOmega fiber bundle was designed to co-inhabit the 2dF robot positioner so that no instrument changeovers were required to switch between HERMES and AAOmega, and also that there is no need for connectorisation6. This led to the design of two fibers occupying one magnetic button, one for AAOmega fiber and one HERMES fiber, see the figure below. The 2dF robot positions the magnetic button on the field plate and determines its position by looking at the back illuminated science fiber. .

The fiber cable, with its 4x400 fibers, has been built and equipped with its slit and button assembly. They have been installed and tested on the 2dF fiber positioner at the AAT in October 2013 during scheduled 2df downtime.

The existing cable had a fringing problem that caused a wavelength-dependent intensity fluctuation in the measured spectra. This was found to be related with a cavity that was formed between the prism and the fiber face at the button end of the fiber cable. This connection has been redesigned and adhesives are used that have a better thermal match, low shrinkage and creates a strong bond. The assembly was tested on the AAT for five months and no fringing was observed.

Another point of attention has been to prevent the fibers from stressing as this can cause focal ratio degradation, (FRD). With a fiber cable of almost 50 meters in length there are many points where the fiber is bent and fixated. With large bending radii, protective sleeves and low stress points at fixations, the FRD was kept low and the achieved throughput for the new fiber cable is significantly higher (>50%) than the existing cable.

The 2dF buttons comprise of fibers terminated in a glass ferrule with a polyimide jacket covering the two AAOmega/HERMES science fibers plus a short (30mm long) dummy fiber to align the fibers perpendicular to the prism face. These ferrules are then glued into magnetic buttons to locate them on the 2dF field plate. The images below show the assembly.

Figure18. 2dF button. 1- Prism. 2- AAOmega/HERMES science fiber. 3- Dummy fiber. 4- Glass ferrule. 5- Polyimide tube. 6-

Magnet. 7- Button body (Prism size is 1mm). Right: an image of 10 fibers in a slitlet

At the slit entrance the fibers are assembled in slitlets that locate 10 fibers in v-grooves and collectively they make up a slit of 400 fibers.

The HERMES slitlets were glued and polished successfully. The locations of the fibers in their v-grooves with respect to their nominal positions relative to the slitlet body were measured using a MicroVu co-ordinate measurement system. The fiber locations were within the required radial position tolerance of +/-10µm to prevent crosstalk at the detector images.



7. CONTROLLERS AND ELECTRONICS The electronics for HERMES is broadly separated into two categories: instrument control electronics and detector control electronics, as shown in Figure 10. The HERMES instrument control electronics is responsible for controlling and monitoring all the actuators and sensors used to configure and operate the instrument. The instrument control electronics is based on a distributed control system that uses the CANopen protocol running on the Controller Area Network (CAN) field bus. All analog and digital functions are interfaced to CANopen input/output nodes and all servo motor driven actuators are controlled by CANopen digital servo drives. The CAN bus is connected to an industrial control cabinet PC with a CAN interface, running the Linux operating system and operating as the CANopen master. The instrument control electronics is implemented in six industrial electronics enclosures distributed around the outside of the spectrograph thermal enclosure. The majority of the instrument control electronics is commercial off-the-shelf. Some customization has been done on the slit back illumination control and drive, interlocking and interfacing for the Bonn shutters and servo amplifier breakout.

Detectors

Coude West Room Spectrograph Enclosure

Slit

BlueCamera

GreenCamera

RedCamera

IRCamera

Blue CCD& Cryostat

Green CCD & Cryostat

Red CCD& Cryostat

IR CCD& Cryostat

Blue CCD Controller

Green CCD Controller

Red CCD Controller

IR CCDController

Cryostat Support (Vacuum

Monitoring)

Green CCD Controller

PSU

Red CCD Controller

PSU

IR CCDController

PSU

Fibre Optic Links

LAN

2dF Back Illumination

Instrument Control

Shutter Control & Status

Blue CCD Controller

PSU

Detector Control Electronics

Instrument Control Electronics

Figure 19. Schematic overview of the HERMES Electronics Systems

A CAN/CANopen system including a digital servo drive and digital and analog input and output was prototyped during the final design phase of the project. This has been available to allow software and hardware development and testing to proceed from an early stage in the project.

The assembly of the instrument control electronics is largely complete, and is currently undergoing power up and basic functionality tests prior to being integrated with the instrument hardware.



HERMESSpectrograph

Control

Fibre to FITSFibre

PositionTweak

TelescoTeThControlSystem

Fpi ImageDisplay (Skycat +

DRAMA)

2dF Fibre Positioner(2dF Robot

VxWorks CPUSupervisor

--( CCD #1 )

--( CCD #2 )

--{ CCD #3 )

.---( CCD #43

MO 2 CCU Systems

8. SOFTWARE AND DATA REDUCTION 8.1 Architecture and layout

Extensive use was made of existing software deployed as part of the 2dF/AAOmega instrument. This software was written using the AAO’s DRAMA API[7] for the deployment of the original 2dF Instrument configuration, in 1994, but has been modified over the years for new spectrographs, detector systems and configurations.

For development purposes, the software for HERMES was broken into five major areas. The Observing system is responsible for overall control of the entire observing run-time (including the 2dF robot and CCD operations) and provides the main GUI. The HERMES Spectrograph Control task is responsible for control of the spectrograph itself. The AAO2 CCD detector software[8], shown in the figure below as CCD System, is used to run the detector systems. The Fiber Configuration software, not shown, is responsible for allocating fibers to objects as part of proposal preparation. A separate Data Reduction package provides pipeline reduction to the point of producing calibrated spectra.

Figure 20. Overview of the 2dF observing system software tasks when running in HERMES mode

8.2 The HERMES Observing System

The existing 2dF Observing system has been modified to control HERMES in addition to AAOmega. The Observing system controls the 2dF Fiber Positioner, the Spectrographs, Detector Systems, 2dF Calibration system, 2dF Atmospheric Dispersion Corrector, the Telescope and a number of minor components. Each sub-system has its own DRAMA task. The AAO 2 CCD detector software is itself an independent set of DRAMA tasks used by the 2dF software, as is the AAT’s Telescope Control software. Overall control, software interlocking and synchronization are



provided by the 2dF Control Task. This Observing system has proven flexible and adaptable since being originally commissioned in 1994, with the CCD System, Telescope System and Spectrographs having been changed during that time. For HERMES, we adapted the control task to implement a new mode of operation where the AAOmega Spectrograph DRAMA task is replaced by the new HERMES Spectrograph DRAMA task. Additionally, the control task and detector software were adapted to control four CCD systems, rather than the two previously supported. Switching between AAOmega mode and HERMES mode is via a command line option at system startup.

All sub-systems of the 2dF Observing system are required to implement simulation modes that allow for development of the Observing System without access to the instrument hardware. This was used extensively and as a result the 2dF Control Task was largely adapted to work with HERMES before the instrument itself was completed.

8.3 Spectrograph Control

The HERMES Spectrograph DRAMA task replaces the AAOmega spectrograph task when 2dF is running in HERMES mode. This task is responsible for communication with the spectrograph hardware and implementing high-level commands (DRAMA commands) for controlling the hardware. It provides instrument state for inclusion in FITS file headers and makes status information available via DRAMA parameters for inclusion in the system GUI.

An extensive hardware simulator has been provided using instrument simulator technology previously developed at the AAO[9]. This provides simulation of the CANBUS electronics hardware of the spectrograph at a level that requires no changes to the Spectrograph Task when running in simulation. Individual components of the instrument may be simulated at will. We used this extensively to advance development of the Spectrograph Task.

8.4 CCD Control

HERMES was the first AAO Instrument using 4 readouts (quadrants) per detector. It is also the first instrument using 4 detectors at once and using large detectors of 4kx4k pixels. Previous instruments were limited to 2 readouts per detector and 2 detectors at once. The AAO 2 CCD software was designed to support 4 readouts, but with no such detector configuration previously available, the implementation was not completed. We have now been able to complete this implementation, whilst at the same time optimizing the HERMES detector control modes. Adaption of the software to support 4 detectors running in one configuration was made early in the HERMES project, and we regularly operated four detectors in simulation whilst adapting the 2dF control task for HERMES. Due to hardware limitations, we only had 2 detector controllers available simultaneously before the HERMES instrument was moved to the AAT, so the final testing of the detector control configuration was not possible until then, but all high-risk areas had been tested and the final move to 4 detector controllers was completed without any issues.

8.5 Fiber Allocation

To observe a field on 2dF, you must allocate objects to fibers. This is done using a program known as “AAO Configure”. Implemented originally for 2dF in 1994, it was adapted to support the 6dF Instrument on the UK Schmidt Telescope and FLAMES on the VLT UT2, and to various changes in 2dF over the years. It was also modified to implement a Simulated Annealing allocation method.

Minor changes were required for HERMES - basic instrument support and supporting the use of proper motions[10]. Proper motions had been supported in the FLAMES implementation, but had not been implemented with 2dF until now. The allocation algorithm was modified for HERMES, to optimize for fiber efficiency considerations such as cross talk

8.6 Data Reduction and Data Simulator

The AAO provides software to reduce the image data files produced by HERMES to the extent of generating calibrated spectra with (as far a practical) all instrument signatures removed. Science processing is left to the science teams, but in this case there was clear requirement to interface efficiently to the “Galactic Archaeology” abundance pipeline. The AAO’s existing Fiber Instrument Reduction Package – 2dFdr, was adapted to support HERMES. This package had previously proven to be adaptable to different Instruments and such adaptations are now relatively easy to implement. The signal to noise requirements on HERMES to carry out “Galactic Archaeology” combined with the high resolution of the instrument led to a tough set of requirements being imposed on data reduction for HERMES. Additionally, the typical delay of 6 to 12 months after instrument commissioning before data reduction is optimal was considered unacceptable. Fortunately, most requirements proposed for HERMES also improves the reduction of other instruments supported by the package, allowing significant testing before commissioning. Additionally, we implemented a Data



Simulator[11,12] capable of producing simulated HERMES frame with all known instrument effects accounted for. The following significant improvements were made to the software

• Tramline tracking (tracing of the fiber paths on the detector) accuracy is improved to ~0.1pixel • Optimal extraction routines have been extensively revisited, with more improvements underway. • Routines are more stable (resulting in fewer pixels incorrectly marked bad) • Variance estimation is much more accurate • Tramline mapping in extremely sparse fields has been improved • A b-spline scattered light option has been added to optimal extraction • Improved Wavelength Calibration using an algorithm based on Whale Shark identification15 and tank tracking

to archive wavelength calibration to ~0.1pixel • Principle Components Analysis (PCA) Sky Subtraction[14]

Currently the Galactic Archaeology team is undertaking the analysis required to complete characterization of the data, to allow us to further optimize the reduction. In particular, they must determine the best approaches to sky subtraction and the correct profile to use in the Optimal Extraction.

9. SPECTROGRAPH PERFORMANCE 9.1 Spectrograph on-sky performance

HERMES on-sky commissioning was carried out over the months of October, November and December 2013. A range of observations were carried out and covered a lot of ground; determining readout speeds and combination of amplifiers, the required calibrations and their exposure times, PSF variations, fiber cross talk and scattered light levels, and overall instrumental resolution and throughput. This information allowed selecting the default instrument settings, to determine the magnitude limits, to set up the focus procedure and to confirm the appropriate alignment of the optics. A summary of the commissioning results is presented. 9.2 Spectral Resolution HERMES provides two resolution modes, the nominal resolution mode of R ~ 28,000 and a higher resolution option utilizing a slit-mask (at the cost of 50% light loss). The HERMES nominal and mask mode spectral resolution was measured using the ThXe calibration lamp exposures. 9.3 Throughput The throughput of the AAT+2dF+HERMES system was determined by measuring the detector counts over a range of standard star observations. The over all flux transformation equations (from star to detector) are given below for each channel: Blue Channel: e- per resolution element per hour = 10(-0.4(0.993*B - 24.05)) Green Channel: e- per resolution element per hour = 10^(-0.4(1.18*V - 26.25)) Red Channel: e- per resolution element per hour = 10^(-0.4(1.07*R - 24.98)) IR Channel: e- per resolution element per hour = 10^(-0.4(0.89*I - 22.33)) Note that in the above transformations, B, V, R, I refer to the Johnson B,V, R and I filters which are the nearest bands to the four HERMES channels, and is based on the median seeing conditions at Siding Spring Observatory. Table X gives the corresponding magnitude limit to achieve 104 electrons (signal-to-noise = 100) per resolution element.

Channel Magnitude Blue B = 14.2 Green V = 13.8 Red R = 14.0 IR IR = 13.8

Table 1. The magnitude limits for each HERMES channel to achieve 104 electrons per resolution element, in the nominal HERMES resolution mode.



He Colas Plots PAga.S Waldo.

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Pan: 0.000.00- 8.00Asenure: 91.9Orientation 180.0000- 1.000.00Z -Scale 0.25X 3066 Y. 719 Z 1 Data: 8918 Min: 321 Max 12347 Mean: 15:

Ghosts

The use of the high-resolution mask reduces the flux by a factor of two, raising the limiting magnitude by 0.7mag. Overall the HERMES throughput performance meets or exceeds the required specification to obtain a signal-to-noise of 100 per resolution element for a 14th magnitude star within one-hour exposure time. During lunar bright-time, the sky background limits observations of targets fainter than 14th magnitude. In darker skies, HERMES can be used to observe targets down to 17th magnitude over extended exposure times. 9.4 Ghost and Scattered light Scattered light in the form of dispersed background light from surface reflections is minimal in HERMES. The inter-slitlet regions on the detector can be used to measure the minimum signal and model the shape of the scattered light with a low order polynomial and subtract as part of the standard data reduction process. A Litthrow ghost, typical for VPH gratings used close to its Littrow configuration, affects HERMES data in all channels. The ghost images appear as small localized spots and fall spatially mirrored on the detector in a predictable manner forming the shape of the curved slit. The intensity of the ghost is at most 0.03% of the total flux in the originating fiber.

Figure 22. A test flat field exposure with some of the fibers masked to identify the ghost. 9.5 PSF variations and fiber cross talk The optical PSF varies across the detector both spatially and spectrally in all channels. At the spatial center of the detector, the PSF convolved with a fiber image is circular with a typical spectral FWHM of 3.5pix at the blue wavelength end of the detector increasing to ellipse-shaped PSF convolved with a fiber images with a typical FWHM of 5.0pix at the red wavelength end of the detector. At the spatial top and bottom regions of the detector the elliptical PSF convolved with a fiber image is inclined in opposite directions. As shown in figure 24 this pattern matches the optical design of the instrument.



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Figure 23. (Left) is an image of an arc exposure zoomed in the center of the detector in the HERMES Red channel. The PSF convolved with a fiber images are round and the PSF convolved with a fiber images for adjacent fibers don't overlap significantly. (Right) is an image of the same arc exposure zoomed in the top of the detector. The PSF convolved with a fiber image is now an inclined ellipse and the PSF convolved with a fiber images for adjacent fibers do partly overlap.

Figure 24. (Left) shows the measured fiber images for the blue camera at the center and edges of the field. (Right) shows the predicted (from Zemax) fiber images at the center and edges of the field. The most significant impact of this is on the fiber-to-fiber cross talk within each slitlet. The cross-talk level is such that 3-5% of flux from a fiber in the first and last 100 fibers affects its adjacent fibers. Given the limited hardware options to remove or reduce the observed cross talk, this level of crosstalk will require care during data reduction. Options include attempting to carry out deconvolution of contaminated spectra, which maybe computationally intensive to carry out in 2D, to hard-edge clipping the affected data, which would loosing signal but ensure minimal contamination.



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Figure 25. (Left) plots flux vs. pixel position for a vertical cut across a fiber flat field image, zoomed in the center of the detector in the HERMES Red channel. Note the flux going down to the bias level between the two slitlets, and the flux between the individual fibers goes down similarly. (Right) plots the vertical cut in the same fiber flat, zoomed in the top of the detector. Note here the flux between the two slitlets go down to bias level, but flux level between individual fibers does not, indicating there is illumination from the adjacent fibers. 9.6 HERMES Solar spectra A short 30sec exposure of the day time sky was observed with 2dF+HERMES. The resulting data were reduced and extracted. The data was processed thru the GALAH analysis pipeline and was found to be in good agreement with solar spectra from other high-resolution spectrographs VLT+UVES and Keck+HIRES.

Figure 26. shows the extracted and normalized solar spectra from the four HERMES channels 10. GALAH Survey update The primary science driver for the HERMES spectrograph is to carry out a large-scale Galactic Archaeology survey of the Milky Way[21]. The goal of Galactic Archaeology is to reconstruct the lost substructures of the proto-galaxy, thereby obtaining a detailed physical picture of the formation and evolution of the Milky Way. The GALAH (Galactic Archeology with HERMES) survey is designed to carry out this task using the chemical tagging technique as a means to exploit the vast chemical inventory of one million disk stars[22]. The GALAH survey is an Australian-led project with members from 8 Australian institutes and several key international partners.



GALAH fieldsMain : 73/3300

10.1 Pilot Survey The GALAH team conducted a Pilot Survey from November 2013 to January 2014, to test survey strategy as well as carry out extended tests that were not possible during formal HERMES commissioning. These data address questions such as quality of flat-field correction from the various lamp options, repeatability of targets between fibers and plates, acquisition and guiding dependence on input catalogue parameters and the overall stability of calibrations. GALAH observations have contributed a total of 56 hours to acquire HERMES test data. The Pilot Survey obtained spectra of ~13,000 individual science targets, including fundamental calibration stars, calibration open and globular star cluster fields and specific targeted science fields. These are used for testing the data reduction and analysis pipelines over the range of stellar parameters covered in the GALAH survey. 10.2 Observation summary The GALAH survey was granted 76 (includes the 10 extra nights) nights of observing time over the period of February 2014 to January 2015 for its main observing campaign. In the first 31 nights of the main survey, GALAH observed 23672 stars in 68 main survey fields, as well as the previously mentioned HERMES test data. The GALAH Analysis Pipeline (GAP) conducts the required bookkeeping of the observations, data reduction checks, radial velocity determination, continuum normalization, and operation of the spectrum synthesis determination of abundances. A series of papers outlining the survey goals, observational strategies and detailed pipeline processing are in preparation, expected to be online by late 2014.

Figure 27. The distribution across the sky of pilot survey (red), test (orange) and main survey (green) fields. Main survey fields that also serve as test data are shown as green circles with an orange ring. All 6546 potential survey fields are also shown as open circles; our goal of a million-star sample requires observing 3300 of these. The GALAH survey has set out challenging specifications that can only be met when the individual components meet their design specifications. The required signal to noise level is close to 100 with a 3600 second exposure time for a star of magnitude V14. The predicted performance of the spectrograph is regularly updated for the latest designs, as built geometries and for the measured (coating) performance.

10.3 Performance indicators

The first performance indicator is the total efficiency. In the figure below a “waterfall graph” shows the drop in the efficiency from telescope to detector. The VPH grating and the fiber cable show the significant drop in system efficiency. This graph is based on mainly measured efficiencies.



11. CONCLUSIONS The AAO has finished another very successful spectrograph, the HERMES spectrograph. The spectrograph is facilitating the GALAH Galactic Archeology survey, which is well on its way to achieve the goal of measuring abundances of 1,000,000 stars within the Milky Way. The instrument is performing to specification and the observations are proceeding smoothly. The only small concern is dealing with the a slight excess of cross-talk in the fibers at the edges of the field.

REFERENCES

[1] Barden, S. C., Jones, D. J., Barnes, S. I., Heijmans, J., et al., “HERMES: revisions in the design for a high resolution

multi-element spectrograph for the AAT”, Proc. SPIE 7735, 773509-773509-19 (2010).

[2] Barden, S., Bland Hawthorn, J., et al., “Concepts for a high-resolution multi-object spectrograph for galactic

archeology on the Anglo-Australian Telescope”, Proc. SPIE 7014, 70144J-70144J-12 (2008).

[3] Brzeski, J., Gers, L., “Hermes - the engineering challenges”, Proc. SPIE 8446-30 (2012)

[4] Heijmans, J.A.C., Gers, L., Faught, B., “Design and development of the high-resolution spectrograph HERMES and the unique volume phase holographic gratings”, Proc. SPIE 8167A-45 (2011)

[5] Waller, L, Barton, J, Mayfield, D, Griesbach, J, “AAO2: a general purpose CCD controller for the AAT”, Proc SPIE-5499-51, (2004)

[6] Case, S., Gers, L., Brezki, J., “Design and development of the fiber cable and fore optics of the HERMES spectrograph for the Anglo-Australian Telescope (AAT)”, Proc. SPIE 8125, 8125-03 (2011).

[7] Farrell, T.J., Shortridge, K., Bailey, J. A., “DRAMA – An environment for Instrumentation Software”, Bulletin of the AAS, Volume 25, No 2, (1993).

[8] Shortridge, K., Farrell, T.J., Bailey, J.A., Waller, L.G., “The Data Flow System for the AAO2 Controllers”, Proc. SPIE 5496, 463 (2004)

[9] Shortridge, K., Vuong, M. “Faking it for pleasure and profit: the use of hardware simulation at AAO”, Proc. SPIE 7740, 774008 (2010).

[10] Cannon R., “The calibration and spectrophotometric performance of 2dF”, AAO Newsletter Feb. 2000, pp.14-15

[11] Goodwin, M., Farrell, T., Smedley, S., Heald, R., Heijmans, J., De Silva, G., “The AAO Fiber Instrument Data Simulator,” Proc. SPIE 8446-84, (2012) in press.

[12] Goodwin, M., Smedley, S., Barnes, S., Farrell, T., Barden, S., “Data simulator for the HERMES instrument,” Proc. SPIE 7735, 77357U (2010).

[13] Sharp, R., Birchall, M. N., Optimal Extraction of Fiber Optic Spectroscopy, Publications of the Astronomical Society of Australia, Volume 27, Issue 1, pp. 91-103.

[14] Sharp, R., Hannah Parkinson, H., “Sky subtraction at the Poisson limit with fiber-optic multi-object spectroscopy”, MNRAS November 2010, Volume 408, Issue 4, pages 2495–2510,

[15] Arzoumanian, Z., Holmberg, J., Norman, B., “An Astronomical pattern-matching algorithm for computer-aided identification of whale sharks”, Journal of Applied Ecology 2005, 42, 991-1011.

[16] Dahl, J., et. al., “Algorithms and software for total variation image reconstruction via first-order methods”, Numer Algor, 53, 67-92, 2010

[17] Jay Kumler, Marc Neer, “Alignment technique for optical assemblies, <http://www.jenoptik.com/en-alignment-pip-generator>, Jenoptik Optical Systems



[18] Jessica R. Zheng, Luke Gers, Jeroen Heijmans, “Metrology measurements for large aperture VPH gratings”, Proc. SPIE 8838, Optical Manufacturing and Testing X, 88380G (2013).

[19] Jerone Heijmans, Luke Gers, Brendon Faught, “ Design and development of the high-resolution spectrograph HERMES and the unique holographic gratings:, Proc. SPIE 8167A – 45, (2010).

[20] Gers L., Staszak N., “The deterministic optical alignment of the HERMES spectrograph”, Paper to be presented at SPIE Montreal 2014.

[21] Freeman & Bland-Hawthorn, 2002, ARAA, 40, 487

[22] De Silva et al., 2007, AJ, 133, 1161

[23] Lewis et al, “The Anglo-Australian Observatory 2dF facility”, MNRAS (2002) 333 (2): 279-298.



PROCEEDINGS OF SPIE

Volume 9147

Proceedings of SPIE 0277-786X, V. 9147

SPIE is an international society advancing an interdisciplinary approach to the science and application of light.

Ground-based and Airborne Instrumentation for Astronomy V Suzanne K. Ramsay Ian S. McLean Hideki Takami Editors 22–26 June 2014 Montréal, Canada Sponsored by SPIE Cooperating Organizations American Astronomical Society (United States) • Australian Astronomical Observatory (Australia) • Association of Universities for Research in Astronomy (AURA) • Canadian Astronomical Society (CASCA) (Canada) • Canadian Space Agency (Canada) • European Astronomical Society (Switzerland) • European Southern Observatory (Germany) • National Radio Astronomy Observatory • Royal Astronomical Society (United Kingdom) • Science & Technology Facilities Council (United Kingdom) Published by SPIE

Part One of Five Parts

Ground-based and Airborne Instrumentation for Astronomy V, edited by Suzanne K. Ramsay, Ian S. McLean, Hideki Takami, Proc. of SPIE Vol. 9147,

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The papers included in this volume were part of the technical conference cited on the cover and title page. Papers were selected and subject to review by the editors and conference program committee. Some conference presentations may not be available for publication. The papers published in these proceedings reflect the work and thoughts of the authors and are published herein as submitted. The publisher is not responsible for the validity of the information or for any outcomes resulting from reliance thereon. Please use the following format to cite material from this book: Author(s), "Title of Paper," in Ground-based and Airborne Instrumentation for Astronomy V, edited by Suzanne K. Ramsay, Ian S. McLean, Hideki Takami, Proceedings of SPIE Vol. 9147 (SPIE, Bellingham, WA, 2014) Article CID Number. ISSN: 0277-786X ISBN: 9780819496157 Published by SPIE P.O. Box 10, Bellingham, Washington 98227-0010 USA Telephone +1 360 676 3290 (Pacific Time)· Fax +1 360 647 1445 SPIE.org Copyright © 2014, Society of Photo-Optical Instrumentation Engineers. Copying of material in this book for internal or personal use, or for the internal or personal use of specific clients, beyond the fair use provisions granted by the U.S. Copyright Law is authorized by SPIE subject to payment of copying fees. The Transactional Reporting Service base fee for this volume is $18.00 per article (or portion thereof), which should be paid directly to the Copyright Clearance Center (CCC), 222 Rosewood Drive, Danvers, MA 01923. Payment may also be made electronically through CCC Online at copyright.com. Other copying for republication, resale, advertising or promotion, or any form of systematic or multiple reproduction of any material in this book is prohibited except with permission in writing from the publisher. The CCC fee code is 0277-786X/14/$18.00. Printed in the United States of America. Publication of record for individual papers is online in the SPIE Digital Library.

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Contents Part One lxiii Conference Committee lxv Introduction SESSION 1 INSTRUMENT PROGRAMS AT MAJOR OBSERVATORIES

9147 02 Instrumentation at Gemini Observatory (Invited Paper) [9147-1] S. J. Kleinman, M. Boccas, S. J. Goodsell, P. Gomez, R. Murowinski, A.-N. Chené, D. Henderson, Gemini Observatory (United States) 9147 03 New developments in instrumentation at the W. M. Keck Observatory (Invited Paper) [9147-2] S. M. Adkins, T. E. Armandroff, W. M. Keck Observatory (United States); M. P. Fitzgerald, Univ.

of California, Los Angeles (United States); J. Johnson, W. M. Keck Observatory (United States); J. E. Larkin, Univ. of California, Los Angeles (United States); H. A. Lewis, W. M. Keck Observatory (United States); C. Martin, California Institute of Technology (United States);

K. Y. Matthews, Univ. of California, Los Angeles (United States); J. X. Prochaska, Univ. of California, Santa Cruz (United States); P. Wizinowich, W. M. Keck Observatory

(United States) 9147 04 Paranal instrumentation programme (Invited Paper) [9147-3] L. Pasquini, M. Casali, A. Russel, European Southern Observatory (Germany) 9147 05 An overview and the current status of instrumentation at the Large Binocular Telescope

Observatory (Invited Paper) [9147-4] R. M. Wagner, M. L. Edwards, O. Kuhn, D. Thompson, C. Veillet, Large Binocular Telescope

Observatory (United States) 9147 06 SOFIA science instruments: commissioning, upgrades and future opportunities [9147-5] E. C. Smith, NASA Ames Research Ctr. (United States); J. W. Miles, L. Helton, R. Sankrit, B. G. Andersson, E. E. Becklin, J. M. De Buizer, Universities Space Research Association

(United States); C. D. Dowell, Jet Propulsion Lab. (United States); E. W. Dunham, Lowell Observatory (United States); R. Güsten, Max-Planck-Institut für Radioastronomie (Germany); D. A. Harper, The Univ. of Chicago (United States); T. L. Herter, Cornell Univ. (United States); L. D. Keller, Ithaca College (United States); R. Klein, Universities Space Research Association (United States); A. Krabbe, Univ. Stuttgart (Germany); S. Logsdon, Univ. of California, Los Angeles (United States); P. M. Marcum, NASA Ames Research Ctr. (United States);

I. S. McLean, Univ. of California, Los Angeles (United States); W. T. Reach, Universities Space Research Association (United States); M. J. Richter, Univ. of California, Davis (United States); T. L. Roellig, NASA Ames Research Ctr. (United States); G. Sandell, M. L. Savage, Universities Space Research Association (United States); P. Temi, NASA Ames Research Ctr. (United States); W. D. Vacca, J. E. Vaillancourt, J. E. Van Cleve, E. T. Young, Universities Space Research Association (United States)

iii



9147 07 The Daniel K. Inouye Solar Telescope first light instruments and critical science plan [9147-6] D. F. Elmore, T. Rimmele, National Solar Observatory (United States); R. Casini, National Ctr.

for Atmospheric Research (United States); S. Hegwer, National Solar Observatory (United States); J. Kuhn, H. Lin, Institute for Astronomy, Univ. of Hawai'i (United States);

J. P. McMullin, K. Reardon, National Solar Observatory (United States); W. Schmidt, Kiepenheuer-Institut für Sonnenphysik (Germany); A. Tritschler, F. Wöger, National Solar Observatory (United States)

SESSION 2 NEW INSTRUMENTS AND UPGRADES TO EXISTING INSTRUMENTS

9147 09 Introducing CUBES: the Cassegrain U-band Brazil-ESO spectrograph [9147-8] P. Bristow, European Southern Observatory (Germany); B. Barbuy, Univ. de São Paulo

(Brazil); V. B. Macanhan, B. Castilho, Lab. Nacional de Astrofísica (Brazil); H. Dekker, B. Delabre, European Southern Observatory (Germany); M. Diaz, Univ. de São Paulo

(Brazil); C. Gneiding, Lab. Nacional de Astrofísica (Brazil); F. Kerber, H. Kuntschner, European Southern Observatory (Germany); G. La Mura, Univ. degli Studi di Padova (Italy); R. Reiss, J. Vernet, European Southern Observatory (Germany)

9147 0A LRS2: the new facility low resolution integral field spectrograph for the Hobby-Eberly

telescope [9147-9] T. S. Chonis, G. J. Hill, H. Lee, S. E. Tuttle, B. L. Vattiat, The Univ. of Texas at Austin (United

States) 9147 0B Project status of the Robert Stobie spectrograph near infrared instrument (RSS-NIR) for SALT

[9147-10] M. J. Wolf, M. P. Mulligan, M. P. Smith, D. P. Adler, C. M. Bartosz, M. A. Bershady, Univ. of

Wisconsin-Madison (United States); D. A. H. Buckley, South African Astronomical Observatory (South Africa); M. P. Burse, P. A. Chordia, Inter-Univ. Ctr. for Astronomy and Astrophysics (India); J. C. Clemens, The Univ. of North Carolina at Chapel Hill (United States); H. W. Epps, Lick Observatory, Univ. of California, Santa Cruz (United States);

K. Garot, B. L. Indahl, K. P. Jaehnig, Univ. of Wisconsin-Madison (United States); R. J. Koch, Diron Technologies, Inc. (United States); W. P. Mason, G. Mosby Jr., K. H. Nordsieck,

J. W. Percival, Univ. of Wisconsin-Madison (United States); S. Punnadi, A. N. Ramaprakash, Inter-Univ. Ctr. for Astronomy and Astrophysics (India); J. A. Schier, The Pilot Group (United States); A. I. Sheinis, Australian Astronomical Observatory (Australia); S. A. Smee, Johns Hopkins Univ. (United States); D. J. Thielman, M. W. Werner, Univ. of Wisconsin-Madison (United States); T. B. Williams, South African Astronomical Observatory (South Africa);

J. P. Wong, Paradigm Design Inc. (United States) 9147 0C VISIR upgrade overview and status [9147-11] F. Kerber, H. Käufl, European Southern Observatory (Germany); P. Baksai, European

Southern Observatory (Chile); N. Di Lieto, D. Dobrzycka, P. Duhoux, G. Finger, European Southern Observatory (Germany); S. Heikamp, Leiden Observatory (Netherlands); D. Ives, G. Jakob, L. Lundin, European Southern Observatory (Germany); D. Mawet, European Southern Observatory (Chile); L. Mehrgan, European Southern Observatory (Germany);

Y. Momany, European Southern Observatory (Chile); V. Moreau, E. Pantin, CEA-Ctr. de SACLAY (France); M. Riquelme, European Southern Observatory (Chile); S. Sandrock,

R. Siebenmorgen, A. Smette, J. Taylor, M. van den Ancker, European Southern Observatory (Germany); G. Valdes, European Southern Observatory (Chile); L. Venema, ASTRON (Netherlands); U. Weilenmann, European Southern Observatory (Chile)

iv



9147 0D The camera of the ASTRI SST-2M prototype for the Cherenkov Telescope Array [9147-12] O. Catalano, M. C. Maccarone, C. Gargano, G. La Rosa, A. Segreto, G. Sottile, INAF - Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo (Italy); V. De Caprio, INAF - Osservatorio Astronomico di Capodimonte (Italy); F. Russo, M. Capalbi, P. Sangiorgi,

INAF - Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo (Italy); G. Bonanno, A. Grillo, S. Garozzo, D. Marano, S. Billotta, G. Romeo, INAF - Osservatorio Astrofisico di

Catania (Italy); L. Stringhetti, M. Fiorini, N. La Palombara, S. Incorvaia, G. Toso, INAF - IASF Milano (Italy); D. Impiombato, S. Giarrusso, INAF - Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo (Italy)

9147 0E A two-dimensional spectropolarimeter as a first-light instrument for the Daniel K. Inouye

Solar Telescope [9147-13] W. Schmidt, A. Bell, C. Halbgewachs, F. Heidecke, T. J. Kentischer, O. von der Lühe, T. Scheiffelen, M. Sigwarth, Kiepenheuer-Institut für Sonnenphysik (Germany) 9147 0F Performance of polarization modulation and calibration optics for the Daniel K. Inouye

Solar Telescope [9147-14] D. F. Elmore, National Solar Observatory (United States); S. R. Sueoka, College of Optical

Sciences, The Univ. of Arizona (United States); R. Casini, National Ctr. for Atmospheric Research (United States)

9147 0G KIDSpec: an MKID based medium resolution integral field spectrograph [9147-332] K. O'Brien, N. Thatte, Univ. of Oxford (United Kingdom); B. Mazin, Univ. of California, Santa

Barbara (United States) 9147 0H HIPO in-flight performance improvements [9147-16] E. W. Dunham, T. A. Bida, P. L. Collins, G. Mandushev, S. Zoonematkermani, Lowell

Observatory (United States); J. Van Cleve, Universities Space Research Association (United States); D. Angerhausen, Rensselaer Polytechnic Institute (United States); A. Mandell, NASA Goddard Space Flight Ctr. (United States)

9147 0J A near-infrared SETI experiment: instrument overview [9147-18] S. A. Wright, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada)

and Univ. of Toronto (Canada); D. Werthimer, Univ. of California, Berkeley (United States); R. R. Treffers, Starman Systems, LLC (United States); J. Maire, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada); G. W. Marcy, Univ. of California, Berkeley (United States); R. P. S. Stone, Lick Observatory, Univ. of California, Santa Cruz (United States); F. Drake, SETI Institute (United States); E. Meyer, P. Dorval, Univ. of Toronto (Canada); A. Siemion, Univ. of California, Berkeley (United States)

SESSION 3 HIGH MULTIPLEX AND SURVEY INSTRUMENTS I

9147 0L Project overview and update on WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope [9147-20]

G. Dalton, STFC Rutherford Appleton Lab. (United Kingdom) and Univ. of Oxford (United Kingdom); S. Trager, Univ. of Groningen (Netherlands); D. C. Abrams, Isaac Newton Group of Telescopes (Spain); P. Bonifacio, GEPI, Observatoire de Paris à Meudon (France);

J. A. L. Aguerri, Instituto de Astrofísica de Canarias (Spain); K. Middleton, STFC Rutherford Appleton Lab. (United Kingdom); C. Benn, K. Dee, Isaac Newton Group of Telescopes (Spain); F. Sayède, GEPI, Observatoire de Paris à Meudon (France); I. Lewis, Univ. of Oxford (United Kingdom); J. Pragt, NOVA ASTRON (Netherlands); S. Pico, Isaac Newton Group of

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Telescopes (Spain); N. Walton, Institute of Astronomy, Univ. of Cambridge (United Kingdom); J. Rey, Isaac Newton Group of Telescopes (Spain); C. Allende Prieto, J. Peñate, Instituto de Astrofísica de Canarias (Spain); E. Lhome, Isaac Newton Group of Telescopes (Spain); T. Agócs, NOVA ASTRON (Netherlands); J. Alonso, Instituto de Astrofisica de Canarias (Spain); D. Terrett, STFC Rutherford Appleton Lab. (United Kingdom); M. Brock,

J. Gilbert, Univ. of Oxford (United Kingdom); A. Ridings, Isaac Newton Group of Telescopes (Spain); I. Guinouard, GEPI, Observatoire de Paris à Meudon (France); M. Verheijen, Univ. of Groningen (Netherlands); I. Tosh, K. Rogers, STFC Rutherford Appleton Lab. (United Kingdom); I. Steele, Liverpool John Moores Univ. (United Kingdom); R. Stuik, N. Tromp, NOVA ASTRON (Netherlands); A. Jasko, Konkoly Observatory (Hungary); J. Kragt,

D. Lesman, NOVA ASTRON (Netherlands); C. Mottram, S. Bates, Liverpool John Moores Univ. (United Kingdom); F. Gribbin, Isaac Newton Group of Telescopes (Spain); L. F. Rodriguez,

J. M. Delgado, Instituto de Astrofísica de Canarias (Spain); C. Martin, D. Cano, Isaac Newton Group of Telescopes (Spain); R. Navarro, NOVA ASTRON (Netherlands); M. Irwin,

J. Lewis, E. Gonzalez Solares, Institute of Astronomy, Univ. of Cambridge (United Kingdom); N. O'Mahony, Isaac Newton Group of Telescopes (Spain); A. Bianco, INAF - Osservatorio Astronomico di Brera (Italy); C. Zurita, Instituto de Astrofisica de Canarias (Spain);

R. ter Horst, NOVA ASTRON (Netherlands); E. Molinari, M. Lodi, J. Guerra, INAF - Fundación Galileo Galilei (Spain); A. Vallenari, A. Baruffolo, INAF - Osservatorio Astronomico di Padova (Italy)

9147 0M 4MOST: 4-metre Multi-Object Spectroscopic Telescope [9147-21] R. S. de Jong, S. Barden, O. Bellido-Tirado, J. Brynnel, C. Chiappini, É. Depagne, R. Haynes,

D. Johl, D. P. Phillips, O. Schnurr, A. D. Schwope, J. Walcher, S. M. Bauer, G. Cescutti, M. R. Cioni, F. Dionies, H. Enke, Leibniz-Institut für Astrophysik Potsdam (Germany);

D. Haynes, Leibniz-Institut für Astrophysik Potsdam (Germany) and InnoFSPEC (Germany); A. Kelz, F. S. Kitaura, G. Lamer, I. Minchev, V. Müller, S. E. Nuza, Leibniz-Institut für Astrophysik Potsdam (Germany); J.-C. Olaya, Leibniz-Institut für Astrophysik Potsdam (Germany) and InnoFSPEC (Germany); T. Piffl, E. Popow, A. Saviauk, M. Steinmetz, U. Ural, M. Valentini, R. Winkler, L. Wisotzki, Leibniz-Institut für Astrophysik Potsdam (Germany); W. R. Ansorge, RAMS-CON Management Consultants (Germany); M. Banerji, E. Gonzalez Solares, M. Irwin, R. C. Kennicutt Jr., D. P. King, R. McMahon, S. Koposov, I. R. Parry, X. Sun, N. A. Walton, Univ. of Cambridge (United Kingdom); G. Finger, O. Iwert, M. Krumpe, J.-L. Lizon, V. Mainieri, European Southern Observatory (Germany); J.-P. Amans, P. Bonifacio, M. Cohen, P. François, P. Jagourel, S. B. Mignot, F. Royer, P. Sartoretti, GEPI, Observatoire de Paris à Meudon, CNRS, Univ. Paris Diderot (France); R. Bender, H.-J. Hess, F. Lang-Bardl, B. Muschielok, J. Schlichter, Univ.-Sternwarte München (Germany); H. Böhringer, T. Boller, A. Bongiorno, M. Brusa, T. Dwelly, A. Merloni, K. Nandra, M. Salvato, Max-Planck-Institut für extraterrestrische Physik (Germany); J. H. Pragt, R. Navarro, G. Gerlofsma, R. Roelfsema, NOVA ASTRON (Netherlands); G. B. Dalton, Rutherford Appleton Lab. (United Kingdom) and Univ. of Oxford (United Kingdom); K. F. Middleton, I. A. Tosh, Rutherford Appleton Lab. (United Kingdom); C. Boeche, E. Caffau, N. Christlieb, E. K. Grebel, C. J. Hansen, A. Koch, H.-G. Ludwig, H. Mandel, A. Quirrenbach, L. Sbordone, W. Seifert, G. Thimm, Zentrum für Astronomie der Univ. Heidelberg (Germany); A. Helmi, S. C. trager, Kapteyn Astronomical Institute (Netherlands); T. Bensby, S. Feltzing, G. Ruchti, Lund Univ. (Sweden); B. Edvardsson, A. Korn, K. Lind, Uppsala Univ. (Sweden); W. Boland, NOVA (Netherlands); M. Colless, Australian Astronomical Observatory (Australia) and Australian National Univ. (Australia); G. Frost, J. Gilbert, P. Gillingham, J. Lawrence, N. Legg, W. Saunders, A. Sheinis, Australian Astronomical Observatory (Australia); S. Driver, A. Robotham, Univ. of Western Australia (Australia); R. Bacon, P. Caillier, J. Kosmalski, F. Laurent, J. Richard, Ctr. de Recherche Astrophysique de Lyon (France)

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9147 0N MOONS: the Multi-Object Optical and Near-infrared Spectrograph for the VLT [9147-22] M. Cirasuolo, UK Astronomy Technology Ctr. (United Kingdom) and Institute for Astronomy,

Univ. of Edinburgh (United Kingdom); J. Afonso, Observatorio Astronomico de Lisboa (Portugal); M. Carollo, ETH Zürich (Switzerland); H. Flores, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); R. Maiolino, Univ. of Cambridge (United Kingdom); E. Oliva, INAF - Osservatorio Astrofisico di Arcetri (Italy); S. Paltani, Univ. of Genève (Switzerland);

L. Vanzi, Pontificia Univ. Católica de Chile (Chile); C. Evans, UK Astronomy Technology Ctr. (United Kingdom); M. Abreu, Univ. de Lisboa (Portugal); D. Atkinson, UK Astronomy Technology Ctr. (United Kingdom); C. Babusiaux, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); S. Beard, UK Astronomy Technology Ctr. (United Kingdom); F. Bauer, Pontificia Univ. Católica de Chile (Chile); M. Bellazzini, Univ. degli Studi di Bologna (Italy); R. Bender, Univ.-Sternwarte München (Germany) and Max-Planck-Institut für extraterrestrische Physik (Germany); P. Best, Institute for Astronomy, Univ. of Edinburgh (United Kingdom); N. Bezawada, UK Astronomy Technology Ctr. (United Kingdom); P. Bonifacio, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); A. Bragaglia, INAF - Osservatorio Astronomico di Bologna (Italy); I. Bryson, UK Astronomy Technology Ctr. (United Kingdom); D. Busher, Univ. of Cambridge (United Kingdom); A. Cabral, Univ. de Lisboa (Portugal); K. Caputi, Institute for Astronomy, Univ. of Edinburgh (United Kingdom); M. Centrone, INAF - Osservatorio Astronomico di Roma (Italy); F. Chemla, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); A. Cimatti, Univ. degli Studi di Bologna (Italy); M.-R. Cioni, Univ. of Hertfordshire (United Kingdom); G. Clementini, INAF - Osservatorio Astronomico di Bologna (Italy); J. Coelho, Univ. de Lisboa (Portugal); D. Crnojevic, Institute for Astronomy, Univ. of Edinburgh (United Kingdom); E. Daddi, CEA-Ctr. de SACLAY (France); J. Dunlop, Institute for Astronomy, Univ. of Edinburgh (United Kingdom); S. Eales, Cardiff Univ. (United Kingdom); S. Feltzing, Lund Observatory (Sweden); A. Ferguson, Institute for Astronomy, Univ. of Edinburgh (United Kingdom); M. Fisher, Univ. of Cambridge (United Kingdom); A. Fontana, INAF - Osservatorio Astronomico di Roma (Italy); J. Fynbo, Dark Cosmology Ctr. (Denmark); B. Garilli, INAF - IASF Milano (Italy); G. Gilmore, Univ. of Cambridge (United Kingdom); A. Glauser, ETH Zürich (Switzerland); I. Guinouard, F. Hammer, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); P. Hastings, UK Astronomy Technology Ctr. (United Kingdom); A. Hess, Univ.-Sternwarte München (Germany); R. Ivison, UK Astronomy Technology Ctr. (United Kingdom); P. Jagourel, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); M. Jarvis, Oxford Univ. (United Kingdom); L. Kaper, Astronomical Institute Anton Pannekoer (Netherlands); G. Kauffman, Max-Planck-Institut für Astrophysik (Germany); A. T. Kitching, Univ. College London (United Kingdom); A. Lawrence, Institute for Astronomy, Univ. of Edinburgh (United Kingdom); D. Lee, UK Astronomy Technology Ctr. (United Kingdom); B. Lemasle, Astronomical Institute Anton Pannekoer (Netherlands); G. Licausi, INAF - Osservatorio Astronomico di Roma (Italy); S. Lilly, ETH Zürich (Switzerland); D. Lorenzetti, INAF - Osservatorio Astronomico di Roma (Italy); D. Lunney, UK Astronomy Technology Ctr. (United Kingdom); R. Maiolino, Univ. of Cambridge (United Kingdom); F. Mannucci, INAF - Osservatorio Astrofisico di Arcetri (Italy); R. McLure, Institute for Astronomy, Univ. of Edinburgh (United Kingdom); D. Minniti, Pontificia Univ. Católica de Chile (Chile); D. Montgomery, UK Astronomy Technology Ctr. (United Kingdom); B. Muschielok, Univ.-Sternwarte München (Germany); K. Nandra, Max-Planck-Institut für extraterrestrische Physik (Germany); R. Navarro, NOVA ASTRON (The Netherlands); P. Norberg, Durham Univ. (United Kingdom); S. Oliver, Univ. of Sussex (United Kingdom); L. Origlia, INAF - Osservatorio Astronomico di Bologna (Italy); N. Padilla, Pontificia Univ. Católica de Chile (Chile); J. Peacock, Institute for Astronomy, Univ. of Edinburgh (United Kingdom); F. Pedicini, INAF - Osservatorio Astronomico di Roma (Italy); J. Peng, Univ. of Cambridge (United Kingdom); L. Pentericci, INAF - Osservatorio Astronomico di Roma (Italy); J. Pragt, NOVA ASTRON (Netherlands); M. Puech, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); S. Randich, INAF - Osservatorio

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Astrofisico di Arcetri (Italy); P. Rees, UK Astronomy Technology Ctr. (United Kingdom); A. Renzini, INAF - Osservatorio Astronomico di Padova (Italy); N. Ryde, Lund Observatory (Sweden); M. Rodrigues, European Southern Observatory (Chile); I. Roseboom, Institute for Astronomy, Univ. of Edinburgh (United Kingdom); F. Royer, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); R. Saglia, Univ.-Sternwarte München (Germany) and Max-Planck-Institut für extraterrestrische Physik (Germany); A. Sanchez, Max-Planck-Institut für extraterrestrische Physik (Germany); R. Schiavon, Liverpool John Moores Univ. (United Kingdom); H. Schnetler, UK Astronomy Technology Ctr. (United Kingdom); D. Sobral, Institute for Astronomy, Univ. of Edinburgh (United Kingdom); R. Speziali, INAF - Osservatorio Astronomico di Roma (Italy); D. Sun, Univ. of Cambridge (United Kingdom); R. Stuik, NOVA ASTRON (Netherlands); A. Taylor, Institute for Astronomy, Univ. of Edinburgh (United Kingdom); W. Taylor, S. Todd, UK Astronomy Technology Ctr. (United Kingdom); E. Tolstoy, Kapteyn Astronomical Institute (Netherlands); M. Torres, Pontificia Univ. Católica de Chile (Chile); M. Tosi, E. Vanzella, INAF - Osservatorio Astronomico di Bologna (Italy); L. Venema, Kapteyn Astronomical Institute (Netherlands); F. Vitali, INAF - Osservatorio Astronomico di Roma (Italy); M. Wegner, Univ.-Sternwarte München (Germany); M. Wells, UK Astronomy Technology Ctr. (United Kingdom); V. Wild, St. Andrews Univ. (United Kingdom); G. Wright, UK Astronomy Technology Ctr. (United Kingdom); G. Zamorani, INAF - Osservatorio Astronomico di Bologna (Italy); M. Zoccali, Pontificia Univ. Católica de Chile (Chile)

9147 0O MEGARA: a new generation optical spectrograph for GTC [9147-23] A. Gil de Paz, J. Gallego, Univ. Complutense de Madrid (Spain); E. Carrasco, Instituto

Nacional de Astrofísica, Óptica y Electrónica (Mexico); J. Iglesias-Páramo, Instituto de Astrofísica de Andalucía (Spain); R. Cedazo, Univ. Politécnica de Madrid (Spain);

J. M. Vílchez, Instituto de Astrofísica de Andalucía (Spain); M. L. García-Vargas, FRACTAL S.L.N.E (Spain); X. Arrillaga, M. A. Carrera, Added Value Solutions SL (Spain);

A. Castillo-Morales, Univ. Complutense de Madrid (Spain); E. Castillo-Domínguez, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico); M. C. Eliche-Moral, Univ. Complutense de Madrid (Spain); D. Ferrusca, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico); E. González-Guardia, Univ. Politécnica de Madrid (Spain); B. Lefort, M. Maldonado, FRACTAL S.L.N.E (Spain); R. A. Marino, Univ. Complutense de Madrid (Spain); I. Martínez-Delgado, FRACTAL S.L.N.E (Spain); I. Morales Durán, Instituto de Astrofísica de Andalucía (Spain); E. Mujica, FRACTAL S.L.N.E (Spain); G. Páez, Ctr. de Investigaciones en Óptica (Mexico); S. Pascual, Univ. Complutense de Madrid (Spain);

A. Pérez-Calpena, FRACTAL S.L.N.E (Spain); A. Sánchez-Penim, Univ. Complutense de Madrid (Spain); E. Sánchez-Blanco, S. Tulloch, FRACTAL S.L.N.E (Spain); M. Velázquez, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico); J. Zamorano, Univ. Complutense de Madrid (Spain); A. L. Aguerri, Instituto de Astrofísica de Canarias (Spain) and Univ. de La Laguna (Spain); D. Barrado y Naváscues, Ctr. de Astrobiología (Spain);

E. Bertone, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico); N. Cardiel, Univ. Complutense de Madrid (Spain); A. Cava, Univ. of Genève (Switzerland); J. Cenarro, Ctr. de Estudios de Física del Cosmos de Aragón (Spain); M. Chávez, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico); M. García, Ctr. de Astrobiología (Spain);

J. Guichard, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico); R. Gúzman, Univ. of Florida (United States); A. Herrero, Instituto de Astrofísica de Canarias (Spain) and Univ. de La Laguna (Spain); N. Huélamo, Ctr. de Astrobiología (Spain); D. Hughes, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico); J. Jiménez-Vicente, Univ. de Granada (Spain); C. Kehrig, I. Márquez, J. Masegosa, Instituto de Astrofísica de Andalucía (Spain); Y. D. Mayya, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico);

J. Méndez-Abreu, Univ. of St. Andrews (United Kingdom); M. Mollá, CIEMAT (Spain); C. Muñoz-Tuñón, Instituto de Astrofísica de Canarias (Spain) and Univ. de La Laguna

(Spain); M. Peimbert, Univ. Autónoma de México (Mexico); P. G. Pérez-González, Univ.

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Complutense de Madrid (Spain); E. Pérez Montero, Instituto de Astrofísica de Andalucía (Spain); M. Rodríguez, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico);

J. M. Rodríguez-Espinosa, Instituto de Astrofísica de Canarias (Spain) and Univ. de La Laguna (Spain); L. Rodríguez-Merino, D. Rosa-González, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico); J. Sánchez-Almeida, Instituto de Astrofísica de Canarias (Spain) and Univ. de La Laguna (Spain); C. Sánchez Contreras, Ctr. de Astrobiología (Spain); P. Sánchez-Blázquez, Univ. Autónoma de Madrid (Spain); F. M. Sánchez Moreno, Univ. Politécnica de Madrid (Spain); S. F. Sánchez, Univ. Autónoma de México (Mexico);

A. Sarajedini, Univ. of Florida (United States); F. Serena, Univ. Politécnica de Madrid (Spain); S. Silich, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico); S. Simón-Díaz, Instituto de Astrofísica de Canarias (Spain) and Univ. de La Laguna (Spain);

G. Tenorio-Tagle, E. Terlevich, R. Terlevich, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico); S. Torres-Peimbert, Univ. Autónoma de México (Mexico); I. Trujillo, Instituto de Astrofísica de Canarias (Spain) and Univ. de La Laguna (Spain); Y. Tsamis, Open Univ. (United Kingdom); O. Vega, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico); V. Villar, Univ. Complutense de Madrid (Spain)

SESSION 4 HIGH MULTIPLEX AND SURVEY INSTRUMENTS II

9147 0P The WIYN one degree imager 2014: performance of the partially populated focal plane and instrument upgrade path [9147-24]

D. R. Harbeck, WIYN Observatory (United States); T. Boroson, National Optical Astronomy Observatory (United States) and Las Cumbres Observatory Global Telescope Network (United States); M. Lesser, The Univ. of Arizona (United States); J. Rajagopal, National Optical Astronomy Observatory (United States); A. Yeatts, WIYN Observatory (United States); C. Corson, National Optical Astronomy Observatory (United States); W. Liu, WIYN Observatory (United States); I. Dell'Antonio, Brown Univ. (United States); R. Kotulla, Univ. of Wisconsin-Milwaukee (United States) and Univ. of Wisconsin-Madison (United States);

D. Ouellette, The Univ. of Arizona (United States); E. Hooper, WIYN Observatory (United States) and Univ. of Wisconsin-Madison (United States); M. Smith, Univ. of Wisconsin-Madison (United States); R. Bredthauer, Semiconductor Technology Associates, Inc. (United States); P. Martin, Univ. of Hawai'i at Hilo (United States); G. Muller, GMTO Corp. (United States); P. Knezek, National Science Foundation (United States); M. Hunten, Lunar and Planetary Science Lab. (United States)

9147 0Q VIRUS: production and deployment of a massively replicated fiber integral field

spectrograph for the upgraded Hobby-Eberly Telescope [9147-25] G. J. Hill, McDonald Observatory, The Univ. of Texas at Austin (United States) and The Univ.

of Texas at Austin (United States); S. E. Tuttle, N. Drory, H. Lee, B. L. Vattiat, McDonald Observatory, The Univ. of Texas at Austin (United States); D. L. DePoy, J. L. Marshall, Texas A&M Univ. (United States); A. Kelz, D. Haynes, Leibniz-Institut für Astrophysik Potsdam (Germany) and innoFSPEC Potsdam (Germany); M. H. Fabricius, Max-Planck-Institut für extraterrestrische Physik (Germany); K. Gebhardt, The Univ. of Texas at Austin (United States); R. D. Allen, Texas A&M Univ. (United States); H. Anwad, Institut für Astrophysik Göttingen (Germany); R. Bender, Max-Planck Institut für extraterrestrische Physik (Germany) and Univ.-Sternwarte München (Germany); G. Blanc, Carnegie Observatories (United States); T. Chonis, The Univ. of Texas at Austin (United States); M. E. Cornell, MIT Lincoln Lab. (United States); G. Dalton, Univ. of Oxford (United Kingdom); J. Good, McDonald Observatory, The Univ. of Texas at Austin (United States); T. Jahn, Leibniz-Institut für Astrophysik Potsdam (Germany) and innoFSPEC Potsdam (Germany); H. Kriel, M. Landriau, P. J. MacQueen, McDonald Observatory, The Univ. of Texas at Austin (United

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States); J. D. Murphy, Princeton Univ. (United States); T. W. Peterson, McDonald Observatory, The Univ. of Texas at Austin (United States); T. Prochaska, Texas A&M Univ. (United States); H. Nicklas, Institut für Astrophysik Göttingen (Germany); J. Ramsey, McDonald Observatory, The Univ. of Texas at Austin (United States); M. M. Roth, Leibniz-Institut für Astrophysik Potsdam (Germany) and innoFSPEC Potsdam (Germany);

R. D. Savage, McDonald Observatory, The Univ. of Texas at Austin (United States); J. Snigula, Max-Planck-Institut für extraterrestrische Physik (Germany) 9147 0R The construction, alignment, and installation of the VIRUS spectrograph [9147-26] S. E. Tuttle, G. J. Hill, H. Lee, B. Vattiat, E. Noyola, N. Drory, M. Cornell, T. Peterson, T. Chonis,

McDonald Observatory, The Univ. of Texas at Austin (United States); R. Allen, Texas A&M Univ. (United States); G. Dalton, Univ. of Oxford (United Kingdom); D. DePoy, Texas A&M Univ. (United States); D. Edmonston, McDonald Observatory, The Univ. of Texas at Austin (United States); M. Fabricius, Max-Planck-Institut für extraterrestrische Physik (Germany);

D. Haynes, A. Kelz, Leibniz-Institut für Astrophysik Potsdam (Germany); M. Landriau, McDonald Observatory, The Univ. of Texas at Austin (United States); M. Lesser, The Univ. of Arizona Imaging Technology Lab. (United States); B. Leach, Astronomical Research Cameras, Inc. (United States); J. Marshall, Texas A&M Univ. (United States); J. Murphy,

D. Perry, McDonald Observatory, The Univ. of Texas at Austin (United States); T. Prochaska, Texas A&M Univ. (United States); J. Ramsey, R. Savage, McDonald Observatory, The Univ. of Texas at Austin

9147 0S The Dark Energy Spectroscopic Instrument (DESI) [9147-27] B. Flaugher, Fermi National Accelerator Lab. (United States); C. Bebek, Lawrence Berkeley

National Lab. (United States) 9147 0T Progress with the Prime Focus Spectrograph for the Subaru Telescope: a massively

multiplexed optical and near-infrared fiber spectrograph [9147-28] H. Sugai, N. Tamura, H. Karoji, A. Shimono, Kavli Institute for the Physics and Mathematics of

the Universe, The Univ. of Tokyo (Japan); N. Takato, Subaru Telescope, National Astronomical Observatory of Japan (United States); M. Kimura, Y. Ohyama, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan); A. Ueda, National Astronomical Observatory of Japan (Japan); H. Aghazarian, Jet Propulsion Lab. (United States);

M. V. de Arruda, Lab. Nacional de Astrofísica (Brazil); R. H. Barkhouser, C. L. Bennett, Johns Hopkins Univ. (United States); S. Bickerton, Kavli Institute for the Physics and Mathematics of the Universe, The Univ. of Tokyo (Japan); A. Bozier, Aix-Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); D. F. Braun, Jet Propulsion Lab. (United States);

K. Bui, California Institute of Technology (United States); C. M. Capocasale, Jet Propulsion Lab. (United States); M. A. Carr, Princeton Univ. (United States); B. Castilho, Lab. Nacional de Astrofísica (Brazil); Y.-C. Chang, H.-Y. Chen, R. C. Y. Chou, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan); O. R. Dawson, Jet Propulsion Lab. (United States); R. G. Dekany, Caltech Optical Observatories (United States); E. M. Ek, Jet Propulsion Lab. (United States); R. S. Ellis, California Institute of Technology (United States); R. J. English, Jet Propulsion Lab. (United States); D. Ferrand, Aix-Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); D. Ferreira, Lab. Nacional de Astrofísica (Brazil); C. D. Fisher, Jet Propulsion Lab. (United States); M. Golebiowski, Aix-Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); J. E. Gunn, Princeton Univ. (United States); M. Hart,

T. M. Heckman, Johns Hopkins Univ. (United States); P. T. P. Ho, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan); S. Hope, Johns Hopkins Univ. (United States);

L. E. Hovland, Jet Propulsion Lab. (United States); S.-F. Hsu, Y.-S. Hu, P. J. Huang, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan); M. Jaquet, Aix-Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); J. E. Karr, Institute of Astronomy and

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Astrophysics, Academia Sinica (Taiwan); J. G. Kempenaar, M. E. King, Jet Propulsion Lab. (United States); O. Le Fèvre, D. Le Mignant, Aix-Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); H.-H. Ling, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan); C. Loomis, R. H. Lupton, Princeton Univ. (United States); F. Madec, Aix-Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); P. Mao, California Institute of Technology (United States); L. S. Marrara, Lab. Nacional de Astrofísica (Brazil); B. Ménard, Johns Hopkins Univ. (United States); C. Morantz, Jet Propulsion Lab. (United States);

H. Murayama, Kavli Institute for the Physics and Mathematics of the Universe, The Univ. of Tokyo (Japan); G. J. Murray, Durham Univ. (United Kingdom); A. C. de Oliveira, Lab. Nacional de Astrofísica (Brazil); C. M. de Oliveira, Univ. de São Paulo (Brazil);

L. S. de Oliveira, Lab. Nacional de Astrofísica (Brazil); J. D. Orndorff, Johns Hopkins Univ. (United States); R. de Paiva Vilaça, Lab. Nacional de Astrofísica (Brazil); E. J. Partos, Jet Propulsion Lab. (United States); S. Pascal, T. Pegot-Ogier, Aix-Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); D. J. Reiley, R. Riddle, California Institute of Technology (United States); L. Santos, J. B. dos Santos, Lab. Nacional de Astrofísica (Brazil); M. A. Schwochert, Jet Propulsion Lab. (United States); M. D. Seiffert, Jet Propulsion Lab. (United States) and California Institute of Technology (United States); S. A. Smee, Johns Hopkins Univ. (United States); R. M. Smith, Caltech Optical Observatories (United States);

R. E. Steinkraus, Jet Propulsion Lab. (United States); L. Sodré Jr., Univ. de São Paulo (Brazil); D. N. Spergel, Princeton Univ. (United States); C. Surace, L. Tresse, C. Vidal, S. Vives, Aix-Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); S.-Y. Wang, C.-Y. Wen, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan); A. C. Wu, Jet Propulsion Lab. (United States); R. Wyse, Johns Hopkins Univ. (United States); C.-H. Yan, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan)

9147 0U Results of the verification of the NIR MOS EMIR [9147-29] F. Garzón, Instituto de Astrofísica de Canarias (Spain) and Univ. de La Laguna (Spain); N. Castro-Rodríguez, M. Insausti, L. López-Martín, Instituto de Astrofísica de Canarias

(Spain); P. Hammersley, Univ. de La Laguna (Spain); M. Barreto, P. Fernández, E. Joven, P. López, A. Mato, H. Moreno, M. Núñez, J. Patrón, J. L. Rasilla, P. Redondo, J. Rosich, Instituto de Astrofísica de Canarias (Spain); S. Pascual, European Southern Observatory (Germany); R. Grange, Lab. d'Astrophysique Marseille, CNRS (France)

9147 0V DOTIFS: a new multi-IFU optical spectrograph for the 3.6-m Devasthal optical telescope

[9147-270] H. Chung, Seoul National Univ. (Korea, Republic of) and Korea Institute for Advanced

Study (Korea, Republic of); A. N. Ramaprakash, Inter-Univ. Ctr. for Astronomy and Astrophysics (India); A. Omar, Aryabhatta Research Institute of Observational Sciences (India); S. Ravindranath, S. Chattopadhyay, C. V. Rajarshi, P. Khodade, Inter-Univ. Ctr. for Astronomy and Astrophysics (India)

9147 0W Performance of the K-band multi-object spectrograph (KMOS) on the ESO VLT [9147-31] R. Sharples, Durham Univ. (United Kingdom); R. Bender, Univ.-Sternwarte München

(Germany) and Max-Planck-Institut für extraterrestrische Physik (Germany); A. Agudo Berbel, Max-Planck-Institut für extraterrestrische Physik (Germany); R. Bennett, N. Bezawada, UK Astronomy Technology Ctr. (United Kingdom); R. Castillo, European

Southern Observatory (Germany); M. Cirasuolo, UK Astronomy Technology Ctr. (United Kingdom); P. Clark, Durham Univ. (United Kingdom); G. Davidson, UK Astronomy Technology Ctr. (United Kingdom); R. Davies, Max-Planck-Institut für extraterrestrische Physik (Germany); R. Davies, Univ. of Oxford (United Kingdom); M. Dubbeldam, Durham Univ. (United Kingdom); A. Fairley, UK Astronomy Technology Ctr. (United Kingdom);

G. Finger, European Southern Observatory (Germany); N. F. Schreiber, R. Genzel,

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Max-Planck-Institut für extraterrestrische Physik (Germany); R. Haefner, A. Hess, Univ.-Sternwarte München (Germany); I. Jung, European Southern Observatory

(Germany); I. Lewis, Univ. of Oxford (United Kingdom); D. Montgomery, J. Murray, UK Astronomy Technology Ctr. (United Kingdom); B. Muschielok, Univ.-Sternwarte München

(Germany); J. Pirard, S. Ramsey, European Southern Observatory (Germany); P. Rees, UK Astronomy Technology Ctr. (United Kingdom); J. Richter, Univ.-Sternwarte München (Germany); D. Robertson, Durham Univ. (United Kingdom); I. Robson, UK Astronomy Technology Ctr. (United Kingdom); S. Rolt, Durham Univ. (United Kingdom); R. Saglia,

Univ.-Sternwarte München (Germany); I. Saviane, European Southern Observatory (Germany); J. Schlichter, Univ.-Sternwarte München (Germany); L. Schmidtobreik,

A. Segovia, A. Smette, European Southern Observatory (Germany); M. Tecza, Univ. of Oxford (United Kingdom); S. Todd, UK Astronomy Technology Ctr. (United Kingdom);

M. Wegner, Univ.-Sternwarte München (Germany); E. Wiezorrek, Max-Planck-Institut für extraterrestrische Physik (Germany)

9147 0X Demonstration of high-performance cryogenic probe arms for deployable IFUs [9147-32] S. S. Eikenberry, C. H. Murphey, S. A. Mullin, J. G. Bennett, S. N. Raines, K. Ackley, R. D. Stelter, A. Garner, Univ. of Florida (United States); J. Sabater, Univ. de Barcelona

(Spain); S. A. Eikenberry, Eastside High School (United States); B. Chinn, H. V. Donoso, C. S. Vega, Univ. of Florida (United States); J. M. Gómez, J. Torra, Univ. de Barcelona

(Spain); M. D. Herlevich, R. Frommeyer, P. Miller, Univ. of Florida (United States) 9147 0Y First light results from the Hermes spectrograph at the AAT [9147-33] A. Sheinis, Australian Astronomical Observatory (Australia) and The Univ. of Sydney

(Australia); S. Barden, Leibniz-Institut für Astrophysik Potsdam (Germany); M. Birchall, Australian Astronomical Observatory (Australia); D. Carollo, Macquarie Univ. (Australia);

J. Bland-Hawthorn, The Univ. of Sydney (Australia); J. Brzeski, S. Case, R. Cannon, V. Churilov, W. Couch, R. Dean, G. De Silva, Australian Astronomical Observatory

(Australia); V. D'Orazi, Macquarie Univ. (Australia); T. Farrell, K. Fiegert, Australian Astronomical Observatory (Australia); K. Freeman, Australian National Univ. (Australia);

G. Frost, L. Gers, M. Goodwin, D. Gray, R. Heald, Australian Astronomical Observatory (Australia); J. Heijmans, TNO (Netherlands); D. Jones, Prime Optics (Australia); S. Keller, The Australian National Univ. (Australia); U. Klauser, Y. Kondrat, Australian Astronomical Observatory (Australia); J. Lawrence, Australian Astronomical Observatory (Australia) and Macquarie Univ. (Australia); S. Lee, S. Mali, Australian Astronomical Observatory (Australia); S. Martell, Australian Astronomical Observatory (Australia) and The Univ. of New South Wales (Australia); D. Mathews, D. Mayfield, S. Miziarski, R. Muller, N. Pai, R. Patterson,

E. Penny, D. Orr, K. Shortridge, Australian Astronomical Observatory (Australia); J. Simpson, Macquarie Univ. (Australia); S. Smedley, G. Smith, D. Stafford, N. Staszak, M. Vuong,

L. Waller, Australian Astronomical Observatory (Australia); E. Wylie de Boer, Australian National Univ. (Australia); P. Xavier, J. Zheng, R. Zhelem, Australian Astronomical Observatory (Australia); D. Zucker, Macquarie Univ. (Australia)

SESSION 5 HIGH MULTIPLEX AND SURVEY INSTRUMENTS III

9147 0Z KOSMOS and COSMOS: new facility instruments for the NOAO 4-meter telescopes [9147-34] P. Martini, The Ohio State Univ. (United States); J. Elias, National Optical Astronomy

Observatory (United States); S. Points, Cerro Tololo Inter-American Observatory (Chile); D. Sprayberry, National Optical Astronomy Observatory (United States); M. A. Derwent, R. Gonzalez, J. A. Mason, T. P. O'Brien, D. P. Pappalardo, R. W. Pogge, The Ohio State Univ. (United States); R. Stoll, The Ohio State Univ. (United States) and Yale Univ. (United States);

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R. Zhelem, The Ohio State Univ (United States) and Australian Astronomical Observatory (Australia); P. Daly, M. Fitzpatrick, J. R. George, National Optical Astronomy Observatory (United States); M. Hunten, National Optical Astronomy Observatory (United States) and The Univ. of Arizona (United States); R. Marshall, G. Poczulp, S. Rath, R. Seaman, National Optical Astronomy Observatory (United States); M. Trueblood, National Optical Astronomy Observatory (United States) and Winer Observatory (United States); K. Zelaya, National Optical Astronomy Observatory (United States)

9147 10 TAIPAN: optical spectroscopy with StarBugs [9147-35] K. Kuehn, J. Lawrence, D. M. Brown, S. Case, Australian Astronomical Observatory

(Australia); M. Colless, The Australian National Univ. (Australia); R. Content, L. Gers, Australian Astronomical Observatory (Australia); J. Gilbert, Australian Astronomical Observatory (Australia) and Univ. of Oxford (United Kingdom); M. Goodwin, A. M. Hopkins, Australian Astronomical Observatory (Australia); M. Ireland, Australian National Univ. (Australia); N. P. F. Lorente, R. Muller, V. Nichani, A. Rakman, Australian Astronomical Observatory (Australia); S. N. Richards, The Univ. of Sydney (Australia); W. Saunders,

N. F. Staszak, J. Tims, L. G. Waller, Australian Astronomical Observatory (Australia) 9147 12 mxSPEC: a massively multiplexed full-disk spectroheliograph for solar physics research

[9147-37] H. Lin, Institute for Astronomy, Univ. of Hawai'i (United States) 9147 13 BATMAN: a DMD-based multi-object spectrograph on Galileo telescope [9147-38] F. Zamkotsian, Lab. d'Astrophysique de Marseille, CNRS (France); P. Spano, INAF -

Osservatorio Astronomico di Brera (Italy); P. Lanzoni, H. Ramarijaona, Lab. d'Astrophysique de Marseille, CNRS (France); M. Moschetti, M. Riva, INAF - Osservatorio Astronomico di Brera (Italy); W. Bon, Lab. d'Astrophysique de Marseille, CNRS (France); L. Nicastro, INAF - IASF Bologna (Italy); E. Molinari, R. Cosentino, A. Ghedina, M. Gonzalez, INAF - Telescopio Nazionale Galileo (Spain); P. Di Marcantonio, I. Coretti, R. Cirami, INAF - Osservatorio Astronomico di Trieste (Italy); F. Zerbi, INAF - Osservatorio Astronomico di Brera (Italy);

L. Valenziano, INAF - IASF Bologna (Italy) SESSION 6 HIGH SPECTRAL RESOLUTION INSTRUMENTS I

9147 14 Infrared Doppler instrument (IRD) for the Subaru telescope to search for Earth-like planets around nearby M-dwarfs [9147-39]

T. Kotani, National Astronomical Observatory of Japan (Japan); M. Tamura, National Astronomical Observatory of Japan (Japan) and The Univ. of Tokyo (Japan); H. Suto, National Astronomical Observatory of Japan (Japan); J. Nishikawa, National Astronomical Observatory of Japan (Japan) and The Graduate Univ. for Advanced Studies (Japan);

B. Sato, Tokyo Institute of Technology (Japan); W. Aoki, T. Usuda, National Astronomical Observatory of Japan (Japan) and The Graduate Univ. for Advanced Studies (Japan);

T. Kurokawa, National Astronomical Observatory of Japan (Japan) and Tokyo Univ. of Agriculture and Technology (Japan); K. Kashiwagi, Tokyo Univ. of Agriculture and Technology (Japan); S. Nishiyama, Miyagi Univ. of Education (Japan); Y. Ikeda, Photocoding (Japan); D. B. Hall, K. W. Hodapp, Institute for Astronomy, Univ. of Hawai'i (United States); J. Hashimoto, The Univ. of Oklahoma (United States); J. Morino, National Astronomical Observatory of Japan (Japan); Y. Okuyama, Y. Tanaka, S. Suzuki, S. Inoue, Tokyo Univ. of Agriculture and Technology (Japan); J. Kwon, The Univ. of Tokyo (Japan); T. Suenaga, National Astronomical Observatory of Japan (Japan); D. Oh, The Graduate Univ. for Advanced Studies (Japan); H. Baba, National Astronomical Ovatory of Japan

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(Japan) and The Graduate Univ. for Advanced Studies (Japan); N. Narita, E. Kokubo, National Astronomical Observatory of Japan (Japan); Y. Hayano, Subaru Telescope, National Astronomical Observatory of Japan (United States); H. Izumiura, E. Kambe, National Astronomical Observatory of Japan (Japan); T. Kudo, Subaru Telescope, National Astronomical Observatory of Japan (United States); N. Kusakabe, National Astronomical Observatory of Japan (Japan); M. Ikoma, The Univ. of Tokyo (Japan); Y. Hori, Univ. of California Santa Cruz (United States); M. Omiya, National Astronomical Observatory of Japan (Japan); H. Genda, Tokyo Institute of Technology (Japan); A. Fukui, National Astronomical Observatory of Japan (Japan); Y. Fujii, Tokyo institute of Technology (Japan); O. Guyon, Subaru Telescope, National Astronomical Observatory of Japan (United States); H. Harakawa, M. Hayashi, National Astronomical Observatory of Japan (Japan); M. Hidai, Tokai Univ. (Japan); T. Hirano, M. Kuzuhara, Tokyo Institute of Technology (Japan);

M. Machida, Kyusyu Univ. (Japan); T. Matsuo, T. Nagata, Kyoto Univ. (Japan); H. Onuki, National Astronomical Observatory of Japan (Japan); M. Ogihara, Nagoya Univ. (Japan); H. Takami, National Astronomical Observatory of Japan (Japan); N. Takato, Subaru Telescope, National Astronomical Observatory of Japan (United States); Y. H. Takahashi, National Astronomical Observatory of Japan (Japan); C. Tachinami, Tokyo Institute of Technology (Japan); H. Terada, National Astronomical Observatory of Japan (United States); H. Kawahara, The Univ. of Tokyo (Japan); T. Yamamuro, Optocraft (Japan)

9147 15 SPIRou: the near-infrared spectropolarimeter/high-precision velocimeter for the Canada-

France-Hawaii telescope [9147-40] É. Artigau, Univ. de Montréal (Canada); D. Kouach, J.-F. Donati, Institut de Recherche en

Astrophysique et Planétologie, CNR, Univ. de Toulouse (France); R. Doyon, Univ. de Montréal (Canada); X. Delfosse, Institut de Planétologie et d’Astrophysique de Grenoble, CNRS, Univ. Joseph Fourier (France); S. Baratchart, M. Lacombe, Institut de Recherche en Astrophysique et Planétologie, CNR, Univ. de Toulouse (France); C. Moutou,

Canada-France-Hawaii Telescope (United States); P. Rabou, Institut de Planétologie et d’Astrophysique de Grenoble, CNRS, Univ. Joseph Fourier (France); L. P. Parès, Y. Micheau, Institut de Recherche en Astrophysique et Planétologie, CNR, Univ. de Toulouse (France);

S. Thibault, Univ. Laval (Canada); V. A. Reshetov, NRC - Herzburg Institute of Astrophysics (Canada); B. Dubois, Institut de Recherche en Astrophysique et Planétologie, CNR, Univ. de Toulouse (France); O. Hernandez, P. Vallée, Univ. de Montréal (Canada); S.-Y. Wang, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan); F. Dolon, Institut de Recherche en Astrophysique et Planétologie, CNR, Univ. de Toulouse (France); F. A. Pepe, Observatoire Astronomique de l’Univ. de Genève (Switzerland); F. Bouchy, Aix Marseille Univ., CNRS, Lab. d’Astrophysique de Marseille (Switzerland); N. Striebig, Institut de Recherche en Astrophysique et Planétologie, CNR, Univ. de Toulouse (France); F. Hénault, Institut de Planétologie et d’Astrophysique de Grenoble, CNRS, Univ. Joseph Fourier (France); D. Loop, L. Saddlemyer, NRC - Herzberg Institute of Astrophysics (Canada); G. Barrick, T. Vermeulen, Canada-France-Hawaii Telescope (United States); M. Dupieux, Institut de Recherche en Astrophysique et Planétologie, CNR, Univ. de Toulouse (France); G. Hébrard, Institut d'Astrophysique de Paris, CNRS, Univ. Pierre et Marie Curie (France); I. Boisse, Univ. do Porto (Portugal); E. Martioli, Lab. Nacional de Astrofísica (Brazil); S. H. P. Alencar, Univ. Federal de Minas Gerais (Brazil); J.-D. do Nascimento, Univ. Federal do Rio Grande do Norte (Brazil); P. Figueira, Univ. do Porto (Portugal)

9147 16 NRES: the network of robotic Echelle spectrographs [9147-41] J. D. Eastman, Las Cumbres Observatory Global Telescope (United States) and Univ. of

California, Santa Barbara (United States); T. M. Brown, Las Cumbres Observatory Global Telescope (United States) and Univ. of Colorado Boulder (United States); J. Hygelund, Las Cumbres Observatory Global Telescope (United States); J. van Eyken, Las Cumbres

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Observatory Global Telescope (United States) and Univ. of California, Santa Barbara (United States); J. R. Tufts, Las Cumbres Observatory Global Telescope (United States);

S. Barnes, Stuart Barnes Optical Design (Netherlands) 9147 17 High resolution broad-band spectroscopy in the NIR using the Triplespec externally

dispersed interferometer at the Hale telescope [9147-42] D. J. Erskine, Lawrence Livermore National Lab. (United States); J. Edelstein, M. Sirk, E. Wishnow, Y. Ishikawa, E. McDonald, W. V. Shourt, Space Sciences Lab., Univ. of

California, Berkeley (United States) 9147 18 A design for high-resolution spectroscopy with adaptive optics at the Large Binocular

Telescope [9147-43] R. O. Reynolds, L. Dettmann, J. C. Guerra, Large Binocular Telescope Observatory (United States) 9147 19 CRIRES+: a cross-dispersed high-resolution infrared spectrograph for the ESO VLT [9147-44] R. Follert, Thüringer Landessternwarte Tautenburg (Germany); R. J. Dorn, European

Southern Observatory (Germany); E. Oliva, INAF - Osservatorio Astrofisico di Arcetri (Italy); J. L. Lizon, European Southern Observatory (Germany); A. Hatzes, Thüringer

Landessternwarte Tautenburg (Germany); N. Piskunov, Uppsala Univ. (Sweden); A. Reiners, U. Seemann, Georg-August-Univ. Göttingen (Germany); E. Stempels, U. Heiter, T. Marquart, M. Lockhart, Uppsala Univ. (Sweden); G. Anglada-Escude, Georg-August-Univ. Göttingen (Germany); T. Löwinger, Thüringer Landessternwarte Tautenburg (Germany); D. Baade, J. Grunhut, P. Bristow, B. Klein, Y. Jung, D. J. Ives, F. Kerber, E. Pozna, J. Paufique, H. U. Kaeufl, European Southern Observatory (Germany); L. Origlia, INAF - Osservatorio Astronomico di Bologna (Italy); E. Valenti, D. Gojak, M. Hilker, L. Pasquini, A. Smette, J. Smoker, European Southern Observatory (Germany)

9147 1A On-sky performance of a high resolution silicon immersion grating spectrometer [9147-45] J. Ge, S. Powell, B. Zhao, S. Schofield, F. Varosi, C. Warner, J. Liu, S. Sithajan, L. Avner, H. Jakeman, J. A. Gittelmacher, W. A. Yoder, Univ. of Florida (United States); M. Muterspaugh, M. Williamson, J. E. Maxwell, Tennessee State Univ. (United States) 9147 1C A laser frequency comb featuring sub-cm/s precision for routine operation on HARPS

[9147-47] R. A. Probst, Max-Planck-Institut für Quantenoptik (Germany); G. Lo Curto, G. Avila,

European Southern Observatory (Germany); B. L. Canto Martins, J. R. de Medeiros, Univ. Federal do Rio Grande do Norte (Brazil); M. Esposito, J. I. González Hernández, Instituto de Astrofísica de Canarias (Spain); T. W. Hänsch, Max-Planck-Institut für Quantenoptik (Germany); R. Holzwarth, Max-Planck-Institut für Quantenoptik (Germany) and Menlo Systems GmbH (Germany); F. Kerber, European Southern Observatory (Germany);

I. C. Leão, Univ. Federal do Rio Grande do Norte (Brazil); A. Manescau, L. Pasquini, European Southern Observatory (Germany); R. Rebolo-López, Instituto de Astrofísica de Canarias (Spain); T. Steinmetz, Max-Planck-Institut für Quantenoptik (Germany) and Menlo Systems GmbH (Germany); T. Udem, Max-Planck-Institut für Quantenoptik (Germany);

Y. Wu, Max-Planck-Institut für Quantenoptik (Germany) and Menlo Systems GmbH (Germany)

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9147 1D Design and early performance of IGRINS (Immersion Grating Infrared Spectrometer) [9147-48] C. Park, Korea Astronomy and Space Science Institute (Korea, Republic of); D. T. Jaffe, The

Univ. of Texas at Austin (United States); I.-S. Yuk, M.-Y. Chun, Korea Astronomy and Space Science Institute (Korea, Republic of); S. Pak, Kyung Hee Univ. (Korea, Republic of);

K.-M. Kim, Korea Astronomy and Space Science Institute (Korea, Republic of); M. Pavel, H. Lee, The Univ. of Texas at Austin (United States); H. Oh, Korea Astronomy and Space

Science Institute (Korea, Republic of) and Univ. of Science and Technology (Korea, Republic of); U. Jeong, Korea Astronomy and Space Science Institute (Korea, Republic of); C. K. Sim, H.-I. Lee, H. A. Nguyen Le, Kyung Hee Univ. (Korea, Republic of); J. Strubhar,

M. Gully-Santiago, The Univ. of Texas at Austin (United States); J. S. Oh, S.-M. Cha, B. Moon, K. Park, Korea Astronomy and Space Science Institute (Korea, Republic of); C. Brooks, The

Univ. of Texas at Austin (United States); K. Ko, J.-Y. Han, J. Nah, Korea Astronomy and Space Science Institute (Korea, Republic of); P. C. Hill, The Univ. of Texas at Austin (United States); S. Lee, Space Environment Lab. (Korea, Republic of); S. Barnes, Stuart Barnes Optical Design (Netherlands); Y. S. Yu, Korea Astronomy and Space Science Institute (Korea, Republic of); K. Kaplan, G. Mace, The Univ. of Texas at Austin (United States);

H. Kim, J.-J. Lee, N. Hwang, Korea Astronomy and Space Science Institute (Korea, Republic of); B.-G. Park, Korea Astronomy and Space Science Institute (Korea, Republic of) and Univ. of Science and Technology (Korea, Republic of)

9147 1E High resolution near IR spectroscopy with GIANO-TNG [9147-49] L. Origlia, INAF - Osservatorio Astronomico di Bologna (Italy); E. Oliva, C. Baffa, G. Falcini, E. Giani, F. Massi, INAF - Osservatorio Astrofisico di Arcetri (Italy); P. Montegriffo, INAF -

Osservatorio Astronomico di Bologna (Italy); N. Sanna, INAF - Osservatorio Astrofisico di Arcetri (Italy); S. Scuderi, INAF - Osservatorio Astrofisico di Catania (Italy); M. Sozzi, A. Tozzi, INAF - Osservatorio Astrofisico di Arcetri (Italy); I. Carleo, Bologna Univ. (Italy) and INAF - Osservatorio Astrofisico di Padova (Italy); R. Gratton, INAF - Osservatorio Astrofisico di Padova (Italy); F. Ghinassi, M. Lodi, Telescopio Nazionale Galileo (Spain)

SESSION 7 HIGH SPECTRAL RESOLUTION INSTRUMENTS II

9147 1F CARMENES instrument overview [9147-50] A. Quirrenbach, Landessternwarte Heidelberg (Germany); P. J. Amado, Instituto de

Astrofísica de Andalucía (Spain); J. A. Caballero, Ctr. de Astrobiología (Spain); R. Mundt, Max-Planck-Institut für Astronomie (Germany); A. Reiners, Institut für Astrophysik Göttingen (Germany); I. Ribas, Institut de Ciències de l'Espai (Spain); W. Seifert, Landessternwarte Heidelberg (Germany); M. Abril, Instituto de Astrofísica de Andalucía (Spain); J. Aceituno, Calar Alto Observatory (Spain); F. J. Alonso-Floriano, Univ. Complutense de Madrid (Spain);

M. Ammler-von Eiff, Thüringer Landessternwarte Tautenburg (Germany); R. Antona Jiménez, Instituto de Astrofísica de Andalucía (Spain); H. Anwand-Heerwart,

Institut für Astrophysik Göttingen (Germany); M. Azzaro, Calar Alto Observatory (Spain); F. Bauer, Institut für Astrophysik Göttingen (Germany); D. Barrado, Calar Alto Observatory

(Spain); S. Becerril, Instituto de Astrofísica de Andalucía (Spain); V. J. S. Béjar, Instituto de Astrofísica de Canarias (Spain); D. Benítez, Calar Alto Observatory (Spain); Z. M. Berdiñas,

M. C. Cárdenas, E. Casal, A. Claret, Instituto de Astrofísica de Andalucía (Spain); J. Colomé, Institut de Ciències de l’Espai (Spain); M. Cortés-Contreras, Univ. Complutense

de Madrid (Spain); S. Czesla, Hamburger Sternwarte (Germany); M. Doellinger, Thüringer Landessternwarte Tautenburg (Germany); S. Dreizler, Institut für Astrophysik Göttingen (Germany); C. Feiz, Landessternwarte Heidelberg (Germany); M. Fernández, Instituto de Astrofísica de Andalucía (Spain); D. Galadí, Calar Alto Observatory (Spain);

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M. C. Gálvez-Ortiz, Ctr. de Astrobiología (Spain); A. García-Piquer, Institut de Ciéncies de l’Espai (Spain); M. L. García-Vargas, FRACTAL S.L.N.E (Spain); R. Garrido, Instituto de Astrofísica de Andalucía (Spain); L. Gesa, Institut de Ciències de l'Espai (Spain);

V. Gómez Galera, Calar Alto Observatory (Spain); E. González Álvarez, Univ. Complutense de Madrid (Spain); J. I. González Hernández, Instituto de Astrofísica de Canarias (Spain);

U. Grözinger, Max-Planck-Institut für Astronomie (Germany); J. Guàrdia, Institut de Ciències de l'Espai (Spain); E. W. Guenther, Thüringer Landessternwarte Tautenburg (Germany);

E. de Guindos, Calar Alto Observatory (Spain); J. Gutiérrez-Soto, Instituto de Astrofísica de Andalucía (Spain); H.-J. Hagen, Hamburger Sternwarte (Germany); A. P. Hatzes, Thüringer Landessternwarte Tautenburg (Germany); P. H. Hauschildt, Hamburger Sternwarte (Germany); J. Helmling, Calar Alto Observatory (Spain); T. Henning, D. Hermann, Max-Planck-Institut für Astronomie (Germany); L. Hernández Castaño, Calar Alto Observatory (Spain); E. Herrero, Institut de Ciències de l'Espai (Spain); D. Hidalgo, G. Holgado, Univ. Complutense de Madrid (Spain); A. Huber, Max-Planck-Institut für Astronomie (Germany); K. F. Huber, Hamburger Sternwarte (Germany); S. Jeffers, Institut für Astrophysik Göttingen (Germany); V. Joergens, Max-Planck-Institut für Astronomie (Germany); E. de Juan, Calar Alto Observatory (Spain); M. Kehr, Thüringer Landessternwarte Tautenburg (Germany);

R. Klein, M. Kürster, Max-Planck-Institut für Astronomie (Germany); A. Lamert, Institut für Astrophysik Göttingen (Germany); S. Lalitha, Hamburger Sternwarte (Germany); W. Laun, Max-Planck-Institut für Astronomie (Germany); U. Lemke, Institut für Astrophysik Göttingen (Germany); R. Lenzen, Max-Planck-Institut für Astronomie (Germany); M. López del Fresno, B. López Martí, Ctr. de Astrobiología (Spain); J. López-Santiago, Univ. Complutense de Madrid (Spain); U. Mall, Max-Planck-Institut für Astronomie (Germany); H. Mandel, Landessternwarte Heidelberg (Germany); E. L. Martín, Ctr. de Astrobiología (Spain);

S. Martín-Ruiz, Instituto de Astrofísica de Andalucía (Spain); H. Martínez-Rodríguez, Univ. Complutense de Madrid (Spain); C. J. Marvin, Institut für Astrophysik Göttingen (Germany); R. J. Mathar, Max-Planck-Institut für Astronomie (Germany); E. Mirabet, Instituto de Astrofísica de Andalucía (Spain); D. Montes, Univ. Complutense de Madrid (Spain);

R. Morales Muñoz, Instituto de Astrofísica de Andalucía (Spain); A. Moya, Ctr. de Astrobiología (Spain); V. Naranjo, Max-Planck-Institut für Astronomie (Germany); A. Ofir, Institut für Astrophysik Göttingen (Germany); R. Oreiro, Instituto de Astrofísica de Andalucía (Spain); E. Pallé, Instituto de Astrofísica de Canarias (Spain); J. Panduro, Max-Planck-Institut für Astronomie (Germany); V.-M. Passegger, Institut für Astrophysik Göttingen (Germany); A. Pérez-Calpena, FRACTAL S.L.N.E (Spain); D. Pérez Medialdea, Instituto de Astrofísica de Andalucía (Spain); M. Perger, Institut de Ciències de l’Espai (Spain); M. Pluto, Thüringer Landessternwarte Tautenburg (Germany); A. Ramón, Instituto de Astrofísica de Andalucía (Spain); R. Rebolo, P. Redondo, Instituto de Astrofísica de Canarias (Spain); S. Reffert, Landessternwarte Heidelberg (Germany); S. Reinhardt, Calar Alto Observatory (Spain);

P. Rhode, Institut für Astrophysik Göttingen (Germany); H.-W. Rix, F. Rodler, Max-Planck-Institut für Astronomie (Germany); E. Rodríguez, C. Rodríguez-López, E. Rodríguez-Pérez, Instituto de Astrofísica de Andalucía (Spain); R.-R. Rohloff, Max-Planck-Institut für Astronomie (Germany); A. Rosich, Institut de Ciències de l’Espai (Spain); E. Sánchez-Blanco, M. A. Sánchez Carrasco, Instituto de Astrofísica de Andalucía (Spain);

J. Sanz-Forcada, Ctr. de Astrobiología (Spain); L. F. Sarmiento, S. Schäfer, Institut für Astrophysik Göttingen (Germany); J. Schiller, Thüringer Landessternwarte Tautenburg (Germany); C. Schmidt, Institut für Astrophysik Göttingen (Germany); J. H. M. M. Schmitt, Hamburger Sternwarte (Germany); E. Solano, Ctr. de Astrobiología (Spain); O. Stahl, Landessternwarte Heidelberg (Germany); C. Storz, Max-Planck-Institut für Astronomie (Germany); J. Stürmer, Landessternwarte Heidelberg (Germany); J. C. Suárez, Instituto de Astrofísica de Andalucía (Spain); R.-G. Ulbrich, Institut für Astrophysik Göttingen (Germany); G. Veredas, K. Wagner, Landessternwarte Heidelberg (Germany); J. Winkler, Thüringer

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Landessternwarte Tautenburg (Germany); M. R. Zapatero Osorio, Ctr. de Astrobiología (Spain); M. Zechmeister, Institut für Astrophysik Göttingen (Germany);

F. J. Abellán de Paco, Univ. Complutense de Madrid (Spain); G. Anglada-Escudé, Univ. of London (United Kingdom); C. del Burgo, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico); A. Klutsch, INAF - Osservatorio Astrofisico di Catania (Italy); J. L. Lizon, European Organisation for Astronomical Research in the Southern Hemisphere (Germany); M. López-Morales, Harvard-Smithsonian Ctr. for Astrophysics (United States); J. C. Morales, LESIA, Observatoire de Paris (France); M. A. C. Perryman, Univ. College Dublin (Ireland); S. M. Tulloch, FRACTAL S.L.N.E (Spain); W. Xu, Wenli Xu Optical System Engineering (Germany)

9147 1G The Habitable-zone Planet Finder: A status update on the development of a stabilized fiber-

fed near-infrared spectrograph for the for the Hobby-Eberly telescope [9147-51] S. Mahadevan, L. W. Ramsey, R. Terrien, S. Halverson, A. Roy, F. Hearty, E. Levi, G. K. Stefansson, P. Robertson, C. Bender, C. Schwab, The Pennsylvania State Univ. (United States); M. Nelson, Univ. of Virginia (United States) 9147 1H ESPRESSO: the radial velocity machine for the VLT [9147-52] D. Mégevand, Observatoire de l’Univ. de Genève (Switzerland); F. M. Zerbi, INAF -

Osservatorio Astronomico di Brera (Italy); P. Di Marcantonio, INAF - Osservatorio Astronomico di Trieste (Italy); A. Cabral, Univ. de Lisboa (Portugal); M. Riva, INAF - Osservatorio Astronomico di Brera (Italy); M. Abreu, Univ. de Lisboa (Portugal); F. Pepe, Observatoire de l’Univ. de Genève (Switzerland); S. Cristiani, INAF - Osservatorio Astronomico di Trieste (Italy); R. Rebolo Lopez, Instituto de Astrofísica de Canarias (Spain); N. C. Santos, Univ. do Porto (Portugal); H. Dekker, European Southern Observatory (Germany); M. Aliverti, INAF - Osservatorio Astronomico di Brera (Italy); C. Allende,

M. Amate, Instituto de Astrofísica de Canarias (Spain); G. Avila, European Southern Observatory (Germany); V. Baldini, INAF - Osservatorio Astronomico di Trieste (Italy);

T. Bandy, Univ. Bern (Switzerland); P. Bristow, European Southern Observatory (Germany); C. Broeg, Univ. Bern (Switzerland); R. Cirami, INAF - Osservatorio Astronomico di Trieste (Italy); J. Coelho, Univ. de Lisboa (Portugal); P. Conconi, INAF - Osservatorio Astronomico di Brera (Italy); I. Coretti, G. Cupani, V. D'Odorico, INAF - Osservatorio Astronomico di Trieste (Italy); V. De Caprio, INAF - Osservatorio Astronomico di Brera (Italy); B. Delabre, R. Dorn, European Southern Observatory (Germany); P. Figueira, Univ. do Porto (Portugal);

A. Fragoso, Instituto de Astrofísica de Canarias (Spain); S. Galeotta, INAF - Osservatorio Astronomico di Trieste (Italy); L. Genolet, Observatoire de l’Univ. de Genève (Switzerland); R. Gomes, Univ. de Lisboa (Portugal); J. González Hernández, Instituto de Astrofísica de Canarias (Spain); I. Hughes, Observatoire de l’Univ. de Genève (Switzerland); O. Iwert,

F. Kerber, European Southern Observatory (Germany); M. Landoni, INAF - Osservatorio Astronomico di Brera (Italy); J.-L. Lizon, European Southern Observatory (Germany);

C. Lovis, C. Maire, Observatoire de l’Univ. de Genève (Switzerland); M. Mannetta, INAF - Osservatorio Astronomico di Trieste (Italy); C. C. J. A. P. Martins, Univ. do Porto (Portugal);

P. Molaro, INAF - Osservatorio Astronomico di Trieste (Italy); M. A. S. Monteiro, Univ. do Porto (Portugal); M. Moschetti, INAF - Osservatorio Astronomico di Brera (Italy); A. Oliveira, Univ. de Lisboa (Portugal); M. R. Zapatero Osorio, Ctr. de Astrobiología (Spain); E. Poretti, INAF - Osservatorio Astronomico di Brera (Italy); J. L. Rasilla, S. Santana Tschudi, Instituto de Astrofísica de Canarias (Spain); P. Santos, Univ. de Lisboa (Portugal); D. Sosnowska, Observatoire de l’Univ. de Genève (Switzerland); S. Sousa, Univ. do Porto (Portugal);

F. Tenegi, Instituto de Astrofísica de Canarias (Spain); G. Toso, INAF - Osservatorio Astronomico di Brera (Italy); E. Vanzella, M. Viel, INAF - Osservatorio Astronomico di Trieste (Italy)

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9147 1I PIMMS échelle: the next generation of compact diffraction limited spectrographs for arbitrary input beams [9147-53]

C. H. Betters, S. G. Leon-Saval, J. Bland-Hawthorn, S. N. Richards, The Univ. of Sydney (Australia); T. A. Birks, I. Gris-Sánchez, Univ. of Bath (United Kingdom)

9147 1J Progress on the Gemini High-Resolution Optical SpecTrograph (GHOST) design [9147-54] M. J. Ireland, Australian National Univ. (Australia); A. Anthony, G. Burley, E. Chisholm, NRC -

Herzberg Institute of Astrophysics (Canada); V. Churilov, Australian Astronomical Observatory (Australia); J. Dunn, NRC - Herzberg Institute of Astrophysics (Canada);

G. Frost, J. Lawrence, Australian Astronomical Observatory (Australia); D. Loop, NRC - Herzberg Institute of Astrophysics (Canada); P. McGregor, The Australian National Univ. (Australia); S. Martell, Univ. of New South Wales (Australia); A. McConnachie, NRC - Herzberg Institute of Astrophysics (Canada); R. M. McDermid, Australian Astronomical Observatory (Australia) and Macquarie Univ. (Australia); J. Pazder, V. Reshetov, NRC - Herzberg Institute of Astrophysics (Canada); J. G. Robertson, A. Sheinis, J. Tims, Australian Astronomical Observatory (Australia); P. Young, The Australian National Univ. (Australia);

R. Zhelem, Australian Astronomical Observatory (Australia) SESSION 8 HIGH SPATIAL RESOLUTION INSTRUMENTS I

9147 1K The integral field spectrograph for the Gemini planet imager [9147-55] J. E. Larkin, J. K. Chilcote, T. Aliado, Univ. of California, Los Angeles (United States); B. J. Bauman, Lawrence Livermore National Lab. (United States); G. Brims, J. M. Canfield,

Univ. of California, Los Angeles (United States); A. Cardwell, Gemini Observatory (Chile); D. Dillon, UARC, Univ. of California, Santa Cruz (United States); R. Doyon, Univ. de Montréal

(Canada); J. Dunn, NRC - Herzberg Institute of Astrophysics (Canada); M. P. Fitzgerald, Univ. of California, Los Angeles (United States); J. R. Graham, Univ. of California, Berkeley (United States); S. Goodsell, M. Hartung, P. Hibon, Gemini Observatory (Chile); P. Ingraham, Kavli Institute for Particle Astrophysics and Cosmology, Stanford Univ. (United States) and Univ. de Montréal (Canada); C. A. Johnson, E. Kress, Univ. of California, Los Angeles (United States); Q. M. Konopacky, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada); B. A. Macintosh, Lawrence Livermore National Lab. (United States) and Kavli Institute for Particle Astrophysics and Cosmology, Stanford Univ. (United States); K. G. Magnone, Univ. of California, Los Angeles (United States); J. Maire, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada); I. S. McLean, Univ. of California, Los Angeles (United States); D. Palmer, Lawrence Livermore National Lab. (United States); M. D. Perrin, Space Telescope Science Institute (United States); C. Quiroz, F. Rantakyrö, N. Sadakuni, Gemini Observatory (Chile); L. Saddlemyer, NRC - Herzberg Institute of Astrophysics (Canada); A. Serio, Gemini Observatory (Chile); S. Thibault, Univ. Laval (Canada); S. J. Thomas, NASA Ames Research Ctr. (United States) and UARC, Univ. of California, Santa Cruz (United States); P. Vallee, Univ. de Montréal (Canada); J. L. Weiss, Univ. of California, Los Angeles (United States)

9147 1L The SPHERE IFS at work [9147-56] R. Claudi, E. Giro, M. Turatto, A. Baruffolo, INAF - Osservatorio Astronomico di Padova

(Italy); P. Bruno, INAF - Osservatorio Astrofisico di Catania (Italy); E. Cascone, V. DeCaprio, INAF - Osservatorio Astronomico di Capodimonte (Italy); S. Desidera, INAF - Osservatorio Astronomico di Padova (Italy); R. Dorn, European Southern Observatory (Germany);

D. Fantinel, INAF - Osservatorio Astronomico di Padova (Italy); G. Finger, European Southern Observatory (Germany); R. Gratton, L. Lessio, INAF - Osservatorio Astronomico di Padova (Italy); J. L. Lizon, European Southern Observatory (Germany); A. L. Maire, D. Mesa,

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B. Salasnich, INAF - Osservatorio Astronomico di Padova (Italy); S. Scuderi, INAF - Osservatorio Astrofisico di Catania (Italy); A. Zurlo, INAF - Osservatorio Astronomico di Padova (Italy); K. Dohlen, Lab. d'Astrophysique de Marseille (France); J. L. Beuzit,

D. Mouillet, P. Puget, Institut de Planétologie et d’Astrophysique de Grenoble (France); F. Wildi, Observatoire de Genève (Switzerland); N. Hubin, M. Kasper, European Southern

Observatory (Germany) 9147 1M The LINC-NIRVANA high resolution imager: challenges from the lab to first light [9147-57] T. M. Herbst, Max-Planck-Institut für Astronomie (Germany); R. Ragazzoni, INAF -

Osservatorio Astronomico di Padova (Italy); A. Eckart, Univ. zu Köln (Germany); G. Weigelt, Max-Planck-Institut für Radioastronomie (Germany)

9147 1O Operation and performance of the mid-infrared camera, NOMIC, on the Large Binocular

Telescope [9147-59] W. F. Hoffmann, P. M. Hinz, D. Defrère, J. M. Leisenring, A. J. Skemer, P. A. Arbo, M. Montoya, Steward Observatory, The Univ. of Arizona (United States); B. Mennesson, Jet

Propulsion Lab. (United States) 9147 1P FRIDA, the diffraction limited NIR imager and IFS for the Gran Telescopio Canarias: status

report [9147-60] J. A. López, Univ. Nacional Autónoma de México (Mexico); J. Acosta, Instituto de

Astrofísica de Canarias (Spain); L. C. Alvarez, Univ. Nacional Autónoma de México (Mexico); V. Bringas, Ctr. de Ingeniería y Desarrollo Industrial (Mexico); N. Cardiel, Univ. Complutense de Madrid (Spain); D. M. Clark, Univ. Nacional Autónoma de México (Mexico); A. Corrales, Ctr. de Ingeniería y Desarrollo Industrial (Mexico); S. Cuevas,

O. Chapa, Univ. Nacional Autónoma de México (Mexico); J. J. Díaz, Instituto de Astrofísica de Canarias (Spain); S. S. Eikenberry, Univ. of Florida (United States); C. Eliche, Univ. Complutense de Madrid (Spain); C. Espejo, R. Flores, J. Fuentes, Univ. Nacional Autónoma de México (Mexico); J. Gallego, Univ. Complutense de Madrid (Spain); J. Garcés, Univ. Nacional Autónoma de México (Mexico); F. Garzón, Instituto de Astrofísica de Canarias (Spain); P. Hammersley, European Southern Observatory (Germany); C. Keiman, G. Lara, Univ. Nacional Autónoma de México (Mexico); P. López, Instituto de Astrofísica de Canarias (Spain); D. Lucero, Ctr. de Ingeniería y Desarrollo Industrial (Mexico); H. Moreno, Instituto de Astrofísica de Canarias (Spain); S. Pascual, Univ. Complutense de Madrid (Spain); J. Patrón, A. Prieto, Instituto de Astrofísica de Canarias (Spain); A. Rodríguez, B. Rodríguez, Ctr. de Ingeniería y Desarrollo Industrial (Mexico); B. Sánchez, Univ. Nacional Autónoma de México (Mexico); D. Torres, J. Uribe, Ctr. de Ingeniería y Desarrollo Industrial (Mexico); A. Watson, Univ. Nacional Autónoma de México (Mexico)

Part Two 9147 1Q Development and recent results from the Subaru coronagraphic extreme adaptive optics

system [9147-61] N. Jovanovic, Subaru Telescope, National Astronomical Observatory of Japan (United

States); O. Guyon, Subaru Telescope, National Astronomical Observatory of Japan (United States) and Steward Observatory, The Univ. of Arizona (United States); F. Martinache, Observatoire de la Côte d'Azur (France); C. Clergeon, G. Singh, Subaru Telescope, National Astronomical Observatory of Japan (United States) and LESIA, Observatoire de Paris à Meudon (France); T. Kudo, Subaru Telescope, National Astronomical Observatory of Japan (United States); K. Newman, College of Optical Sciences, The Univ. of Arizona (United States) and NASA Ames Research Ctr. (United States); J. Kuhn, E. Serabyn, Jet

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Propulsion Lab. (United States); B. Norris, P. Tuthill, P. Stewart, The Univ. of Sydney (Australia); E. Huby, G. Perrin, S. Lacour, S. Vievard, LESIA, Observatoire de Paris à Meudon (France);

N. Murakami, O. Fumika, Hokkaido Univ. (Japan); Y. Minowa, Y. Hayano, Subaru Telescope, National Astronomical Observatory of Japan (United States); J. White, Gemini Observatory (United States); O. Lai, Subaru Telescope, National Astronomical Observatory of Japan (United States); F. Marchis, SETI Institute (United States); G. Duchene, Univ. of California, Berkeley (United States) and Univ. Grenoble Alpes, CNRS, Institut de Planetologie et d'Astrophysique de Grenoble (France); T. Kotani, Subaru Telescope, National Astronomical Observatory of Japan (United States); J. Woillez, European Southern Observatory (Germany)

9147 1R High contrast polarimetry in the infrared with SPHERE on the VLT [9147-62] M. Langlois, Ctr. de Recherche Astronomique de Lyon, Observatoire de Lyon, CNRS, Univ.

de Lyon 1 (France) and Ecole Normale Supérieure de Lyon (France); K. Dohlen, A. Vigan, A. Zurlo, C. Moutou, Aix-Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); H. M. Schmid, ETH Zürich (Switzerland); J. Mili, J.-L. Beuzit, Institut de Planétologie et d’Astrophysique de Grenoble (France); A. Boccaletti, LESIA, Observatoire de Paris (France); M. Carle, A. Costille, Aix-Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); R. Dorn, European Southern Observatory (Germany); L. Gluck, Institut de Planétologie et d’Astrophysique de Grenoble (France); N. Hubin, European Southern Observatory (Germany); M. Feldt, Max-Planck-Institut für Astronomie (Germany); M. Kasper, L. Lizon, European Southern Observatory (Germany); F. Madec, D. Le Mignant, Aix-Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); D. Mouillet, J.-P. Puget, Institut de Planétologie et d’Astrophysique de Grenoble (France); J.-F. Sauvage, ONERA (France);

F. Wildi, Observatoire Astronomique de l’Univ. de Genève (Switzerland) 9147 1S High-precision polarimetry at the Mont-Mégantic Observatory with the new polarimeter

POMM [9147-63] P. Bastien, O. Hernandez, L. Albert, É. Artigau, R. Doyon, Univ. de Montréal (Canada); L. Drissen, Univ. Laval (Canada); D. Lafrenière, A. F. J. Moffat, N. St-Louis, Univ. de Montréal

(Canada) 9147 1T High-resolution imaging in the visible on large ground-based telescopes [9147-64] C. MacKay, Univ. of Cambridge (United Kingdom); R. Rebolo, Consejo Superior de

Investigaciones Científicas (Spain); J. Crass, D. L. King, Univ. of Cambridge (United Kingdom); L. Labadie, Univ. zu Köln (Germany); V. González Escalera, M. Puga, Instituto de Astrofísica de Canarias (Spain); A. Pérez Garrido, Univ. Politécnica de Cartagena (Spain); R. López, A. Oscoz, J. A. Pérez-Prieto, L. F. Rodríguez-Ramos, S. Velasco, Instituto de Astrofísica de Canarias (Spain); I. Villó, Univ. Politécnica de Cartagena (Spain)

SESSION 9 HIGH SPATIAL RESOLUTION INSTRUMENTS II

9147 1U ERIS: preliminary design phase overview [9147-66] H. Kuntschner, L. Jochum, P. Amico, J. K. Dekker, F. Kerber, E. Marchetti, M. Accardo, R. Brast, M. Brinkmann, R. D. Conzelmann, B.-A. Delabre, M. Duchateau, E. Fedrigo, G. Finger, C. Frank, F. G. Rodriguez, B. Klein, J. Knudstrup, M. Le Louarn, L. Lundin, A. Modigliani, M. Mueller, M. Neeser, S. Tordo, E. Valenti, European Southern Observatory

(Germany); F. Eisenhauer, E. Sturm, H. Feuchtgruber, E. M. George, M. Hartl, R. Hofmann, H. Huber, M. P. Plattner, J. Schubert, K. Tarantik, E. Wiezorrek, Max-Planck-Institut für

extraterrestrische Physik (Germany); M. R. Meyer, S. P. Quanz, A. M. Glauser, ETH Zürich (Switzerland); H. Weisz, Ingenieursbureau für den Maschinenbau (Germany); S. Esposito,

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M. Xompero, G. Agapito, J. Antichi, V. Biliotti, M. Bonaglia, R. Briguglio, L. Carbonaro, G. Cresci, L. Fini, E. Pinna, A. T. Puglisi, F. Quirós-Pacheco, A. Riccardi, G. Di Rico, INAF -

Osservatorio Astrofisico di Arcetri (Italy); C. Arcidiacono, INAF - Osservatorio Astronomico di Bologna (Italy); M. Dolci, INAF - Osservatorio Astronomico di Teramo (Italy)

9147 1V High-contrast planet imager for Kyoto 4m segmented telescope [9147-67] T. Matsuo, Kyoto Univ. (Japan); N. Murakami, Hokkaido Univ. (Japan); T. Kotani, National

Astronomical Observatory of Japan (Japan); H. Kawahara, The Univ. of Tokyo (Japan); N. Natsume, M. Kino, K. Yamamoto, Kyoto Univ. (Japan); H. Imada, Univ. of Tsukuba

(Japan); M. Kurita, Kyoto Univ. (Japan); M. Iribe, H. Nishida, Osaka Electro-Communication Univ. (Japan); M. Kida, H. Kitou, Hokkaido Univ. (Japan); K. Ishikawa, RIKEN (Japan); Y. Uda, Osaka Electro-Communication Univ. (Japan); H. Tokoro, Nano-Optonics Research Institute (Japan); T. Nagata, F. Iwamuro, Kyoto Univ. (Japan); N. Miura, The Univ. of Tokyo (Japan); S. Oya, Subaru Telescope, National Astronomical Observatory of Japan (United States);

Y. Itoh, Nishi-Harima Astronomical Observatory (Japan); H. Shibai, Osaka Univ. (Japan); M. Tamura, National Astronomical Observatory of Japan (Japan) and The Univ. of Tokyo

(Japan) 9147 1W Construction and status of the CHARIS high contrast imaging spectrograph [9147-68] T. D. Groff, N. J. Kasdin, M. A. Limbach, M. Galvin, M. A. Carr, G. Knapp, T. Brandt, C. Loomis, N. Jarosik, Princeton Univ. (United States); K. Mede, National Astronomical

Observatory of Japan (Japan); M. W. McElwain, NASA Goddard Space Flight Ctr. (United States); M. Janson, Princeton Univ. (United States); O. Guyon, N. Jovanovic, N. Takato,

F. Martinache, Subaru Telescope, National Astronomical Observatory of Japan (United States); M. Hayashi, National Astronomical Observatory of Japan (Japan)

SESSION 10 INSTRUMENTS FOR EXTREMELY LARGE TELESCOPES

9147 1Y Status of the instrumentation program for the Giant Magellan Telescope (Invited Paper) [9147-70]

G. H. Jacoby, A. Bouchez, Giant Magellan Telescope Organization (United States); M. Colless, The Australian National Univ. (Australia); D. DePoy, Texas A&M Univ. (United States); D. Jaffe, The Univ. of Texas at Austin (United States); J. Lawrence, Australian Astronomical Observatory (Australia); P. McGregor, The Australian National Univ. (Australia); R. Bernstein, Giant Magellan Telescope Organization (United States) and Carnegie Observatories (United States); S. Shectman, Carnegie Observatories (United States); A. Szentgyorgyi, Harvard-Smithsonian Ctr. for Astrophysics (United States)

9147 1Z The E-ELT instrument roadmap: a status report (Invited Paper) [9147-71] S. K. Ramsay, M. M. Casali, J. C. González, N. Hubin, European Southern Observatory

(Germany) 9147 20 An update on the wide field, multi-object, moderate-resolution, spectrograph for the Giant

Magellan Telescope [9147-72] D. L. DePoy, R. Allen, T. Li, J. L. Marshall, C. Papovich, T. Prochaska, Texas A&M Univ. (United

States); S. Shectman, Carnegie Observatories (United States) 9147 21 METIS: the mid-infrared E-ELT imager and spectrograph [9147-73] B. R. Brandl, Leiden Univ. (Netherlands); M. Feldt, Max-Planck-Institut für Astronomie

(Germany); A. Glasse, UK Astronomy Technology Ctr. (United Kingdom); M. Guedel, Univ. Wien (Austria); S. Heikamp, M. Kenworthy, Leiden Univ. (Netherlands); R. Lenzen,

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Max-Planck-Institut für Astronomie (Germany); M. R. Meyer, ETH Zürich (Switzerland); F. Molster, NOVA (Netherlands) and Leiden Univ. (Netherlands); S. Paalvast, Janssen

Precision Engineering BV (Netherlands); E. J. Pantin, Groupe LFEPS, Service d'Astrophysique (France); S. P. Quanz, ETH Zürich (Switzerland); E. Schmalzl, Leiden Univ. (Netherlands);

R. Stuik, Leiden Univ. (Netherlands) and NOVA-ASTRON (Netherlands); L. Venema, Leiden Univ. (Netherlands) and ASTRON (Netherlands); C. Waelkens, Katholieke Univ. Leuven (Belgium)

9147 22 GMTNIRS (Giant Magellan Telescope Near-Infrared Spectrograph): optimizing the design

for maximum science productivity and minimum risk [9147-74] D. T. Jaffe, The Univ. of Texas at Austin (United States); S. Barnes, Stuart Barnes Optical

Design (New Zealand); C. Brooks, M. Gully-Santiago, The Univ. of Texas at Austin (United States); S. Pak, Kyung Hee Univ. (Korea, Republic of); C. Park, I. Yuk, Korea Astronomy and Space Science Institute (Korea, Republic of)

9147 23 HIRES: the high resolution spectrograph for the E-ELT [9147-75] F. M. Zerbi, Scientific Directorate of INAF (Italy); F. Bouchy, Lab. d'Astrophysique de

Marseille, CNRS (France); J. Fynbo, Dark Cosmology Ctr. (Denmark); R. Maiolino, Univ. of Cambridge (United Kingdom); N. Piskunov, Uppsala Univ. (Sweden); R. Rebolo Lopez, Instituto de Astrofísica de Canarias (Spain); N. Santos, Univ. do Porto (Portugal); K. Strassmeier, Leibniz-Institut für Astrophysik Potsdam (Germany); S. Udry, Observatoire Astronomique, Univ. de Genève (Switzerland); L. Vanzi, Pontificia Univ. Católica de Chile (Chile); M. Riva, INAF - Osservatorio Astronomico di Brera (Italy); A. Basden, Univ. of Durham (United Kingdom); I. Boisse, Lab. d'Astrophysique de Marseille, CNRS (France); X. Bonfils, Observatoire de Science de l'Univ. de Grenoble (France); D. Buscher, Univ. of Cambridge (United Kingdom); A. Cabral, Univ. de Lisboa (Portugal); P. Dimarcantonio, INAF - Osservatorio Astronomico di Trieste (Italy); I. Di Varano, Observatoire Astronomique, Univ. de Genève (Switzerland); D. Henry, UK Astronomy Technology Ctr. (United Kingdom); M. Monteiro, Univ. do Porto (Portugal); T. Morris, G. Murray, Durham Univ. (United Kingdom); E. Oliva, INAF - Osservatorio Astrofisico di Arcetri (Italy); I. Parry, Univ. of Cambridge (United Kingdom); F. Pepe, Observatoire Astronomique, Univ. de Genève (Switzerland); A. Quirrenbach, Landessternwarte Heidelberg (Germany); J. L. Rasilla, Instituto de Astrofísica de Canarias (Spain); P. Rees, UK Astronomy Technology Ctr. (United Kingdom); E. Stempels, Uppsala Univ. (Sweden); L. Valenziano, INAF - IASF Bologna (Italy); M. Wells, UK Astronomy Technology Ctr. (United Kingdom); F. Wildi, Observatoire Astronomique, Univ. de Genève (Switzerland); L. Origlia, INAF - Osservatorio Astronomico di Bologna (Italy); C. Allende Prieto, Instituto de Astrofísica de Canarias (Spain); A. Chiavassa, Observatoire de la Côte d’Azur (France); S. Cristiani, INAF - Osservatorio Astronomico di Trieste (Italy); P. Figueira, Univ. do Porto (Portugal); B. Gustafsson, Uppsala Univ. (Sweden); A. Hatzes, Thüringer Landessternwarte Tautenburg (Germany); M. Haehnelt, Univ. of Cambridge (United Kingdom); K. Heng, Univ. Bern (Switzerland); G. Israelian, Instituto de Astrofísica de Canarias (Spain); O. Kochukhov, Uppsala Univ. (Sweden); C. Lovis, Observatoire Astronomique, Univ. de Genève (Switzerland); A. Marconi, Univ. degli Studi di Firenze (Italy); C. J. A. P. Martins, Univ. do Porto (Portugal); P. Noterdaeme, P. Petitjean, Institut d'Astrophysique de Paris (France); T. Puzia, Pontificia Univ. Católica de Chile (Chile); D. Queloz, Univ. of Cambridge (United Kingdom); A. Reiners, Georg-August-Univ. Göttingen (Germany); M. Zoccali, Pontificia Univ. Católica de Chile (Chile)

9147 24 The Infrared Imaging Spectrograph (IRIS) for TMT: instrument overview [9147-76] A. M. Moore, Caltech Optical Observatories (United States); J. E. Larkin, Univ. of California,

Los Angeles (United States); S. A. Wright, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada) and Univ. of Toronto (Canada); B. Bauman, Lawrence Livermore

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National Lab. (United States); J. Dunn, NRC - Herzberg Institute of Astrophysics (Canada); B. Ellerbroek, Thirty Meter Telescope Observatory Corp. (United States); A. C. Phillips, Univ. of California Observatories (United States); L. Simard, NRC - Dominion Astrophysical Observatory (Canada); R. Suzuki, National Astronomical Observatory of Japan (Japan); K. Zhang, Nanjing Institute of Astronomical Optics and Technology (China); T. Aliado, G. Brims, J. Canfield, Univ. of California, Los Angeles (United States); S. Chen, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada); R. Dekany, A. Delacroix, Caltech Optical Observatories (United States); T. Do, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada) and Univ. of Toronto (Canada); G. Herriot, NRC - Herzberg Institute of Astrophysics (Canada); B. Ikenoue, National Astronomical Observatory of Japan (Japan); C. Johnson, Univ. of California, Los Angeles (United States); E. Meyer, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada) and Univ. of Toronto (Canada); Y. Obuchi, National Astronomical Observatory of Japan (Japan); J. Pazder, V. Reshetov, NRC - Herzberg Institute of Astrophysics (Canada); R. Riddle, Caltech Optical Observatories (United States); S. Saito, National Astronomical Observatory of Japan (Japan); R. Smith, Caltech Optical Observatories (United States); J. M. Sohn, Univ. of California, Los Angeles (United States); F. Uraguchi, T. Usuda, National Astronomical Observatory of Japan (Japan); E. Wang, Univ. of California, Los Angeles (United States); L. Wang, Thirty Meter Telescope Observatory Corp. (United States); J. Weiss, Univ. of California, Los Angeles (United States); R. Wooff, NRC - Herzberg Institute of Astrophysics (Canada)

9147 25 HARMONI: the first light integral field spectrograph for the E-ELT [9147-77] N. A. Thatte, F. Clarke, Univ. of Oxford (United Kingdom); I. Bryson, H. Schnetler, UK

Astronomy Technology Ctr. (United Kingdom); M. Tecza, Univ. of Oxford (United Kingdom); R. M. Bacon, A. Remillieux, CRAL, Observatoire de Lyon (France); E. Mediavilla,

J. M. Herreros Linares, Instituto de Astrofísica de Canarias (Spain); S. Arribas, Ctr. de Astrobiologica (Spain); C. J. Evans, D. W. Lunney, UK Astronomy Technology Ctr. (United Kingdom); T. Fusco, ONERA (France) and Lab. d'Astrophysique de Marseille (France);

K. O'Brien, Univ. of Oxford (United Kingdom); I. A. Tosh, STFC Rutherford Appleton Lab. (United Kingdom); D. J. Ives, G. Finger, European Southern Observatory (Germany);

R. Houghton, R. L. Davies, J. D. Lynn, J. R. Allen, S. D. Zieleniewski, S. Kendrew, V. Ferraro-Wood, Univ. of Oxford (United Kingdom); A. Pécontal-Rousset, J. Kosmalski, J. Richard, A. Jarno, CRAL, Observatoire de Lyon (France); A. M. Gallie, D. M. Montgomery,

D. Henry, UK Astronomy Technology Ctr. (United Kingdom); G. Zins, Institut de Planétologie et d’Astrophysique de Grenoble (France); D. Freeman, Kidger Optics Associates (United Kingdom); B. García-Lorenzo, L. F. Rodríguez-Ramos, J. S.-C. Revuelta, E. Hernández-Suárez, A. Bueno-Bueno, J. V. Gigante-Ripoll, Instituto de Astrofísica de Canarias (Spain);

A. Garcia, SENER Ingeniería y Sistemas S.A. (Spain); K. Dohlen, B. Neichel, Lab. d'Astrophysique de Marseille (France)

9147 26 A preliminary design for the GMT-Consortium Large Earth Finder (G-CLEF) [9147-78] A. Szentgyorgyi, Harvard-Smithsonian Ctr. for Astrophysics (United States); S. Barnes, Stuart

Barnes Optical Design (Netherlands); J. Bean, The Univ. of Chicago (United States); B. Bigelow, A. Bouchez, Giant Magellan Telescope Organization (United States); M.-Y. Chun, Korea Astronomy and Space Science Institute (Korea, Republic of); J. D. Crane, Carnegie Observatories (United States); H. Epps, Lick Observatory, Univ. of

California, Santa Cruz (United States); I. Evans, J. Evans, Harvard-Smithsonian Ctr. for Astrophysics (United States); A. Frebel, MIT Kavli Institute for Astrophysics and Space Research (United States); G. Furesz, A. Glenday, Harvard-Smithsonian Ctr. for Astrophysics (United States); D. Guzman, Pontificia Univ. Católica de Chile (Chile); T. Hare, Carnegie Observatories (United States); B.-H. Jang, J.-G. Jang, U. Jeong, Korea Astronomy and

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Space Science Institute (Korea, Republic of); A. Jordan, MIT Kavli Institute for Astrophysics and Space Research (United States); K.-M. Kim, J. Kim, Korea Astronomy and Space Science Institute (Korea, Republic of); C.-H. Li, Stuart Barnes Optical Design (Netherlands); M. Lopez-Morales, K. McCracken, B. McLeod, M. Mueller, Harvard-Smithsonian Ctr. for Astrophysics (United States); J. Nah, Korea Astronomy and Space Science Institute (Korea, Republic of); T. Norton, Harvard-Smithsonian Ctr. for Astrophysics (United States); H. Oh, Korea Astronomy and Space Science Institute (Korea, Republic of) and Korea Univ. of Science and Technology (Korea, Republic of); J. S. Oh, Korea Astronomy and Space Science Institute (Korea, Republic of); M. Ordway, Harvard-Smithsonian Ctr. for Astrophysics (United States); B.-G. Park, Korea Astronomy and Space Science Institute (Korea, Republic of) and Korea Univ. of Science and Technology (Korea, Republic of); C. Park, S.-J. Park, Korea Astronomy and Space Science Institute (Korea, Republic of); D. Phillips, D. Plummer, W. Podgorski, F. Rodler, Harvard-Smithsonian Ctr. for Astrophysics (United States);

A. Seifahrt, The Univ. of Chicago (United States); K.-M. Tak, Korea Astronomy and Space Science Institute (Korea, Republic of); A. Uomoto, Carnegie Observatories (United States); M. A. Van Dam, Flat Wavefronts (New Zealand); R. Walsworth, Harvard-Smithsonian Ctr. for Astrophysics (United States); Y. S. Yu, I.-S. Yuk, Korea Astronomy and Space Science Institute (Korea, Republic of)

9147 27 MOSAIC at the E-ELT: A multi-object spectrograph for astrophysics, IGM and cosmology

[9147-79] F. Hammer, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); B. Barbuy, Univ.

de São Paulo (Brazil); J. G. Cuby, Aix Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); L. Kaper, Univ. van Amsterdam (Netherlands); S. Morris, Durham Univ. (United Kingdom); C. J. Evans, UK Astronomy Technology Ctr. (United Kingdom);

P. Jagourel, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); G. Dalton, Univ. of Oxford (United Kingdom) and Rutherford Appleton Lab. (United Kingdom); P. Rees, UK Astronomy Technology Ctr. (United Kingdom); M. Puech, M. Rodrigues, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); D. Pearson, UK Astronomy Technology Ctr. (United Kingdom); K. Disseau, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France)

9147 28 Conceptual design of the MOBIE imaging spectrograph for TMT [9147-80] B. C. Bigelow, Giant Magellan Telescope Organization (United States); M. V. Radovan,

Univ. of California Observatories (United States); R. A. Bernstein, Giant Magellan Telescope Organization (United States); P. M. Onaka, H. Yamada, S. Isani, Institute for Astronomy, Univ. of Hawai'i (United States); S. Miyazaki, S. Ozaki, National Astronomical Observatory of Japan (Japan)

9147 29 Astrophotonic micro-spectrographs in the era of ELTs [9147-81] N. Blind, Max-Planck-Institut für extraterrestrische Physik (Germany) and Institut de

Planétologie et d’Astrophysique de Grenoble, Univ. J. Fourier, CNRS (France); E. Le Coarer, P. Kern, Institut de Planétologie et d’Astrophysique de Grenoble, Univ. J. Fourier, CNRS (France); J. Bland-Hawthorn, The Univ. of Sydney (Australia)

POSTER SESSION: INSTRUMENT PROGRAMS AND NEW SCIENCE INSTRUMENTS AND UPGRADES

9147 2C Updated optical design and trade-off study for MOONS, the Multi-Object Optical and Near

Infrared spectrometer for the VLT [9147-84] E. Oliva, INAF - Osservatorio Astrofisico di Arcetri (Italy); S. Todd, M. Cirasuolo, H. Schnetler,

D. Lunney, P. Rees II, STFC UK Astronomy Technology Ctr. (United Kingdom); A. Bianco,

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INAF - Osservatorio Astronomico di Brera (Italy); E. Diolaiti, INAF - Osservatorio Astronomico di Bologna (Italy); D. Ferruzzi, INAF - Osservatorio Astrofisico di Arcetri (Italy); M. Fisher, Univ. of Cambridge (United Kingdom); I. Guinouard, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); M. Iuzzolino, INAF - Osservatorio Astrofisico di Arcetri (Italy); I. Parry, X. Sun, Univ. of Cambridge (United Kingdom); A. Tozzi, INAF - Osservatorio Astrofisico di Arcetri (Italy); F. Vitali, INAF - Osservatorio Astronomico di Roma (Italy)

9147 2D Optical, mechanical and electronic design and integration of POMM, a polarimeter for the

Observatoire du mont Mégantic [9147-85] M. R. Leclerc, P. Côté, F. Duchesne, INO (Canada); P. Bastien, Univ. de Montréal

(Canada); O. Hernandez, Univ. de Montréal (Canada) and Observatoire du Mont Mégantic (Canada); P. Colonna d'Istria, Univ. de Montréal (Canada); M. Demers,

M. Girard, M. Savard, D. Lemieux, INO (Canada); S. Thibault, D. Brousseau, Univ. Laval (Canada)

9147 2F A polarimetric unit for HARPS-North at the Telescopio Nazionale Galileo: HANPO [9147-87] F. Leone, Univ. degli Studi di Catania (Italy) and INAF - Osservatorio Astrofisico di Catania

(Italy); M. Cecconi, R. Cosentino, A. Ghedina, INAF - Fundación Galileo Galilei (Spain); M. Giarrusso, Univ. degli Studi di Catania (Italy) and INAF - Osservatorio Astrofisico di

Catania (Italy); M. Gonzalez, V. Lorenzi, INAF - Fundación Galileo Galilei (Spain); M. Munari, INAF - Osservatorio Astrofisico di Catania (Italy); H. Perez Ventura, L. Riverol, J. San Juan, INAF - Fundación Galileo Galilei (Spain); S. Scuderi, INAF - Osservatorio Astrofisico di Catania (Italy)

9147 2G An off-the-shelf guider for the Palomar 200-inch telescope: interfacing amateur astronomy

software with professional telescopes for an easy life [9147-88] F. Clarke, J. Lynn, N. Thatte, M. Tecza, Univ. of Oxford (United Kingdom) 9147 2H Design updates and status of the fourth generation TripleSpec spectrograph [9147-89] E. Schlawin, T. L. Herter, C. Henderson, Cornell Univ. (United States); J. C. Wilson, Univ. of

Virginia (United States); R. Probst, D. Sprayberry, National Optical Astronomy Observatory (United States); M. Bonati, P. Schurter, D. James, M. Warner, R. Tighe, Cerro Tololo Inter-American Observatory (Chile); J. D. Adams, Univ. Research Space Association

(United States); M. Martinez, Cerro Tololo Inter-American Observatory (Chile) 9147 2J A Fabry-Perot and grism imaging spectrograph LISS (Line Imager and Slit Spectrograph)

[9147-91] Y. Hashiba, M. Doi, S. Sako, T. Morokuma, The Univ. of Tokyo (Japan); H. Kuncarayakti,

Millennium Institute of Astrophysics (Chile) and Univ. de Chile (Chile); M. Kokubo, K. Mitsuda, H. Takahashi, K. Tateuchi, The Univ. of Tokyo (Japan); M. Watanabe, H. Nakao,

Hokkaido Univ. (Japan) 9147 2K The mechanical design for the WEAVE prime focus corrector system [9147-93] D. C. Abrams, K. Dee, Isaac Newton Group of Telescopes (Spain); T. Agócs, NOVA ASTRON

(Netherlands); E. Lhome, Isaac Newton Group of Telescopes (Spain); J. Peñate, Instituto de Astrofísica de Canarias (Spain); A. Jaskó, E. Bányai, MTA Research Ctr. for Astronomy and Earth Sciences (Hungary); J. A. Burgal, Instituto de Astrofísica de Canarias (Spain);

G. Dalton, STFC Rutherford Appleton Lab. (United Kingdom) and Univ. of Oxford (United Kingdom); K. Middleton, STFC Rutherford Appleton Lab. (United Kingdom); P. Bonifacio, GEPI, Observatoire de Paris à Meudon (France); J. A. L. Aguerri, Instituto de Astrofísica de Canarias (Spain); S. C. Trager, Univ. of Groningen (Netherlands); M. Balcells, Isaac Newton Group of Telescopes (Spain)

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9147 2L Conceptual design of a low resolution spectrograph for the Astronomical Observatory of Córdoba [9147-94]

D. Q. Nagasawa, J. L. Marshall, D. L. DePoy, N. Mondrik, Texas A&M Univ. (United States) 9147 2M The GRAVITY spectrometers: design report of the optomechanics and active cryogenic

mechanisms [9147-95] M. Wiest, S. Yazici, Univ. zu Köln (Germany); S. Fischer, Deutsches Zentrum für Luft- und

Raumfahrt e.V. (Germany); M. Thiel, Kayser-Threde GmbH (Germany); M. Haug, Max-Planck-Institut für extraterrestrische Physik (Germany); C. Araujo-Hauck, Gemini

Observatory (Chile); C. Straubmeier, I. Wank, Univ. zu Köln (Germany); F. Eisenhauer, Max-Planck-Institut für extraterrestrische Physik (Germany); G. Perrin, Lab. d'Etudes Spatiales et d'Instrumentation en Astrophysique (France), LESIA, Observatoire de Paris, CNRS, UPMC, Univ. Paris Diderot (France), and Groupement d’Intérêt Scientifique PHASE (France); W. Brandner, Max-Planck-Institut für Astronomie (Germany); K. Perraut, Lab. d’Astrophysique Observatoire de Grenoble (France); A. Amorim, CENTRA-SIM (Portugal); M. Schöller, European Southern Observatory (Germany); A. Eckart, Univ. zu Köln (Germany) and Max-Planck-Institut für Radioastronomie (Germany)

9147 2N First-generation instrumentation for the Discovery Channel Telescope [9147-96] T. A. Bida, E. W. Dunham, P. Massey, H. G. Roe, Lowell Observatory (United States) 9147 2Q POMM: design of rotating mechanism and hexapod structure [9147-99] P. Côté, M. Leclerc, M. Demers, INO (Canada); P. Bastien, O. Hernandez, Univ. de Montréal

(Canada) 9147 2R Testing fully depleted CCD [9147-100] R. Casas, Institut de Ciències de l’Espai (Spain); L. Cardiel-Sas, Institut de Física d’Altes

Energies (Spain); F. J. Castander, Institut de Ciències de l’Espai (Spain); J. Jiménez, Institut de Física d'Altes Energies (Spain); J. de Vicente, Ctr. de Investigaciones Energéticas, Medioambientales y Tecnológicas (Spain)

9147 2S Readout electronics of physics of accelerating universe camera [9147-101] J. de Vicente, J. Castilla, Ctr. de Investigaciones Energéticas, Medioambientales y

Tecnológicas (Spain); J. Jiménez, L. Cardiel-Sas, J. M. Illa, Institut de Física d'Altes Energies (Spain)

9147 2T Acousto-optical imaging spectropolarimetric devices: new opportunities and

developments [9147-102] V. Y. Molchanov, S. P. Anikin, S. I. Chizhikov, K. B. Yushkov, O. Y. Makarov, National Univ. of

Science and Technology "MISiS" (Russian Federation); A. M. Tatarnikov, S. A. Potanin, V. F. Esipov, Lomonosov Moscow State Univ. (Russian Federation) 9147 2V The near infrared camera for the Subaru Prime Focus Spectrograph [9147-104] S. A. Smee, Johns Hopkins Univ. (United States); J. E. Gunn, Princeton Univ. (United States);

M. Golebiowski, R. Barkhouser, Johns Hopkins Univ. (United States); S. Vivès, S. Pascal, Aix Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); M. Carr, Princeton Univ. (United States); S. C. Hope, Johns Hopkins Univ. (United States); C. Loomis, Princeton Univ. (United States); M. Hart, Johns Hopkins Univ. (United States); H. Sugai, N. Tamura,

A. Shimono, Kavli Institute for the Physics and Mathematics of the Universe, The Univ. of Tokyo (Japan)

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9147 2W Detector driver systems and photometric estimates for RIMAS [9147-105] V. L. Toy, Univ. of Maryland, College Park (United States); A. S. Kutyrev, Univ. of Maryland,

College Park (United States) and NASA Goddard Space Flight Ctr. (United States); E. I. Lyness, NASA Goddard Space Flight Ctr. (United States); M. Muench, Norwegian Univ.

of Science and Technology (Norway); F. D. Robinson, G. N. Lotkin, NASA Goddard Space Flight Ctr. (United States); J. I. Capone, S. Veilleux, Univ. of Maryland, College Park (United States); S. H. Moseley, N. A. Gehrels, NASA Goddard Space Flight Ctr. (United States);

S. N. Vogel, Univ. of Maryland, College Park (United States) 9147 2X FIFI-LS: the facility far-infrared spectrometer for SOFIA [9147-106] R. Klein, SOFIA-USRA, NASA Ames Research Ctr. (United States); S. Beckmann, A. Bryant, S. Colditz, C. Fischer, F. Fumi, Univ. Stuttgart (Germany); N. Geis, Max-Planck-Institut für

extraterrestrische Physik (Germany); R. Hönle, A. Krabbe, Univ. Stuttgart (Germany); L. Looney, Univ. of Illinois at Urbana-Champaign (United States); A. Poglitsch, W. Raab,

Max-Planck-Institut für extraterrestrische Physik (Germany); F. Rebell, Univ. Stuttgart (Germany); M. Savage, SOFIA-USRA, NASA Ames Research Ctr. (United States)

9147 2Y FLITECAM: early commissioning results [9147-108] S. E. Logsdon, I. S. McLean, Univ. of California, Los Angeles (United States); E. E. Becklin,

USRA, NASA Ames Research Ctr. (United States); E. W. Dunham, Lowell Observatory (United States); R. T. Hamilton, USRA, NASA Ames Research Ctr. (United States); C. A. Johnson, Univ. of California, Los Angeles (United States); J. W. Milburn, California Institute of Technology (United States); M. L. Savage, S. S. Shenoy, USRA, NASA Ames Research Ctr. (United States); E. C. Smith, NASA Ames Research Ctr. (United States); W. D. Vacca, USRA, NASA Ames Research Ctr. (United States)

9147 2Z One controlling and driving module based on FPGA in optical fiber positioning device

[9147-111] J. Guo, Y. Gu, Y. Jin, C. Zhai, Univ. of Science and Technology of China (China) 9147 30 Weather monitor station and 225 GHz radiometer system installed at Sierra Negra: the

Large Millimeter Telescope site [9147-112] D. Ferrusca, J. Contreras R., Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico) 9147 32 Near-infrared wavelength calibration of astrophysical spectrographs with the emission

spectrum of the CN molecule [9147-115] A. Boesch, A. Reiners, Georg-August-Univ. Göttingen (Germany); P. F. Bernath, Old

Dominion Univ. (United States); A. Seifahrt, The Univ. of Chicago (United States) 9147 33 The characteristics and development status of the control and housekeeping electronics of

FRIDA [9147-116] J. J. Díaz, Instituto de Astrofísica de Canarias (Spain); R. Flores-Meza, B. Sánchez, Univ.

Nacional Autónoma de México (Mexico); J. Patrón, Instituto de Astrofísica de Canarias (Spain)

9147 34 Fibre positioning concept for the WEAVE spectrograph at the WHT [9147-117] I. J. Lewis, Univ. of Oxford (United Kingdom); G. B. Dalton, Univ. of Oxford (United Kingdom)

and Rutherford Appleton Lab. (United Kingdom); M. Brock, J. Gilbert, Univ. of Oxford (United Kingdom); D. C. Abrams, Isaac Newton Group of Telescopes (Spain);

J. A. L. Aguerri, Instituto de Astrofísica de Canarias (Spain); P. Bonifacio, GEPI, Observatoire de Paris (France); K. Middleton, Rutherford Appleton Lab. (United Kingdom); S. C. Trager, Univ. of Groningen (Netherlands)

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9147 35 Precise angular positioning at 6K: the FIFI-LS grating assembly [9147-118] F. Rebell, Univ. Stuttgart (Germany); W. Raab, Max-Planck-Institut für extraterrestrische

Physik (Germany); S. Colditz, S. Beckmann, A. Bryant, C. Fischer, F. Fumi, Univ. Stuttgart (Germany); N. Geis, Max-Planck-Institut für extraterrestrische Physik (Germany); R. Hönle, Univ. Stuttgart (Germany); R. Klein, SOFIA-USRA (United States); A. Krabbe, Univ. Stuttgart (Germany) and Deutsches SOFIA Institut (Germany); L. Looney, Univ. of Illinois at Urbana-Champaign (United States); A. Poglitsch, Max-Planck-Institut für extraterrestrische Physik (Germany); S. Ragan, Max-Planck Institut fuer Astronomie (Germany); M. Savage, SOFIA-USRA, NASA Ames Research Ctr. (United States)

9147 36 Cryogenic optical systems for the rapid infrared imager/spectrometer (RIMAS) [9147-119] J. I. Capone, Univ. of Maryland, College Park (United States); D. A. Content, NASA

Goddard Space Flight Ctr. (United States); A. S. Kutyrev, Univ. of Maryland, College Park (United States) and NASA Goddard Space Flight Ctr. (United States); F. D. Robinson,

G. N. Lotkin, NASA Goddard Space Flight Ctr. (United States) and Global Science and Technology, Inc. (United States); V. L. Toy, S. Veilleux, Univ. of Maryland, College Park (United States); S. H. Moseley, N. A. Gehrels, NASA Goddard Space Flight Ctr. (United States); S. N. Vogel, Univ. of Maryland, College Park (United States)

9147 37 An update on the development of IO:I: a NIR imager for the Liverpool Telescope [9147-120] R. M. Barnsley, I. A. Steele, S. D. Bates, C. J. Mottram, Liverpool John Moores Univ. (United

Kingdom) 9147 38 The precise measurement of the attenuation coefficients of various IR optical materials

applicable to immersion grating [9147-121] S. Kaji, Kyoto-Sangyo Univ. (Japan); Y. Sarugaku, Japan Aerospace Exploration Agency

(Japan); Y. Ikeda, Photocoding (Japan) and Kyoto-Sangyo Univ. (Japan); N. Kobayashi, The Univ. of Tokyo (Japan); K. Nakanishi, S. Kondo, Kyoto-Sangyo Univ. (Japan); C. Yasui, The Univ. of Tokyo (Japan); H. Kawakita, Kyoto-Sangyo Univ. (Japan)

9147 39 Mechanical design of mounts for IGRINS focal plane arrays and field flattening lenses [9147-122]

J. S. Oh, C. Park, S.-M. Cha, I.-S. Yuk, K.-M. Kim, M.-Y. Chun, K. Ko, H. Oh, U. Jeong, J. Nah, Korea Astronomy and Space Science Institute (Korea, Republic of); H. Lee, McDonald Observatory, The Univ. of Texas at Austin (United States); M. Pavel, D. T. Jaffe, The Univ. of Texas at Austin (United States)

9147 3B ARNICA and LonGSp: the refurbishment of two near infrared instruments [9147-124] S. Koshida, L. Vanzi, D. Guzman, R. Leiva, Pontificia Univ. Católica de Chile (Chile); M. A. Bonati, Cerro Tololo Inter-American Observatory (Chile); R. L. Avilés, Pontificia Univ.

Católica de Chile (Chile); C. Baffa, F. Palla, F. Mannucci, INAF - Osservatorio Astrofisico di Arcetri (Italy); T. C. Shen, Pontificia Univ. Católica de Chile (Chile) and Blue Shadows Astronomy and Engineering Ltd. (Chile); V. Suc, Pontificia Univ. Católica de Chile (Chile)

9147 3C Revised specifications and current development status of MIMIZUKU: the mid-infrared

instrument for the TAO 6.5-m telescope [9147-125] T. Kamizuka, T. Miyata, S. Sako, R. Ohsawa, K. Asano, M. Uchiyama, K. Okada, M. Uchiyama, T. Nakamura, I. Sakon, T. Onaka, The Univ. of Tokyo (Japan); H. Kataza,

Japan Aerospace Exploration Agency (Japan); T. Aoki, The Univ. of Tokyo (Japan) and Kiso Observatory, The Univ. of Tokyo (Japan); M. Doi, N. M. Kato, K. Kawara, Y. Kitagawa,

K. Kohno, M. Konishi, The Univ. of Tokyo (Japan); S. Koshida, Pontificia Univ. Católica de Chile (Chile); T. Minezaki, T. Morokuma, K. Motohara, The Univ. of Tokyo (Japan); T. Soyano, The Univ. of Tokyo (Japan) and Kiso Observatory, The Univ. of Tokyo (Japan); H. Takahashi,

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Y. Tamura, T. Tanabé, M. Tanaka, The Univ. of Tokyo (Japan); K. Tarusawa, The Univ. of Tokyo (Japan) and Kiso Observatory, The Univ. of Tokyo (Japan); K. Tateuchi, S. Todo,

Y. Yoshii, The Univ. of Tokyo (Japan) 9147 3E Daytime site characterisation of La Palma, and its relation to night-time conditions [9147-128] M. J. Townson, A. Kellerer, J. Osborn, T. Butterley, T. Morris, R. W. Wilson, Durham Univ.

(United Kingdom) 9147 3G First successful deployment of the ZIMPOL-3 system at the GREGOR telescope [9147-130] R. Ramelli, Istituto Ricerche Solari Locarno (Switzerland); D. Gisler, Istituto Ricerche Solari

Locarno (Switzerland) and Kiepenheuer-Institut für Sonnenphysik (Germany); M. Bianda, Istituto Ricerche Solari Locarno (Switzerland); N. Bello González, S. Berdyugina, D. Soltau, Kiepenheuer-Institut für Sonnenphysik (Germany)

9147 3I MuSICa image slicer prototype at 1.5-m GREGOR solar telescope [9147-132] A. Calcines, R. L. López, Instituto de Astrofísica de Canarias (Spain); M. Collados, Instituto

de Astrofísica de Canarias (Spain) and Univ. de La Laguna (Spain); N. Vega Reyes, Instituto de Astrofísica de Canarias (Spain)

9147 3J Gemini Planet Imager observational calibrations I: overview of the GPI data reduction

pipeline [9147-133] M. D. Perrin, Space Telescope Science Institute (United States); J. Maire, Dunlap Institute for

Astronomy and Astrophysics, Univ. of Toronto (Canada); P. Ingraham, Kavli Institute for Particle Astrophysics and Cosmology, Stanford Univ. (United States) and Univ. de Montréal (Canada); D. Savransky, Cornell Univ. (United States); M. Millar-Blanchaer, Univ. of Toronto (Canada); S. G. Wolff, Johns Hopkins Univ. (United States) and Space Telescope Science Institute (United States); J.-B. Ruffio, SETI Institute (United States); J. J. Wang, Univ. of California, Berkeley (United States); Z. H. Draper, Univ. of Victoria (Canada) and NRC - Herzberg Institute of Astrophysics (Canada); N. Sadakuni, Gemini Observatory (Chile); C. Marois, NRC - Herzberg Institute of Astrophysics (Canada) and Univ. of Victoria (Canada); A. Rajan, Arizona State Univ. (United States); M. P. Fitzgerald, Univ. of California, Los Angeles (United States); B. Macintosh, Kavli Institute for Particle Astrophysics and Cosmology, Stanford Univ. (United States) and Lawrence Livermore National Lab. (United States); J. R. Graham, Univ. of California, Berkeley (United States); R. Doyon, Univ. de Montréal (Canada); J. E. Larkin, J. K. Chilcote, Univ. of California, Los Angeles (United States); S. J. Goodsell, Gemini Observatory (Chile); D. W. Palmer, Lawrence Livermore National Lab. (United States); K. Labrie, Gemini Observatory (United States); M. Beaulieu, Observatoire de la Côte d’Azur, Univ. de Nice Sophia-Antipolis (France); R. J. De Rosa, Arizona State Univ. (United States) and Univ. of Exeter (United Kingdom); A. Z. Greenbaum, Johns Hopkins Univ. (United States) and Space Telescope Science Institute (United States); M. Hartung, P. Hibon, Gemini Observatory (Chile); Q. Konopacky, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada); D. Lafreniere, Univ. de Montréal (Canada); J.-F. Lavigne, ABB, Inc. (Canada); F. Marchis, SETI Institute (United States); J. Patience, Arizona State Univ. (United States); L. Pueyo, Space Telescope Science Institute (United States); F. T. Rantakyrö, Gemini Observatory (Chile); R. Soummer, A. Sivaramakrishnan, Space Telescope Science Institute (United States); S. Thomas, NASA Ames Research Ctr. (United States) and Univ. of California, Santa Cruz (United States); K. Ward-Duong, Arizona State Univ. (United States); S. Wiktorowicz, Univ. of California, Santa Cruz (United States)

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9147 3K KOALA, a wide-field 1000 element integral-field unit for the Anglo-Australian Telescope: assembly and commissioning [9147-134]

R. Zhelem, J. Brzeski, S. Case, V. Churilov, S. Ellis, T. Farrell, A. Green, A. Heng, A. Horton, Australian Astronomical Observatory (Australia); M. Ireland, Mount Stromlo Observatory (Australia); D. Jones, Prime Optics (Australia); U. Klauser, J. Lawrence, S. Miziarski, D. Orr,

N. Pai, N. Staszak, J. Tims, M. Vuong, L. Waller, P. Xavier, Australian Astronomical Observatory (Australia)

9147 3L Single-lock: a stable Fabry-Perot based wavelength calibrator [9147-136] T. M. McCracken, C. A. Jurgenson, D. A. Fischer, R. A. Stoll, A. E. Szymkowiak, J. Bradford,

Yale Univ. (United States); W. Rutter, Massachusetts Institute of Technology (United States) 9147 3N 225GHz opacity measurements at Summit camp, Greenland, for the GreenLand Telescope

(GLT) site testing [9147-138] P. L. Martin-Cocher, K. Asada, S. Matsushita, M.-T. Chen, Institute of Astronomy and

Astrophysics, Academia Sinica (Taiwan); P. T. P. Ho, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan) and Harvard-Smithsonian Ctr. for Astrophysics (United States);

C. Chen, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan) 9147 3O S4EI (Spectral Sampling with Slicer for Stellar and Extragalactical Instrumentation): a new-

generation of 3D spectro-imager dedicated to night astronomy [9147-139] F. Sayède, M. Puech, GEPI, Observatoire de Paris à Meudon (France); P. Mein, LESIA,

Observatoire de Paris (France); P. Bonifacio, GEPI, Observatoire de Paris à Meudon (France); J.-M. Malherbe, R. Galicher, LESIA, Observatoire de Paris (France); J.-P. Amans,

G. Fasola, GEPI, Observatoire de Paris à Meudon (France) 9147 3P Development of Nayoro optical camera and spectrograph for 1.6-m Pirka telescope of

Hokkaido University [9147-140] H. Nakao, M. Watanabe, K. Sorai, Hokkaido Univ. (Japan); M. Yamada, Kobe Univ.

(Japan); Y. Itoh, Univ. of Hyogo (Japan); S. Sako, T. Miyata, The Univ. of Tokyo (Japan) 9147 3Q Instrument control software based on LabVIEW for HARPS-N [9147-141] X. Gao, A. Vick, UK Astronomy Technology Ctr. (United Kingdom); A. Glenday, Harvard-

Smithsonian Ctr. for Astrophysics (United States); M. Gonzalez, INAF - Fundación Galileo Galilei (Spain)

9147 3R Optomecatronic design and integration of a high resolution equipment Berkut to the 1-meter class telescopes [9147-142] R. Granados, R. López, A. Farah, Univ. Nacional Autónoma de México (Mexico) 9147 3S VIRUS instrument collimator assembly [9147-143] J. L. Marshall, D. L. DePoy, T. Prochaska, R. D. Allen, P. Williams, J.-P. Rheault, T. Li, D. Q. Nagasawa, C. Akers, D. Baker, E. Boster, C. Campbell, E. Cook, A. Elder, A. Gary, J. Glover, M. James, E. Martin, W. Meador, N. Mondrik, M. Rodriguez-Patino, S. Villanueva

Jr., Texas A&M Univ. (United States); G. J. Hill, S. Tuttle, B. Vattiat, H. Lee, McDonald Observatory, The Univ. of Texas at Austin (United States); T. S. Chonis, The Univ. of Texas at Austin (United States); G. B. Dalton, M. Tacon, Univ. of Oxford (United Kingdom)

9147 3T Reverse and concurrent engineering applied of a high resolution equipment Berkut for 1-meter class telescopes [9147-144] R. López, R. Granados, A. Farah, Univ. Nacional Autónoma de México (Mexico)

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9147 3U Remote and automatic small-scale observatories: experience with an all-sky fireball patrol camera [9147-145]

F. C. M. Bettonvil, NOVA ASTRON (Netherlands) and Univ. Leiden (Netherlands) 9147 3V Optical integration and verification of LINC-NIRVANA [9147-146] J. Moreno-Ventas, H. Baumeister, T. Bertram, P. Bizenberger, F. Briegel, D. Greggio, F. Kittmann, L. Marafatto, L. Mohr, K. Radhakrishnan, H. Schray, Max-Planck-Institut für

Astronomie (Germany) 9147 3W The ZIMPOL high contrast imaging polarimeter for SPHERE: system test results [9147-147] R. Roelfsema, NOVA ASTRON (Netherlands); A. Bazzon, H. M. Schmid, ETH Zürich

(Switzerland); J. Pragt, NOVA ASTRON (Netherlands); D. Gisler, ETH Zürich (Switzerland); C. Dominik, Astronomical Institute Anton Pannekoek (Netherlands); A. Baruffolo, INAF - Osservatorio Astronomico di Padova (Italy); J.-L. Beuzit, IPAG, Univ. Joseph Fourier (France); A. Costille, K. Dohlen, Lab. d'Astrophysique de Marseille, CNRS, Univ. de Provence (France); M. Downing, European Southern Observatory (Germany); E. Elswijk, M. de Haan, NOVA ASTRON (Netherlands); N. Hubin, M. Kasper, European Southern Observatory (Germany); C. Keller, Leiden Observatory (Netherlands); J.-L. Lizon, European Southern Observatory (Germany); D. Mouillet, IPAG, Univ. Joseph Fourier (France); A. Pavlov, Max-Planck-Institut für Astronomie (Germany); P. Puget, IPAG, Univ. Joseph Fourier (France); B. Salasnich, INAF - Osservatorio Astronomico di Padova (Italy); J.-F. Sauvage, ONERA (France); F. Wildi, Observatoire Astronomique de l’Univ. de Genève (Switzerland)

9147 3X PANIC in the lab: status before commissioning [9147-148] B. Dorner, A. Huber, Max-Planck-Institut für Astronomie (Germany); M. C. Cárdenas Vázquez, I. M. Ferro Rodriguez, Instituto de Astrofísica de Andalucía

(Spain); P. Bizenberger, V. Naranjo, J. Panduro, U. Mall, M. Alter, R. Mathar, C. Storz, R.-R. Rohloff, P. Fopp, W. Laun, Max-Planck-Institut für Astronomie (Germany); J. M. Iban ez,

A. J. García Segura, V. Terron, Instituto de Astrofísica de Andalucía (Spain); J. W. Fried, Max-Planck-Institut für Astronomie (Germany); M. Fernández, J. F. Rodríguez Gómez, Instituto de Astrofísica de Andalucía (Spain); K. Meisenheimer, Max-Planck-Institut für Astronomie (Germany)

Part Three 9147 3Y PISCO: the Parallel Imager for Southern Cosmology Observations [9147-149] B. Stalder, A. A. Stark, S. M. Amato, J. Geary, Harvard-Smithsonian Ctr. for Astrophysics

(United States); S. A. Shectman, Carnegie Observatories (United States); C. W. Stubbs, Harvard Univ. (United States) and Harvard-Smithsonian Ctr. for Astrophysics (United States); A. Szentgyorgyi, Harvard-Smithsonian Ctr. for Astrophysics (United States)

9147 3Z SITELLE optical design, assembly, and testing [9147-150] D. Brousseau, S. Thibault, S. Fortin-Boivin, Univ. Laval (Canada); H. Zhang, ImmerVision

(Canada); P. Vallée, Univ. de Montréal (Canada); H. Auger, L. Drissen, Univ. Laval (Canada)

9147 40 Automated alignment and on-sky performance of the Gemini planet imager coronagraph

[9147-151] D. Savransky, Cornell Univ. (United States); S. J. Thomas, NASA Ames Research Ctr. (United States); L. A. Poyneer, Lawrence Livermore National Lab. (United States); J. Dunn,

NRC - Herzburg Institute of Astrophysics (Canada); B. A. Macintosh, Kavli Institute for

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Particle Astrophysics and Cosmology, Stanford Univ. (United States); N. Sadakuni, Gemini Observatory (Chile); D. Dillon, Univ. of California Observatories (United States) and Lick Observatory, Univ. of California, Santa Cruz (United States); S. J. Goodsell, M. Hartung,

P. Hibon, F. Rantakyrö, A. Cardwell, A. Serio, Gemini Observatory (Chile) 9147 43 Better flat-fielding for ground-based UV spectrographs [9147-154] F. Kerber, R. Hanuschik, S. Moehler, European Southern Observatory (Germany); A. Smette,

J. Smoker, P. Bourget, European Southern Observatory (Chile); P. J. Dwyer, Energetiq Technology, Inc. (United States); M. Rotschädl, Mountain Photonics GmbH (Germany)

9147 44 Developing micro DC-brushless motor driver and position control for fiber positioners [9147-155] L. Jenni, P. Hörler, L. Makarem, J.-P. Kneib, D. Gillet, H. Bleuler, M. Bouri, Ecole Polytechnique

Fédérale de Lausanne (Switzerland); F. Prada, G. De Rivera, Univ. Autónoma de Madrid (Spain); J. Sanchez, Instituto de Astrofísica de Andalucía (Spain)

9147 45 A miniature cryogenic scanning Fabry-Perot interferometer for mid-IR to submm

astronomical observations [9147-156] S. C. Parshley, E. M. Vavagiakis, T. Nikola, G. J. Stacey, Cornell Univ. (United States) 9147 46 The development of ground-based infrared multi-object spectrograph based on the

microshutter array [9147-157] D.-S. Moon, Univ. of Toronto (Canada); S. Sivanandam, Dunlap Institute of Astronomy and

Astrophysics, Univ. of Toronto (Canada); A. S. Kutyrev, S. H. Moseley Jr., NASA Goddard Space Flight Ctr. (United States); J. R. Graham, Univ. of California, Berkeley (United States); A. Roy, Indian Institute of Technology, Kharagpur (India)

9147 47 Optical design of the SuMIRe/PFS spectrograph [9147-158] S. Pascal, S. Vives, Aix Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); R. Barkhouser, Johns Hopkins Univ. (United States); J. E. Gunn, Princeton Univ. (United States) 9147 48 Spherical grating spectrometers [9147-159] D. O'Donoghue, South African Astronomical Observatory (South Africa); J. C. Clemens, The

Univ. of North Carolina at Chapel Hill (United States) 9147 49 Inverse analysis method to optimize the optic tolerances of MEGARA: the future IFU and

multi-object spectrograph for GTC [9147-161] R. Ortiz, E. Carrasco, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico); G. Páez, Ctr. de Investigaciones en Óptica, A.C. (Mexico); E. Sánchez-Blanco, FRACTAL

S.L.N.E (Spain); A. Gil de Paz, J. Gallego, Univ. Complutense de Madrid (Spain); R. Cedazo, Univ. Politécnica de Madrid (Spain); J. Iglesias-Páramo, Instituto de Astrofísica de Andalucía (Spain)

9147 4A Status and first results of the Canarias infrared camera experiment (CIRCE) for the Gran

Telescopio Canarias [9147-162] A. Garner, R. D. Stelter, S. S. Eikenberry, Univ. of Florida (United States); N. Lasso-Cabrera,

Ctr. de Estudios de Física del Cosmos de Aragón (Spain); S. N. Raines, Univ. of Florida (United States); M. Charcos, NASA, SOFIA (United States); M. Edwards, Large Binocular Telescope Observatory (United States); A. Marín-Franch, Ctr. de Estudios de Física del Cosmos de Aragón (Spain); K. Ackley, Univ. of Florida (United States); A. J. Cenarro, Ctr. de Estudios de Física del Cosmos de Aragón (Spain); J. G. Bennett, B. Chinn, R. Frommeyer,

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M. D. Herlevich, P. Miller, C. H. Murphey, Univ. of Florida (United States); C. Packham, The Univ. of Texas at San Antonio (United States)

9147 4B LINC-NIRVANA: Diffraction limited optics in cryogenic environment [9147-163] P. Bizenberger, H. Baumeister, P. Fopp, T. Herbst, W. Laun, L. Mohr, J. Moreno-Ventas, Max-Planck-Institut für Astronomie (Germany) 9147 4C A comparison of concepts for a photonic spectrograph [9147-164] R. J. Harris, J. R. Allington-Smith, Durham Univ. (United Kingdom); D. MacLachlan, R. R. Thomson, Scottish Universities Physics Alliance (United Kingdom) 9147 4D MSE spectrograph optical design: a novel pupil slicing technique [9147-165] P. Spanò, NRC - Herzberg Institute of Astrophysics (Canada) 9147 4E New GRISMs for AFOSC based on volume phase holographic gratings in photopolymers

[9147-166] A. Zanutta, Politecnico di Milano (Italy) and INAF - Osservatorio Astronomico di Brera (Italy);

A. Bianco, M. Landoni, INAF - Osservatorio Astronomico di Brera (Italy); L. Tomasella, S. Benetti, E. Giro, INAF - Osservatorio Astronomico di Padova (Italy) 9147 4F Characterization of the reflectivity of various black materials [9147-167] J. L. Marshall, P. Williams, J.-P. Rheault, T. Prochaska, R. D. Allen, D. L. DePoy, Texas A&M Univ. (United States) 9147 4G FIFI-LS observation planning and data reduction [9147-168] A. Bryant, C. Fischer, R. Hönle, S. Beckmann, S. Colditz, F. Fumi, Univ. Stuttgart (Germany);

N. Geis, Max-Planck-Institut für extraterrestrische Physik (Germany); C. Iserlohe, Univ. zu Köln (Germany); R. Klein, Universities Space Research Association (United States); A. Krabbe, Univ. Stuttgart (Germany); L. Looney, Univ. of Illinois at Urbana-Champaign (United States);

A. Poglitsch, W. Raab, Max-Planck-Institut für extraterrestrische Physik (Germany); S. Ragan, Max-Planck-Institut für Astronomie (Germany); F. Rebell, Univ. Stuttgart (Germany);

M. Savage, Universities Space Research Association (United States) 9147 4H Tests and procedures for optimizing EMIR cooling system [9147-169] P. Fernández Izquierdo, Instituto de Astrofísica de Canarias (Spain); J. L. Lizon, European

Southern Observatory (Germany); M. Á. Núñez Cagigal, J. Patrón Recio, M. Barreto Cabrera, F. Garzón López, Instituto de Astrofísica de Canarias (Spain)

9147 4J Design, alignment, and deployment of the Hobby Eberly Telescope prime focus instrument

package [9147-172] B. Vattiat, G. J. Hill, H. Lee, W. Moreira, N. Drory, J. Ramsey, L. Elliot, M. Landriau, D. M. Perry,

R. Savage, H. Kriel, The Univ. of Texas at Austin (United States); M. Häuser, F. Mangold, Ludwig-Maximilians-Univ. München (Germany)

9147 4K A near-infrared SETI experiment: probability distribution of false coincidences [9147-173] J. Maire, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada); S. A. Wright, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada)

and Univ. of Toronto (Canada); D. Werthimer, Univ. of California, Berkeley (United States); R. R. Treffers, Starman Systems, LLC (United States); G. W. Marcy, Univ. of California, Berkeley (United States); R. P. S. Stone, Lick Observatory, Univ. of California, Santa Cruz (United States); F. Drake, SETI Institute (United States); A. Siemion, Univ. of California, Berkeley (United States)

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9147 4M Automatisms in EMIR instrument to improve operation, safety and maintenance [9147-175] P. Fernández Izquierdo, M. Núñez Cagigal, R. Barreto Rodríguez, N. Martínez Rey, S. Santana Tschudi, M. Barreto Cabrera, J. Patrón Recio, F. Garzón López, Instituto de

Astrofísica de Canarias (Spain) 9147 4O HONIR: an optical and near-infrared simultaneous imager, spectrograph, and polarimeter

for the 1.5-m Kanata telescope [9147-177] H. Akitaya, Y. Moritani, T. Ui, T. Urano, Y. Ohashi, K. S. Kawabata, Hiroshima Univ. (Japan); A. Nakashima, Nagoya City Science Museum (Japan); M. Sasada, Kyoto Univ. (Japan); K. Sakimoto, T. Harao, Hiroshima Univ. (Japan); H. Miyamoto, Molex Japan Co., Ltd.

(Japan); R. Matsui, R. Itoh, K. Takaki, I. Ueno, T. Ohsugi, Hiroshima Univ. (Japan); H. Nakaya, T. Yamashita, National Astronomical Observatory of Japan (Japan); M. Yoshida, Hiroshima Univ. (Japan)

9147 4Q PAUCam readout electronics assembly, integration and test (AIT) [9147-179] J. Jiménez, J. M. Illa, L. Cardiel-Sas, Institut de Física d'Altes Energies (Spain); J. de Vicente,

J. Castilla, Ctr. de Investigaciones Energéticas, Medioambientales y Tecnológicas (Spain); R. Casas, Institut de Ciències de l'Espai (Spain)

9147 4R A flux calibration device for the SuperNova Integral Field Spectrograph (SNIFS) [9147-180] S. Lombardo, Univ. Bonn (Germany); G. Aldering, Lawrence Berkeley National Lab. (United

States); A. Hoffmann, M. Kowalski, D. Küsters, K. Reif, M. Rigault, Univ. Bonn (Germany) 9147 4S Boresight calibration of FIFI-LS: in theory, in the lab and on sky [9147-181] S. Colditz, Univ. Stuttgart (Germany); R. Klein, SOFIA-USRA, NASA Ames Research Ctr.

(United States); S. Beckmann, Univ. Stuttgart (Germany) and Deutsches SOFIA Institut (Germany); A. Bryant, C. Fischer, F. Fumi, Univ. Stuttgart (Germany); N. Geis, Max-Planck-Institut für extraterrestrische Physik (Germany); R. Hönle, Univ. Stuttgart (Germany);

A. Krabbe, Univ. Stuttgart (Germany) and Deutsches SOFIA Institut (Germany); L. W. Looney, Univ. of Illinois at Urbana-Champaign (United States); A. Poglitsch, W. Raab,

Max-Planck-Institut für extraterrestrische Physik (Germany); S. E. Ragan, Max-Planck-Institut für Astronomie (Germany); F. Rebell, Univ. Stuttgart (Germany); M. L. Savage, SOFIA-USRA, NASA Ames Research Ctr. (United States)

9147 4T SPHERE/IRDIS: final performance assessment of the dual-band imaging and long slit

spectroscopy modes [9147-182] A. Vigan, Aix Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); M. Langlois,

Ctr. de Recherche Astronomique de Lyon, CNRS, Univ. Lyon 1 (France); K. Dohlen, A. Zurlo, Aix Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); C. Moutou, Aix Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France) and Canada-France-Hawaii Telescope (United States); A. Costille, C. Gry, F. Madec, D. Le Mignant, Aix Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); L. Gluck, Univ. Joseph Fourier-Grenoble1, CNRS, Institut de Planétologie et d’Astrophysique de Grenoble (France); J.-F. Sauvage, ONERA (France)

9147 4U Characterization of the atmospheric dispersion corrector of the Gemini planet imager

[9147-183] P. Hibon, Gemini South Observatory (Chile); S. Thomas, NASA Ames Research Ctr. (United

States); J. Dunn, J. Atwood, L. Saddlemyer, NRC - Herzburg Institute of Astrophysics (Canada); N. Sadakuni, Gemini South Observatory (Chile); S. Goodsell, Gemini North Observatory (United States); B. Macintosh, Stanford Univ. (United States); J. Graham, Univ. of California, Berkeley (United States); M. Perrin, Space Telescope Science Institute (United

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States); F. Rantakyro, V. Fesquet, A. Serio, C. Quiroz, A. Cardwell, G. Gausachs, Gemini South Observatory (Chile); D. Savransky, Cornell Univ. (United States); D. Kerley, NRC - Herzberg Institute of Astrophysics (Canada); M. Hartung, R. Galvez, K. Hardie, Gemini South Observatory (Chile)

9147 4W Vibration specifications for VLT instruments [9147-185] G. Jakob, J.-L. Lizon, European Southern Observatory (Germany) 9147 4X ARDOLORES: an Arduino based motors control system for DOLORES [9147-186] M. Gonzalez, H. Ventura, J. San Juan, L. Di Fabrizio, Telescopio Nazionale Galileo (Spain) 9147 4Y Design and integration of a mechanism for focusing and alignment of the Echelle

spectrograph for the telescope of 2.1 meters of the National Astronomic Observatory [9147-188]

H. O. A. Gutiérrez, A. S. Farah, J. M. Echevarria R., G. D. Sierra, Univ. Nacional Autónoma de México (Mexico)

9147 4Z Gemini planet imager observational calibrations IX: least-squares inversion flux extraction

[9147-189] Z. H. Draper, Univ. of Victoria (Canada) and NRC - Herzberg Institute of Astrophysics

(Canada); C. Marois, NRC - Herzberg Institute of Astrophysics (Canada) and Univ. of Victoria (Canada); S. Wolff, Johns Hopkins Univ. (United States) and Space Telescope Science Institute (United States); M. Perrin, Space Telescope Science Institute (United States); P. J. Ingraham, Kavli Institute for Particle Astrophysics and Cosmology, Stanford Univ. (United States) and Univ. de Montréal (Canada); J.-B. Ruffio, Institut Supérieur de l’Aéronautique et de l’Espace (France) and SETI Institute (United States); F. T. Rantakyrö,

M. Hartung, S. J. Goodsell, Gemini Observatory (Chile) 9147 50 Gemini planet imager one button approach [9147-190] J. Dunn, D. Kerley, L. Saddlemyer, M. Smith, R. Wooff, NRC - Herzberg Institute of

Astrophysics (Canada); D. Savransky, Cornell Univ. (United States); D. Palmer, B. Macintosh, Lawrence Livermore National Lab. (United States); J. Weiss, Univ. of

California, Los Angeles (United States); C. Quiroz, F. T. Rantakyrö, Gemini Observatory (Chile); S. J. Goodsell, Gemini Observatory (United States)

9147 51 A format standard for efficient interchange of high-contrast direct imaging science

products [9147-191] É. Choquet, Space Telescope Science Institute (United States); A. Vigan, Aix Marseille Univ.,

CNRS, Lab. d’Astrophysique de Marseille (France); R. Soummer, Space Telescope Science Institute (United States); G. Chauvin, Univ. Joseph Fourier-Grenoble 1, CNRS, INSU, IPAG (France); L. Pueyo, M. D. Perrin, D. C. Hines, Space Telescope Science Institute

(United States) 9147 52 Environmental control system for Habitable-zone Planet Finder (HPF) [9147-192] F. Hearty, The Pennsylvania State Univ. (United States) and Univ. of Virginia (United States);

E. Levi, The Pennsylvania State Univ. (United States); M. Nelson, Univ. of Virginia (United States); S. Mahadevan, The Pennsylvania State Univ. (United States) and Ctr. for Exoplanets and Habitable Worlds (United States); A. Burton, Univ. of Virginia (United States); L. Ramsey, C. Bender, R. Terrien, S. Halverson, P. Robertson, A. Roy, The Pennsylvania State Univ. (United States) and Ctr. for Exoplanets and Habitable Worlds (United States); B. Blank,

K. Blanchard, PulseRay (United States); G. Stefansson, The Pennsylvania State Univ. (United States)

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9147 53 Concept study for DREAMS: a Dedicated Robotic EArths-finding single-Mode Spectrograph [9147-193]

J. F. P. Spronck, Leiden Observatory, Leiden Univ. (Netherlands) 9147 54 Characterizing U-Ne hollow cathode lamps at near-IR wavelengths for the CARMENES

survey [9147-194] L. F. Sarmiento, A. Reiners, U. Seemann, U. Lemke, Institut für Astrophysik Göttingen

(Germany); J. Winkler, M. Pluto, E. W. Günther, Thüringer Landessternwarte Tautenburg (Germany); A. Quirrenbach, Landessternwarte, Zentrum für Astronomie der Univ. Heidelberg (Germany); P. J. Amado, Instituto de Astrofisica de Andalucía (Spain); I. Ribas, Institut de Ciències de l'Espai (Spain); J. A. Caballero, Ctr. de Astrobiología (Spain);

R. Mundt, Max-Planck-Institut für Astronomie (Germany); W. Seifert, Landessternwarte, Zentrum für Astronomie der Univ. Heidelberg (Germany)

9147 55 Gemini planet imager observational calibrations VIII: characterization and role of satellite

spots [9147-195] J. J. Wang, Univ. of California, Berkeley (United States); A. Rajan, Arizona State Univ. (United

States); J. R. Graham, Univ. of California, Berkeley (United States); D. Savransky, Cornell Univ. (United States); P. J. Ingraham, Kavli Institute for Particle Astrophysics and Cosmology, Stanford Univ. (United States); K. Ward-Duong, J. Patience, Arizona State Univ.

(United States); R. J. De Rosa, Arizona State Univ. (United States) and Univ. of Exeter (United Kingdom); J. Bulger, Arizona State Univ. (United States); A. Sivaramakrishnan, M. D. Perrin, Space Telescope Science Institute (United States); S. J. Thomas, NASA Ames

Research Ctr. (United States) and Univ. of California, Santa Cruz (United States); N. Sadakuni, Gemini Observatory (Chile); A. Z. Greenbaum, Johns Hopkins Univ. (United States) and Space Telescope Science Institute (United States); L. Pueyo, Space

Telescope Science Institute (United States); C. Marois, NRC - Herzberg Institute of Astrophysics (Canada) and Univ. of Victoria (Canada); B. R. Oppenheimer, American Museum of Natural History (United States); P. Kalas, Univ. of California, Berkeley

(United States); A. Cardwell, S. Goodsell, P. Hibon, F. T. Rantakyrö, Gemini Observatory (Chile)

9147 56 MASCARA: opto-mechanical design and integration [9147-196] J. F. P. Spronck, A.-L. Lesage, R. Stuik, Leiden Observatory, Leiden Univ. (Netherlands); F. Bettonvil, Leiden Observatory, Leiden Univ. (Netherlands) and NOVA (Netherlands);

I. A. G. Snellen, Leiden Observatory, Leiden Univ. (Netherlands) 9147 57 Study on a multi-delay spectral interferometry for stellar radial velocity measurement

[9147-197] K. Zhang, H. Jiang, J. Tang, H. Ji, Y. Zhu, Nanjing Institute of Astronomical Optics and

Technology (China); L. Wang, National Astronomical Observatories (China) 9147 58 Test of multi-object exoplanet search spectral interferometer [9147-198] K. Zhang, Nanjing Institute of Astronomical Optics and Technology (China); L. Wang,

National Astronomical Observatories (China); H. Jiang, Y. Zhu, Y. Hou, S. Dai, J. Tang, Z. Tang, Y. Zeng, Y. Chen, L. Wang, Z. Hu, Nanjing Institute of Astronomical Optics and

Technology (China) 9147 5A Diffraction-limited lucky imaging with a 12" commercial telescope [9147-201] B. J. Baptista, National Geospatial-Intelligence Agency (United States)

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9147 5B Archon: a modern controller for high performance astronomical CCDs [9147-202] G. Bredthauer, Semiconductor Technology Associates Inc. (United States) 9147 5C Near field modal noise reduction using annealed optical fiber [9147-203] S. N. Osterman, Johns Hopkins Univ. Applied Physics Lab. (United States) and Univ. of

Colorado, Boulder (United States); G. G. Ycas, National Institute of Standards and Technology (United States); C. L. Donaldson, Southwest Research Institute (United States);

S. A. Diddams, National Institute of Standards and Technology (United States) and Univ. of Colorado, Boulder (United States); S. Mahadevan, L. W. Ramsey, The Pennsylvania State Univ. (United States); P. P. Plavchan, NASA Exoplanet Science Institute (United States) and Missouri State Univ. (United States)

9147 5D Control and operation of the 1.6 m New Solar Telescope in Big Bear [9147-204] J. Varsik, C. Plymate, P. Goode, A. Kosovichev, W. Cao, R. Coulter, K. Ahn, N. Gorceix, S. Shumko, Big Bear Solar Observatory (United States) 9147 5F DigiCam: fully digital compact camera for SST-1M telescope [9147-206] J. A. Aguilar, Univ. de Genève (Switzerland); W. Bilnik, AGH Univ. of Science and

Technology (Poland); L. Bogacz, Jagiellonian Univ. (Poland); T. Bulik, Univ. of Warsaw (Poland); A. Christov, D. della Volpe, Univ. de Genève (Switzerland); M. Dyrda, Instytut Fizyki Jądrowej (Poland); A. Frankowski, Nicolaus Copernicus Astronomical Ctr. (Poland);

M. Grudzinska, Univ. of Warsaw (Poland); J. Grygorczuk, Centrum Badań Kosmicznych (Poland); M. Heller, Univ. de Genève (Poland); B. Idźkowski, Jagiellonian Univ. (Poland);

M. Janiak, Nicolaus Copernicus Astronomical Ctr. (Poland); M. Jamrozy, Jagiellonian Univ. (Poland); M. Karczewski, Centrum Badań Kosmicznych (Poland); J. Kasperek, AGH Univ. of Science and Technology (Poland); E. Lyard, Univ. de Genève (Switzerland); A. Marszałek, Jagiellonian Univ. (Poland); J. Michałowski, Instytut Fizyki Jądrowej (Poland); R. Moderski, Nicolaus Copernicus Astronomical Ctr. (Poland); T. Montaruli, A. Neronov, Univ. de Genève (Switzerland); J. Nicolau-Kukliński, Centrum Badań Kosmicznych (Poland); J. Niemiec, Instytut Fizyki Jądrowej (Poland); M. Ostrowski, Jagiellonian Univ. (Poland); P. Paśko,

Ł. Płatos, Centrum Badań Kosmicznych (Poland); E. Prandini, Univ. de Genève (Switzerland); R. Pruchniewicz, AGH Univ. of Science and Technology (Poland); J. Rafalski, Instytut Fizyki Jądrowej (Poland); P. J. Rajda, AGH Univ. of Science and Technology (Poland); M. Rameez, Univ. de Genève (Switzerland); M. Rataj, Centrum Badań Kosmicznych (Poland); M. Rupiński, AGH Univ. of Science and Technology (Poland);

K. Rutkowski, K. Seweryn, M. Sidz, Centrum Badań Kosmicznych (Poland); Ł. Stawarz, M. Stodulska, Jagiellonian Univ. (Poland); M. Stodulski, Instytut Fizyki Jądrowej (Poland); M. Tokarz, Centrum Badań Kosmicznych (Poland); S. Toscano, I. Troyano Pujadas, R. Walter,

Univ. de Genève (Switzerland); P. Wawer, R. Wawrzaszek, L. Wiśniewski, Centrum Badań Kosmicznych (Poland); K. Ziętara, Jagiellonian Univ. (Poland); P. Ziółkowski, P. Żychowski, Instytut Fizyki Jądrowej (Poland)

9147 5G Wavelength calibration from 1-5µm for the CRIRES+ high-resolution spectrograph at the VLT

[9147-208] U. Seemann, G. Anglada-Escude, Georg-August-Univ. Göttingen (Germany); D. Baade, P. Bristow, R. J. Dorn, European Southern Observatory (Germany); R. Follert, Thüringer

Landessternwarte Tautenburg (Germany); D. Gojak, J. Grunhut, European Southern Observatory (Germany); A. P. Hatzes, Thüringer Landessternwarte Tautenburg (Germany); U. Heiter, Uppsala Univ. (Sweden); D. J. Ives, European Southern Observatory (Germany);

P. Jeep, Georg-August Univ. Göttingen (Germany); Y. Jung, H.-U. Käufl, F. Kerber, B. Klein, J. Lizon, European Southern Observatory (Germany); M. Lockhart, Uppsala Univ. (Sweden);

T. Löwinger, Thüringer Landessternwarte Tautenburg (Germany); T. Marquart, Uppsala Univ.

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(Sweden); E. Oliva, INAF - Osservatorio Astrofisico di Arcetri (Italy); J. Paufique, European Southern Observatory (Germany); N. Piskunov, Uppsala Univ. (Sweden); E. Pozna, European Southern Observatory (Germany); A. Reiners, Georg-August-Univ. Göttingen (Germany);

A. Smette, J. Smoker, European Southern Observatory (Germany); E. Stempels, Uppsala Univ. (Sweden); E. Valenti, European Southern Observatory (Germany)

9147 5H Characterization of new components for a miniaturized heterodyne infrared spectrometer

[9147-209] P. Krause, Univ. zu Köln (Germany); G. Sonnabend, RPG Radiometer Physics GmbH

(Germany); L. Labadie, M. Sornig, Univ. zu Köln (Germany); R. Thomson, A. Arriola, Heriot-Watt Univ. (United Kingdom); A. Rodenas, Univ. Rovira i Virgili (Spain); T. Hewagama, Univ. of Maryland, College Park (United States); F. Rutz, Fraunhofer-Institut für Angewandte Festkörperphysik (Germany)

9147 5K MUSE from Europe to the Chilean Sky [9147-362] P. Caillier, Ctr. de Recherche Astrophysique de Lyon, CNRS, Univ. Claude-Bernard Lyon I

(France); M. Accardo, European Southern Observatory (Germany); L. Adjali, Ctr. de Recherche Astrophysique de Lyon, CNRS, Univ. Claude-Bernard Lyon I (France);

H. Anwand, Georg-August-Univ. Göttingen (Germany); R. Bacon, D. Boudon, L. Capoani, E. Daguisé, Ctr. de Recherche Astrophysique de Lyon, CNRS, Univ. Claude-Bernard Lyon I (France); M. Dupieux, Institut de Recherche en Astrophysique et Planétologie, CNRS, Univ. Paul Sabatier (France) and Observatoire Midi Pyrénées (France); C. Dupuy, European Southern Observatory (Germany); M. François, Ctr. de Recherche Astrophysique de Lyon, CNRS, Univ. Claude-Bernard Lyon I (France); A. Glindemann, D. Gojak, European Southern Observatory (Germany); F. Gonté, N. Haddad, European Southern Observatory (Chile);

G. Hansali, Ctr. de Recherche Astrophysique de Lyon, CNRS, Univ. Claude-Bernard Lyon I (France); T. Hahn, Leibniz-Institut für Astrophysik Potsdam (Germany); A. Jarno, Ctr. de Recherche Astrophysique de Lyon, CNRS, Univ. Claude-Bernard Lyon I (France); A. Kelz, Leibniz-Institut für Astrophysik Potsdam (Germany); K. Koehler, Georg-August-Univ. Göttingen (Germany); J. Kosmalski, F. Laurent, Ctr. de Recherche Astrophysique de Lyon, CNRS, Univ. Claude-Bernard Lyon I (France); M. Larrieu, Institut de Recherche en Astrophysique et Planétologie, CNRS, Univ. Paul Sabatier (France) and Observatoire Midi Pyrénées (France); J. Lizon, European Southern Observatory (Germany); M. Loupias, Ctr. de Recherche Astrophysique de Lyon, CNRS, Univ. Claude-Bernard Lyon I (France); A. Manescau, European Southern Observatory (Germany); J. E. Migniau, Ctr. de Recherche Astrophysique de Lyon, CNRS, Univ. Claude-Bernard Lyon I (France); C. Monstein, ETH Zurich (Switzerland); H. Nicklas, Georg-August-Univ. Göttingen (Germany); L. Parès, Institut de Recherche en Astrophysique et Planétologie, CNRS, Univ. Paul Sabatier (France) and Observatoire Midi Pyrénées (France); A. Pécontal-Rousset, L. Piqueras, Ctr. de Recherche Astrophysique de Lyon, CNRS, Univ. Claude-Bernard Lyon I (France); R. Reiss, European Southern Observatory (Germany); A. Remillieux, E. Renault, Ctr. de Recherche Astrophysique de Lyon, CNRS, Univ. Claude-Bernard Lyon I (France); G. Rupprecht, European Southern Observatory (Germany); O. Streicher, Leibniz-Institut für Astrophysik Potsdam (Germany); R. Stuik, Leiden Observatory, Leiden Univ. (Netherlands); H. Valentin, Institut de Recherche en Astrophysique et Planétologie, CNRS, Univ. Paul Sabatier (France) and Observatoire Midi Pyrénées (France); J. Vernet, European Southern Observatory (Germany); P. Weilbacher, Leibniz-Institut für Astrophysik Potsdam (Germany); G. Zins, Institut de Planétologie et d'Astrophysique de Grenoble, CNRS, Univ. de Grenoble 1 (France)

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9147 5L Spectrophotometric calibration of the Swope and duPont telescopes for the Carnegie supernova project 2 [9147-370]

J-P. Rheault, N. P. Mondrik, D. L. DePoy, J. L. Marshall, N. B. Suntzeff, Texas A&M Univ. (United States) POSTER SESSION: SURVEY AND HIGH MULTIPLEX INSTRUMENTS

9147 5M Fibre system of DESI [9147-210] J. Allington-Smith, Durham Univ. (United Kingdom); C. Poppett, Lawrence Berkeley National

Lab. (United States); D. Bramall, Durham Univ. (United Kingdom); J. Edelstein, Univ. of California, Berkeley (United States); R. Lafever, Lawrence Berkeley National Lab. (United States); J. Schmoll, C. Dunlop, G. Murray, Durham Univ. (United Kingdom); R. Besuner, Univ. of California, Berkeley (United States); G. Talbot, Durham Univ. (United Kingdom)

9147 5N MEGARA fiber bundles [9147-211] A. Pérez-Calpena, M. L. García-Vargas, FRACTAL S.L.N.E (Spain); X. Arrillaga, AVS Added

Value Solutions (Spain); A. Gil de Paz, Univ. Complutense de Madrid (Spain); E. Sánchez-Blanco, I. Martínez-Delgado, FRACTAL S.L.N.E (Spain); M. A. Carrera, AVS

Added Value Solutions (Spain); J. Gallego, Univ. Complutense de Madrid (Spain); E. Carrasco, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico); F. M. Sánchez-Moreno, Univ. Politécnica de Madrid (Spain); J. Iglesias-Páramo, Instituto de

Astrofísica de Andalucía (Spain) 9147 5Q Prime focus instrument of prime focus spectrograph for Subaru telescope [9147-213] S.-Y. Wang, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan); D. F. Braun,

M. A. Schwochert, Jet Propulsion Lab. (United States); P.-J. Huang, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan); M. Kimura, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan) and Kavli Institute for the Physics and Mathematics of the Universe, The Univ. of Tokyo (Japan); H.-Y. Chen, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan); D. J. Reiley, P. Mao, California Institute of Technology (United States); C. D. Fisher, Jet Propulsion Lab. (United States); N. Tamura, Kavli Institute for the Physics and Mathematics of the Universe, The Univ. of Tokyo (Japan); Y.-C. Chang, Y.-S. Hu, H.-H. Ling, C.-Y. Wen, R. C.-Y. Chou, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan); N. Takato, Subaru Telescope, National Astronomical Observatory of Japan (United States); H. Sugai, Kavli Institute for the Physics and Mathematics of the Universe, The Univ. of Tokyo (Japan); Y. Ohyama, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan); H. Karoji, A. Shimono, Kavli Institute for the Physics and Mathematics of the Universe, The Univ. of Tokyo (Japan);

A. Ueda, National Astronomical Observatory of Japan (Japan) 9147 5R MEGARA main optics opto-mechanics [9147-214] E. Castillo-Domínguez, J. L. Avilés, E. Carrasco, Instituto Nacional de Astrofísica, Óptica y

Electrónica (Mexico); M. Maldonado, FRACTAL S.L.N.E (Spain); A. Gil de Paz, J. Gallego, Univ. Complutense de Madrid (Spain); R. Cedazo, Univ. Politécnica de Madrid (Spain);

J. Iglesias, Instituto de Astrofísica de Andalucía (Spain) 9147 5S Metrology camera system of prime focus spectrograph for Subaru telescope [9147-215] S.-Y. Wang, R. C.-Y. Chou, Y.-C. Chang, P.-J. Huang, Y.-S. Hu, H.-Y. Chen, Institute of

Astronomy and Astrophysics, Academia Sinica (Taiwan); N. Tamura, Kavli Institute for the Physics and Mathematics of the Universe, The Univ. of Tokyo (Japan); N. Takato, Subaru Telescope, National Astronomical Observatory of Japan (United States); H.-H. Ling, Institute

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of Astronomy and Astrophysics, Academia Sinica (Taiwan); J. E. Gunn, Princeton Univ. (United States); J. Karr, C.-H. Yan, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan); P. Mao, California Institute of Technology (United States); Y. Ohyama, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan); H. Karoji, H. Sugai, A. Shimono, Kavli Institute for the Physics and Mathematics of the Universe, The Univ. of Tokyo (Japan);

9147 5U Multiplexed astronomical images: advantages, method, and prototype instrument [9147-217] S. Ben-Ami, B. Zackay, A. Rubin, I. Sagiv, A. Gal-Yam, E. O. Ofek, Weizmann Institute of

Science (Israel) 9147 5V BOMBOLO: A 3-arms optical imager for SOAR Observatory [9147-218] D. Guzmán, Pontificia Univ. Católica de Chile (Chile); R. Angeloni, Pontificia Univ. Católica

de Chile (Chile) and Max-Planck-Institut fur Astronomie (Germany); T. Puzia, Pontificia Univ. Católica de Chile (Chile); D. Jones, Prime Optics (Australia); A. Jordán, Pontificia Univ. Católica de Chile (Chile); T. Anguita, Univ. Andrés Bello (Chile); S. Benecchi, Planetary Science Institute (United States) and Carnegie Institution of Washington (United States);

E. Garcés, Pontificia Univ. Católica de Chile (Chile) 9147 5W MMP: multi mini prism device for ESPRESSO APSU, prototyping, and integration [9147-219] S. dell'Agostino, M. Riva, M. Genoni, M. Landoni, M. Moschetti, M. Aliverti, INAF -

Osservatorio Astronomico di Brera (Italy); F. Pepe, D. Mégevand, Observatoire de Genève (Switzerland); F. M. Zerbi, INAF - Osservatorio Astronomico di Brera (Italy); S. Cristiani, INAF - Osservatorio Astronomico di Trieste (Italy); A. Cabral, Univ. de Lisboa (Portugal);

P. Conconi, INAF - Osservatorio Astronomico di Brera (Italy) 9147 5Z Integration and test activities for the SUMIRE prime focus spectrograph at LAM [9147-222] F. Madec, J. Marc, S. Pascal, A. Bozier, D. Le Mignant, S. Vives, D. Ferrand, T. Pegot-Ogier,

G. Arthaud, Aix Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); M. Golebiowski, Johns Hopkins Univ. (United States); H. Sugai, N. Tamura, Kavli Institute for

the Physics and Mathematics of the Universe, The Univ. of Tokyo (Japan); J. Gunn, Princeton Univ. (United States); S. Smee, Johns Hopkins Univ. (United States); L. Oliveira, Lab. Nacional de Astrofísica (Brazil)

9147 60 Efficient and affordable catadioptric spectrograph designs for 4MOST and Hector [9147-223] W. Saunders, Australian Astronomical Observatory (Australia) 9147 62 Current status of the spectrograph system for the SuMIRe/PFS [9147-227] S. Vives, D. Le Mignant, Aix Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille

(France); J. E. Gunn, Princeton Univ. (United States); S. Smee, Johns Hopkins Univ. (United States); L. Souza de Oliveira, Lab. Nacional de Astrofísica (Brazil); N. Tamura, H. Sugai, Institute for the Physics and Mathematics of the Universe, The Univ. of Tokyo (Japan);

R. Barkhouser, Johns Hopkins Univ. (United States); A. Bozier, Aix Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); M. A. Carr, Princeton Univ. (United States);

A. C. de Oliveira, Lab. Nacional de Astrofísica (Brazil); D. Ferrand, Aix Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); M. Golebiowski, M. Hart, S. Hope, Johns Hopkins Univ. (United States); M. Jaquet, F. Madec, S. Pascal, T. Pegot-Ogier, Aix Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); M. Vital de Arruda, Lab. Nacional de Astrofísica (Brazil)

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9147 63 Focal ratio degradation performance of fiber positioning technology used in the Dark Energy Spectroscopic Instrument (DESI) [9147-228]

C. L. Poppett, Lawrence Berkeley National Lab. (United States); J. Edelstein, R. Besuner, Space Sciences Lab. (United States); J. H. Silber, Lawrence Berkeley National Lab.

(United States) 9147 64 Virtual MOONS: a focal plane simulator for the MOONS thousand-fiber NIR spectrograph

[9147-229] G. Li Causi, INAF - Osservatorio Astronomico di Roma (Italy); A. Cabral, Univ. of Lisbon

(Portugal); D. Ferruzzi, INAF - Osservatorio Astrofisico di Arcetri (Italy); G. Finger, European Southern Observatory (Germany); G. Giacalone, Univ. di Roma La Sapienza (Italy);

I. Guinouard, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); D. Lorenzetti, INAF - Osservatorio Astronomico di Roma (Italy); E. Oliva, INAF - Osservatorio Astrofisico di Arcetri (Italy); F. Pedichini, INAF - Osservatorio Astronomico di Roma (Italy); F. Royer, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); S. Todd, STFC UK Astronomy Technology Ctr. (United Kingdom); F. Vitali, INAF - Osservatorio Astronomico di Roma (Italy)

9147 65 Design and performance of a F/#-conversion microlens for prime focus spectrograph at

Subaru Telescope [9147-230] N. Takato, Y. Tanaka, Subaru Telescope, National Astronomical Observatory of Japan

(United States); J. E. Gunn, Princeton Univ. (United States); N. Tamura, A. Shimono, H. Sugai, H. Karoji, Kavli Institute for the Physics and Mathematics of the Universe, The Univ. of Tokyo (Japan); A. Ueda, K. Waseda, National Astronomical Observatory of Japan (Japan);

M. Kimura, Y. Ohyama, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan) 9147 66 Preliminary results on the characterization and performances of ZBLAN fiber for infrared

spectrographs [9147-231] M. Iuzzolino, A. Tozzi, N. Sanna, L. Zangrilli, E. Oliva, INAF - Osservatorio Astrofisico di Arcetri

(Italy) 9147 67 The hardware control system for WEAVE at the William Herschel telescope [9147-232] J. M. Delgado Hernandez, L. F. Rodríguez-Ramos, Instituto de Astrofísica de Canarias

(Spain); D. Cano Infantes, C. Martin, C. Bevil, S. Picó, K. M. Dee, D. C. Abrams, Isaac Newton Group of Telescopes (Spain); I. J. Lewis, Univ. of Oxford (United Kingdom); J. Pragt, R. Stuik, N. Tromp, NOVA ASTRON (Netherlands); G. Dalton, Univ. of Oxford (United Kingdom); J. A. L. Aguerri, Univ. de La Laguna (Spain); P. Bonifacio, Observatoire de Paris à Meudon (France); K. F. Middleton, Rutherford Appleton Lab. (United Kingdom);

S. C. Trager, Univ. of Groningen (Netherlands) Part Four 9147 6A 4MOST fiber feed concept design [9147-235] D. M. Haynes, R. Winkler, A. Saviauk, R. Haynes, S. Barden, O. Bellido-Tirado, S. Bauer, R. S. de Jong, Leibniz-Institut für Astrophysik Potsdam (Germany); E. Depagne, South

African Astronomical Observatory (South Africa); F. Dionies, K. Ehrlich, A. Kelz, Leibniz-Institut für Astrophysik Potsdam (Germany); W. Saunders, Australian Astronomical Observatory (Australia); M. Woche, Leibniz-Institut für Astrophysik Potsdam (Germany)

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9147 6B Scrambling and modal noise mitigation in the Habitable Zone Planet Finder fiber feed [9147-236]

A. Roy, S. Halverson, S. Mahadevan, L. W. Ramsey, The Pennsylvania State Univ. (United States) 9147 6C Development of a new readout system for the near-infrared detector of HONIR [9147-237] T. Ui, Hiroshima Univ. (Japan); S. Sako, The Univ. of Tokyo (Japan); T. Yamashita, National

Astronomical Observatory of Japan (Japan); H. Akitaya, K. S. Kawabata, Hiroshima Univ. (Japan); H. Nakaya, National Astronomical Observatory of Japan (Japan); Y. Moritani,

R. Itoh, K. Takaki, T. Urano, I. Ueno, T. Ohsugi, M. Yoshida, Hiroshima Univ. (Japan); H. Nakao, Hokkaido Univ. (Japan); Y. Hashiba, The Univ. of Tokyo (Japan) 9147 6D Okayama astrophysical observatory wide field camera [9147-238] K. Yanagisawa, Y. Shimizu, K. Okita, D. Kuroda, H. Koyano, H. Tsutsui, H. Toda, H. Izumiura,

National Astronomical Observatory of Japan (Japan); M. Yoshida, Hiroshima Univ. (Japan); K. Ohta, Kyoto Univ. (Japan); N. Kawai, Tokyo Institute of Technology (Japan);

T. Yamamuro, OptCraft (Japan) 9147 6E Polarization properties of a birefringent fiber optic image slicer for diffraction-limited dual-

beam spectropolarimetry [9147-239] T. Schad, H. Lin, Institute for Astronomy, Univ. of Hawai'i (United States); K. Ichimoto, Kyoto

Univ. (Japan); Y. Katsukawa, National Astronomical Observatory of Japan (Japan) 9147 6F The S4I prototype, a beam-slicer dedicated to the new generation Multichannel

Subtractive Double Pass for EST imaging spectropolarimetry [9147-240] F. Sayède, GEPI, Observatoire de Paris (France); P. Mein, J.-M. Malherbe, LESIA,

Observatoire de Paris (France); J.-P. Amans, GEPI, Observatoire de Paris (France); D. Crussaire, R. Lecocguen, LESIA, Observatoire de Paris (France) 9147 6H The design of the WEAVE spectrograph [9147-242] K. Rogers, STFC Rutherford Appleton Lab. (United Kingdom); R. Stuik, NOVA ASTRON

(Netherlands) and Leiden Observatory, Leiden Univ. (Netherlands); I. A. Steele, Liverpool John Moores Univ. (United Kingdom); J. Pragt, NOVA ASTRON (Netherlands);

K. F. Middleton, STFC Rutherford Appleton Lab. (United Kingdom); S. Bates, Liverpool John Moores Univ. (United Kingdom); J. Kragt, N. Tromp, D. Lesman, NOVA ASTRON (Netherlands); E. Lhomé, Isaac Newton Group of Telescopes (Spain); G. Dalton, STFC Rutherford Appleton Lab. (United Kingdom) and Univ. of Oxford (United Kingdom);

S. Trager, Univ. of Groningen (Netherlands); R. Navarro, NOVA ASTRON (Netherlands); D. C. Abrams, Isaac Newton Group of Telescopes (Spain); I. Tosh, STFC Rutherford Appleton

Lab. (United Kingdom); A. Jasko, Konkoly Thege Miklós Astronomical Institute (Hungary); C. Martin, N. O'Mahony, S. Pico, D. Cano Infantes, Isaac Newton Group of Telescopes

(Spain); A. Bianca, INAF - Osservatorio Astronomico di Brera (Italy); J. Delgado, L. F. Rodríguez, Instituto de Astrofísica de Canarias (Spain) 9147 6I The 4MOST instrument concept overview [9147-243] R. Haynes, S. Barden, R. de Jong, O. Schnurr, O. Bellido, J. Walcher, D. Haynes, R. Winkler, S.-M. Bauer, F. Dionies, A. Saviauk, C. Chiappini, A. Schwope, J. Brynnel, M. Steinmetz, Leibniz-Institut für Astrophysik Potsdam (Germany); R. McMahon, Univ. of

Cambridge (United Kingdom); S. Feltzing, Lund Observatory (Sweden); P. Francois, GEPI, Observatoire de Paris à Meudon (France); S. Trager, Kapteyn Astronomical Institute, Univ. of Groningen (Netherlands); I. Parry, M. Irwin, N. Walton, D. King, Univ. of Cambridge (United Kingdom); D. Sun, Cavendish Lab., Univ. of Cambridge (United Kingdom);

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E. Gonzalez-Solares, Univ. of Cambridge (United Kingdom); I. Tosh, Rutherford Appleton Lab. (United Kingdom); G. Dalton, Univ. of Oxford (United Kingdom); K. Middleton, Rutherford Appleton Lab. (United Kingdom); P. Bonifacio, P. Jagourel, S. Mignot, M. Cohen, J.-P. Amans, F. Royer, P. Sartoretti, GEPI, Observatoire de Paris à Meudon (France); J. Pragt, G. Gerlofsma, R. Roelfsema, R. Navarro, ASTRON (Netherlands); G. Thimm, Univ. Heidelberg (Germany); W. Seifert, N. Christlieb, H. Mandel, Landessternwarte, Zentrum für Astronomie der Univ. Heidelberg (Germany); T. Trifonov, Univ. Heidelberg (Germany); W. Xu, Optical System Engineering (Germany);F. Lang-Bardl, B. Muschielok, J. Schlichter, H.-J. Hess, Univ.-Sternwarte München (Germany); F. Grupp, H. Boehringer, T. Boller, T. Dwelly, R. Bender, Max-Planck-Institut für extraterrestrische Physik (Germany); P. Rosati, O. Iwert, G. Finger, J.-L. Lizon L'Allemand, European Southern Observatory (Germany); W. Saunders, A. Sheinis, G. Frost, T. Farrell, L. Waller, Australian Astronomical Observatory (Australia); E. Depagne, Leibniz-Institut für Astrophysik Potsdam (Germany) and South African Astronomical Observatory (South Africa); F. Laurent, P. Caillier, J. Kosmalski, J. Richard, R. Bacon, Ctr. de Recherche Astrohysique de Lyon (France); W. Ansorge, RAMS-CON (Germany)

9147 6K Development of a simultaneous two-color near-infrared multi-object spectrograph SWIMS

for the TAO 6.5-m telescope [9147-245] K. Motohara, M. Konishi, H. Takahashi, K. Tateuchi, Y. Kitagawa, S. Todo, N. M. Kato, R. Ohsawa, The Univ. of Tokyo (Japan); T. Aoki, Kiso Observatory, The Univ. of Tokyo

(Japan); K. Asano, M. Doi, T. Kamizuka, K. Kawara, K. Kohno, The Univ. of Tokyo (Japan); S. Koshida, The Univ. of Tokyo (Japan) and Pontificia Univ. Católica de Chile (Chile); T. Minezaki, T. Miyata, T. Morokuma, K. Okada, S. Sako, The Univ. of Tokyo (Japan); T. Soyano, Kiso Observatory, The Univ. of Tokyo (Japan); Y. Tamura, T. Tanabe, M. Tanaka,

The Univ. of Tokyo (Japan); K. Tarusawa, Kiso Observatory, The Univ. of Tokyo (Japan); M. Uchiyama, Y. Yoshii, The Univ. of Tokyo (Japan) 9147 6L Sky background subtraction with fiber-fed spectrographs [9147-246] M. Puech, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); M. Rodrigues,

GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France) and European Southern Observatory (Chile); Y. Yang, H. Flores, F. Royer, K. Disseau, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); T. Gonçalves, Univ. Federal do Rio de Janeiro (Brazil);

F. Hammer, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); M. Cirasuolo, SUPA, Institute for Astronomy, Univ. of Edinburgh, Royal Observatory (United Kingdom);

C. J. Evans, UK Astronomy Technology Ctr. (United Kingdom); G. Li Causi, INAF - Osservatorio Astronomico di Roma (Italy); R. Maiolino, Univ. of Cambridge (United Kingdom); C. Melo, European Southern Observatory (Chile)

9147 6M Accuracy research for survey telescope fiber position measurement [9147-247] Z. Zhou, Z. Liu, H. Hu, J. Wang, C. Zhai, J. Chu, Univ. of Science and Technology of China

(China) 9147 6N Development of multi-object spectroscopy unit for simultaneous-color wide-field infrared

multi-object spectrograph [9147-248] H. Takahashi, M. Konishi, K. Motohara, N. M. Kato, K. Tateuchi, Y. Kitagawa, S. Todo, The

Univ. of Tokyo (Japan) 9147 6P Achieving decameter velocity precision with a multi-object spectrograph [9147-251] J. I. Bailey III, M. L. Mateo, Univ. of Michigan (United States); J. D. Crane, Carnegie

Observatories (United States)

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9147 6Q Wide FastCam: a wide field imaging camera for the TCS [9147-252] G. Murga, IDOM (Spain); A. Oscoz, R. López, Instituto de Astrofísica de Canarias (Spain); R. Campo, U. Etxegarai, IDOM (Spain); E. Pallé, Instituto de Astrofísica de Canarias (Spain) 9147 6R The DESI wide field corrector optics [9147-253] P. Doel, Univ. College London (United Kingdom); M. J. Sholl, Lawrence Berkeley National

Lab. (United States); M. Liang, National Optical Astronomy Observatory (United States); D. Brooks, Univ. College London (United Kingdom); B. Flaugher, G. Gutierrez, S. Kent, Fermi National Accelerator Lab. (United States); M. Lampton, T. Miller, Lawrence Berkeley National Lab. (United States); D. Sprayberry, National Optical Astronomy Observatory (United States)

9147 6S MEGARA cryostat advanced design [9147-254] D. Ferrusca, E. Castillo-Domínguez, M. Velázquez, Instituto Nacional de Astrofísica, Óptica y

Electrónica (Mexico); A. Gil de Paz, Univ. Complutense de Madrid (Spain); E. Carrasco, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico); J. Gallego, Univ. Complutense de Madrid (Spain); R. Cedazo, Univ. Politécnica de Madrid (Spain);

J. Iglesias-Páramo, Instituto de Astrofísica de Andalucia (Spain) 9147 6T Performance of the Southern African Large Telescope (SALT) High Resolution Spectrograph

(HRS) [9147-256] L. A. Crause, South African Astronomical Observatory (South Africa); R. M. Sharples, D. G. Bramall, J. Schmoll, P. Clark, E. J. Younger, Durham Univ. (United Kingdom); L. M. G. Tyas, SALT Foundation (South Africa); S. G. Ryan, Univ. of Hertfordshire (United Kingdom); J. D. Brink, O. J. Strydom, D. A. Buckley, M. Wilkinson, SALT Foundation

(South Africa); S. M. Crawford, Southern African Large Telescope (South Africa); É. Depagne, SALT Foundation (South Africa) 9147 6U VIRUS instrument enclosures [9147-257] T. Prochaska, R. Allen, N. Mondrik, J. P. Rheault, M. Sauseda, E. Boster, M. James, M. Rodriguez-Patino, G. Torres, J. Ham, E. Cook, D. Baker, D. L. DePoy, J. L. Marshall, Texas

A&M Univ. (United States); G. J. Hill, McDonald Observatory, The Univ. of Texas at Austin (United States) and The Univ. of Texas at Austin (United States); D. Perry, R. D. Savage, J. M. Good, B. L. Vattiat, McDonald Observatory, The Univ. of Texas at Austin (United States);

9147 6V Presenting a high accuracy Theta-Phi-style fiber-positioner prototype with a 15-mm pitch [9147-258]

M. Haeuser, F. Lang-Bardl, J. Richter, H.-J. Hess, A. Degwert, A. Karasz, R. Kosyra, Univ.-Sternwarte München (Germany); U. Hopp, R. Bender, Univ.-Sternwarte München

(Germany) and Max-Planck-Institut für extraterrestrische Physik (Germany) 9147 6X ROS2: a multichannel vision for the robotic REM telescope [9147-260] E. Molinari, INAF - Istituto di Astrofisica Spaziale e Fisica Cosmica (Italy) and INAF -

Fundación Galileo Galilei (Spain); S. Covino, G. Crimi, INAF - Osservatorio Astronomico di Brera (Italy); F. D'Alessio, INAF - Osservatorio Astronomico di Roma (Italy); S. Incorvaia, INAF - Istituto di Astrofisica Spaziale e Fisica Cosmica (Italy); D. Fugazza, INAF - Osservatorio Astronomico di Brera (Italy); P. Spanò, NRC - Herzburg Institute of Astrophysics (Canada); G. Toso, D. Tresoldi, INAF - Istituto di Astrofisica Spaziale e Fisica Cosmica (Italy); F. Vitali, INAF - Osservatorio Astronomico di Brera (Italy)

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9147 6Y Towards a spectroscopic survey of one hundred thousand spatially resolved galaxies with Hector [9147-261]

J. S. Lawrence, Australian Astronomical Observatory (Australia); J. Bland-Hawthorn, The Univ. of Sydney (Australia); D. Brown, Australian Astronomical Observatory (Australia);

J. J. Bryant, Australian Astronomical Observatory (Australia) and The Univ. of Sydney (Australia); G. Cecil, The Univ. of North Carolina (United States); R. Content, Australian Astronomical Observatory (Australia); S. Croom, The Univ. of Sydney (Australia); L. Gers,

P. R. Gillingham, Australian Astronomical Observatory (Australia); S. Richards, The Univ. of Sydney (Australia); W. Saunders, N. Staszak, Australian Astronomical Observatory (Australia)

9147 6Z Monitoring the atmospheric throughput at Cerro Tololo Inter-American Observatory with

aTmCam [9147-262] T. Li, D. L. DePoy, J. L. Marshall, D. Q. Nagasawa, D. W. Carona, S. Boada, Texas A&M Univ.

(United States) 9147 70 Methods for the detection and the characterization of low mass companions using the IFS

of SPHERE [9147-263] A. Zurlo, Aix Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France) and INAF -

Osservatorio Astronomico di Padova (Italy); D. Mesa, R. Gratton, R. Claudi, S. Desidera, E. Giro, INAF - Osservatorio Astronomico di Padova (Italy); J.-L. Beuzit, Univ. Joseph Fourier-

Grenoble1, CNRS-INSU, Institut de Planétologie et d’Astrophysique de Grenoble (France); K. Dohlen, Aix Marseille Univ., CNRS, Lab. d’Astrophysique de Marseille (France); D. Mouillet, P. Puget, Univ. Joseph Fourier-Grenoble1, CNRS-INSU, Institut de Planétologie et d’Astrophysique de Grenoble (France); F. Wildi, Observatoire de Genève, Univ. de Genève (Switzerland); M. Feldt, O. Moeller-Nilsson, Max-Planck-Institut für Astronomie (Germany); A. Baruffolo, D. Fantinel, B. Salasnich, INAF - Osservatorio Astronomico di Padova (Italy); M. Kasper, European Southern Observatory (Germany); A. Costille, Aix Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); J.-F. Sauvage, ONERA (France); A. Vigan, C. Moutou, Aix Marseille Univ., CNRS, Lab. d’Astrophysique de Marseille (France); M. Langlois, Ctr. de Recherche Astronomique de Lyon, CNRS, Univ. Lyon 1 (France); J. Antichi, INAF - Osservatorio Astrofisico di Arcetri (Italy); A. Pavlov, Max-Planck-Institut für Astronomie (Germany); N. Zimmerman, European Southern Observatory (Germany); M. Turatto, INAF - Osservatorio Astronomico di Padova (Italy)

9147 71 MEGARA optical manufacturing process [9147-264] E. Carrasco, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico); G. Páez, Ctr.

de Investigaciones en Óptica (Mexico); F. Granados, E. Percino, E. Castillo-Domínguez, J. L. Avilés, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico); M. L. García-

Vargas, Fractal S.L.N.E (Spain); A. Gil de Paz, J. Gallego, Univ. Complutense de Madrid (Spain); J. Iglesias-Páramo, Instituto de Astrofísica de Andalucía (Spain); R. Cedazo, Univ. Politécnica de Madrid (Spain)

9147 72 High speed wide field CMOS camera for Transneptunian Automatic Occultation Survey

[9147-265] S.-Y. Wang, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan); J. C. Geary, S. M. Amato, Harvard-Smithsonian Ctr. for Astrophysics (United States); Y.-S. Hu, H.-H. Ling, P.-J. Huang, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan); G. Furesz, Harvard-Smithsonian Ctr. for Astrophysics (United States); H.-Y. Chen, Y.-C. Chang, Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan); A. Szentgyorgyi, Harvard-Smithsonian Ctr. for Astrophysics (United States); M. Lehner,

Institute of Astronomy and Astrophysics, Academia Sinica (Taiwan); T. Norton, Harvard-Smithsonian Ctr. for Astrophysics (United States)

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9147 73 Final optical design for the WEAVE two-degree prime focus corrector [9147-266] T. Agócs, NOVA ASTRON (Netherlands); D. C. Abrams, E. Lhomé, K. Dee, Isaac Newton

Group of Telescopes (Spain); G. Dalton, STFC Rutherford Appleton Lab. (United Kingdom) and Univ. of Oxford (United Kingdom); K. Middleton, STFC Rutherford Appleton Lab. (United Kingdom); P. Bonifacio, GEPI, Observatoire de Paris (France); J. A. L. Aguerri, Instituto de Astrofísica de Canarias (Spain); S. C. Trager, Univ. of Groningen (Netherlands)

9147 74 The guider and wavefront curvature sensor subsystem for the Large Synoptic Survey

Telescope [9147-267] V. J. Riot, Lawrence Livermore National Lab. (United States); K. Arndt, Purdue Univ. (United

States); C. Claver, Large Synoptic Survey Telescope (United States); P. E. Doherty, Harvard Univ. (United States); D. K. Gilmore, P. A. Hascall, S. Herrmann, SLAC National Accelerator Lab. (United States); I. Kotov, P. O'Connor, Brookhaven National Lab. (United States);

J. Sebag, Large Synoptic Survey Telescope (United States); C. W. Stubbs, Harvard Univ. (United States); M. Warner, Cerro Tololo Inter-American Observatory (Chile)

9147 75 VIRUS: assembly, testing and performance of 33,000 fibres for HETDEX [9147-269] A. Kelz, T. Jahn, D. Haynes, Leibniz-Institut für Astrophysik Potsdam (Germany); G. J. Hill, H. Lee, J. D. Murphy, The Univ. of Texas at Austin (United States); J. Neumann, Leibniz-Institut

für Astrophysik Potsdam (Germany); H. Nicklas, Georg-August-Univ. Göttingen (Germany); M. Rutowska, C. Sandin, O. Streicher, Leibniz-Institut für Astrophysik Potsdam (Germany);

S. Tuttle, The Univ. of Texas at Austin (United States); M. Fabricius, Max-Planck-Institut für extraterrestrische Physik (Germany); S. M. Bauer, Leibniz-Institut für Astrophysik Potsdam (Germany); B. Vattiat, The Univ. of Texas at Austin (United States); H. Anwand, Georg-August-Univ. Göttingen (Germany); R. Savage, The Univ. of Texas at Austin (United States)

9147 77 A multi-pixel room-temperature local oscillator subsystem for array receivers at 1.9 THz

[9147-272] J. V. Siles, I. Mehdi, C. Lee, R. Lin, J. Kawamura, E. Schlecht, P. J. Bruneau, P. F. Goldsmith,

Jet Propulsion Lab. (United States) 9147 78 Multi-object fibre spectroscopy at the WHT: performance enhancements of AF2+WYFFOS

[9147-374] L. Domínquez Palmero, D. Cano, C. Fariña, R. Bassom, E. Lhomé, N. O'Mahony, J. Skvarc,

A. Ridings, C. R. Benn, D. C. Abrams, M. Balcells, Isaac Newton Group of Telescopes (Spain) 9147 79 The Zwicky transient facility observing system [9147-375] R. M. Smith, R. G. Dekany, Caltech Optical Observatories (United States); C. Bebek,

Lawrence Berkeley National Lab. (United States); E. Bellm, K. Bui, J. Cromer, P. Gardner, Caltech Optical Observatories (United States); M. Hoff, Lawrence Berkeley National Lab. (United States); S. Kaye, S. Kulkarni, Caltech Optical Observatories (United States);

A. Lambert, M. Levi, Lawrence Berkeley National Lab. (United States); D. Reiley, Caltech Optical Observatories (United States)

POSTER SESSION: HIGH SPECTRAL AND SPATIAL RESOLUTION INSTRUMENTS 9147 7B Gemini planet imager observational calibrations X: non-redundant masking on GPI [9147-135] A. Z. Greenbaum, Johns Hopkins Univ. (United States); A. Cheetham, The Univ. of Sydney

(Australia); A. Sivaramakrishnan, P. Tuthill, B. Norris, Space Telescope Science Institute (Australia); L. Pueyo, The Univ. of Sydney (United States); N. Sadakuni, F. Rantakyrö,

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P. Hibon, S. Goodsell, M. Hartung, A. Serio, A. Cardwell, Gemini Observatory (Chile); L. Poyneer, Lawrence Livermore National Lab. (United States); B. Macintosh, Lawrence

Livermore National Lab. (United States) and Kavli Institute for Particle Astrophysics and Cosmology, Stanford Univ. (United States); D. Savransky, Cornell Univ. (United States);

M. D. Perrin, The Univ. of Sydney (Australia); S. Wolff, Johns Hopkins Univ. (United States); P. Ingraham, Kavli Institute for Particle Astrophysics and Cosmology, Stanford Univ. (United

States); S. Thomas, NASA Ames Research Ctr. (United States) 9147 7C InnoPOL: an EMCCD imaging polarimeter and 85-element curvature AO system on the 3.6-

m AEOS telescope for cost effective polarimetric speckle suppression [9147-274] D. Harrington, Institute for Astronomy, Univ. of Hawai'i (United States) and Kiepenheuer-

Institut für Sonnenphysik (Germany); S. Berdyugina, Kiepenheuer-Institut für Sonnenphysik (Germany); M. Chun, C. Ftaclas, Institute for Astronomy, Univ. of Hawai'i (United States);

D. Gisler, Kiepenheuer-Institut für Sonnenphysik (Germany); J. Kuhn, Institute for Astronomy, Univ. of Hawai'i (United States)

9147 7D APSU @ ESPRESSO: final design towards the integration [9147-275] M. Riva, P. Conconi, M. Moschetti, S. Dell'Agostino, M. Genoni, M. Aliverti, INAF -

Osservatorio Astronomico di Brera (Italy); F. Pepe, D. Mégevand, Observatoire de Genève, Univ. de Genève (Switzerland); F. M. Zerbi, INAF - Osservatorio Astronomico di Brera (Italy); S. Cristiani, INAF - Osservatorio Astronomico di Trieste (Italy); A. Cabral, Univ. de Lisboa (Portugal); P. Spanò, NRC - Herzberg Institute de Astrophysics (Canada)

9147 7F Design of a radial velocity spectrograph for the Moletai Astronomical Observatory [9147-277] C. A. Jurgenson, D. A. Fischer, T. M. McCracken, R. A. Stoll, A. E. Szymkowiak, M. J. Giguere,

Yale Univ. (United States); F. G. Santoro, G. Muller, ASTRO Electro-Mechanical Engineering (United States)

9147 7G ESPRESSO front end: modular opto-mechanical integration for astronomical instrumentation

[9147-278] M. Riva, M. Aliverti, M. Moschetti, M. Landoni, S. Dell'Agostino, INAF - Osservatorio

Astronomico di Brera (Italy); F. Pepe, D. Mégevand, Observatoire de Genève, Univ. de Genève (Switzerland); F. M. Zerbi, INAF - Osservatorio Astronomico di Brera (Italy);

S. Cristiani, INAF - Osservatorio Astronomico di Trieste (Italy); A. Cabral, Univ. de Lisboa (Portugal)

9147 7H Gemini planet imager observational calibrations IV: wavelength calibration and flexure

correction for the integral field spectograph [9147-279] S. G. Wolff, Johns Hopkins Univ. (United States); M. D. Perrin, Space Telescope Science

Institute (United States); J. Maire, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada); P. J. Ingraham, Stanford Univ. (United States); F. T. Rantakyrö, P. Hibon, Gemini Observatory (Chile)

9147 7I RHEA: the ultra-compact replicable high-resolution exoplanet and asteroseismology

spectrograph [9147-280] T. Feger, C. Bacigalupo, Macquarie Univ. (Australia); T. R. Bedding, The Univ. of Sydney

(Australia); J. Bento, D. W. Coutts, Macquarie Univ. (Australia); M. J. Ireland, Australian National Univ. (Australia); Q. A. Parker, Macquarie Univ. (Australia) and Australian Astronomical Observatory (Australia); A. Rizzuto, I. Spaleniak, Macquarie Univ. (Australia)

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9147 7J SHARK (System for coronagraphy with High order Adaptive optics from R to K band), a proposal for the LBT 2nd generation instrumentation [9147-281]

J. Farinato, INAF - Osservatorio Astronomico di Padova (Italy); F. Pedichini, INAF - Osservatorio Astronomico di Roma (Italy); E. Pinna, INAF - Osservatorio Astrofisico di Arcetri (Italy); F. Bacciotti, C. Baffa, INAF - Osservatorio Astronomico di Arcetri (Italy); A. Baruffolo,

M. Bergomi, INAF - Osservatorio Astronomico di Padova (Italy); P. Bruno, INAF - Osservatorio Astrofisico di Catania (Italy); E. Cappellaro, INAF - Osservatorio Astronomico di Padova (Italy); L. Carbonaro, INAF - Osservatorio Astronomico di Arcetri (Italy); A. Carlotti, Institut de Planétologie et d'Astrophysique de Grenoble (France); M. Centrone, INAF - Osservatorio Astronomico di Roma (Italy); L. Close, J. Codona, Steward Observatory, The Univ. of Arizona (United States); S. Desidera, M. Dima, INAF - Osservatorio Astronomico di Padova (Italy); S. Esposito, INAF - Osservatorio Astronomico di Arcetri (Italy); D. Fantinel, G. Farisato, INAF - Osservatorio Astronomico di Padova (Italy); A. Fontana, INAF - Osservatorio Astronomico di Roma (Italy); W. Gaessler, Max-Planck-Institut für Astronomie (Germany); E. Giallongo, INAF - Osservatorio Astronomico di Roma (Italy); R. Gratton, INAF - Osservatorio Astronomico di Padova (Italy); D. Greggio, INAF - Osservatorio Astronomico di Padova (Italy) and Univ. degli Studi di Padova (Italy); J. C. Guerra, O. Guyon, P. Hinz, Steward Observatory, The Univ. of Arizona (United States); F. Leone, Univ. degli Studi di Catania (Italy); F. Lisi, INAF - Osservatorio Astronomico di Arcetri (Italy); D. Magrin, INAF - Osservatorio Astronomico di Padova (Italy); L. Marafatto, INAF - Osservatorio Astronomico di Padova (Italy) and Univ. di Padova (Italy); M. Munari, I. Pagano, INAF - Osservatorio Astrofisico di Catania (Italy); A. Puglisi, INAF - Osservatorio Astronomico di Arcetri (Italy); R. Ragazzoni, B. Salasnich, INAF - Osservatorio Astronomico di Padova (Italy); E. Sani, INAF - Osservatorio Astronomico di Arcetri (Italy); S. Scuderi, INAF - Osservatorio Astrofisico di Catania (Italy); M. Stangalini, V. Testa, INAF - Osservatorio Astronomico di Roma (Italy); C. Verinaud, Institut de Planétologie et d'Astrophysique de Grenoble (France); V. Viotto, INAF - Osservatorio Astronomico di Padova (Italy)

9147 7K Gemini planet imager observational calibrations III: empirical measurement methods and

applications of high-resolution microlens PSFs [9147-282] P. Ingraham, Kavli Institute for Particle Astrophysics and Cosmology, Stanford Univ. (United

States) and Univ. de Montréal (Canada); J.-B. Ruffio, SETI Institute (United States) and Institut Supérieur de l’Aéronautique et de l’Espace (Canada); M. D. Perrin, S. G. Wolff, Space Telescope Science Institute (United States); Z. H. Draper, Univ. of Victoria (Canada); J. Maire, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada);

F. Marchis, SETI Institute (United States); V. Fesquet, Gemini Observatory (Chile) 9147 7M A laser locked Fabry-Perot etalon with 3 cm/s stability for spectrograph calibration [9147-284] Y. V. Gurevich, Yale Univ. (United States); J. Stürmer, Landessternwarte Heidelberg

(Germany); C. Schwab, The Pennsylvania State Univ. (United States); T. Führer, Technische Univ. Darmstadt (Germany); S. K. Lamoreaux, Yale Univ. (United States); A. Quirrenbach, Landessternwarte Heidelberg (Germany); T. Walther, Technische Univ. Darmstadt (Germany)

9147 7O Gemini planet imager observational calibrations II: detector performance and calibration

[9147-286] P. Ingraham, Kavli Institute for Particle Astrophysics and Cosmology, Stanford Univ. (United

States) and Univ. de Montréal (Canada); M. D. Perrin, Space Telescope Science Institute (United States); N. Sadakuni, Gemini Observatory (Chile); J.-B. Ruffio, SETI Institute (United States) and Institut Supérieur de l’Aéronautique et de l’Espace (France); J. Maire, Dunlap

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Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada); J. Chilcote, J. Larkin, Univ. of California, Los Angeles (United States); F. Marchis, SETI Institute (United States);

R. Galicher, LESIA, CNRS, Observatoire de Paris, Univ. Paris Diderot (France); J. Weiss, Univ. of California, Los Angeles (United States)

9147 7P How to inject light efficiently into single-mode fibers [9147-287] N. Jovanovic, Subaru Telescope, National Astronomical Observatory of Japan (United

States); O. Guyon, Subaru Telescope, National Astronomical Observatory of Japan (United States) and Steward Observatory, Univ. of Arizona (United States); F. Martinache, Observatoire de la Côte d’Azur (France); C. Schwab, The Pennsylvania State Univ. (United States); N. Cvetojevic, The Univ. of Sydney (Australia) and The Australian Astronomical Observatory (Australia)

9147 7Q Manufacturing, integration, and test results of the MATISSE cold optics bench [9147-288] F. C. M. Bettonvil, NOVA ASTRON (Netherlands) and Leiden Univ. (Netherlands); G. Kroes, T. Agoćs, NOVA ASTRON (Netherlands); A. van Duin, ASTRON (Netherlands); E. Elswijk, M. de Haan, R. ter Horst, J. Kragt, NOVA ASTRON (Netherlands); J. Kuindersma, ASTRON

(Netherlands); R. Navarro, R. Roelfsema, M. Schuil, T. Tromp, L. Venema, NOVA ASTRON (Netherlands); F. van Kessel, Irmato Group (Netherlands); A. Jaskó, MTA Research Ctr. for Astronomy and Earth Sciences (Hungary)

9147 7R Concept and optical design of the cross-disperser module for CRIRES+ [9147-289] E. Oliva, A. Tozzi, D. Ferruzzi, INAF - Osservatorio Astrofisico di Arcetri (Italy); L. Origlia, INAF -

Osservatorio Astronomico di Bologna (Italy); A. Hatzes, R. Follert, T. Löwinger, Thüringer Landessternwarte Tautenburg (Germany); N. Piskunov, U. Heiter, M. Lockhart,

T. Marquart, E. Stempels, Uppsala Univ. (Sweden); A. Reiners, G. Anglada-Escude, U. Seemann, Georg-August-Univ. Göttingen (Germany); R. J. Dorn, P. Bristow, D. Baade, B. Delabre, D. Gojak, J. Grunhut, B. Klein, M. Hilker, D. J. Ives, Y. Jung, H. U. Kaeufl, F. Kerber, J. L. Lizon, L. Pasquini, J. Paufique, E. Pozna, A. Smette, J. Smoker, E. Valenti, European

Southern Observatory (Germany) 9147 7S Opto-mechanical design of a new cross dispersion unit for the CRIRES+ high resolution

spectrograph for the VLT [9147-290] J. L. Lizon, B. Klein, European Southern Observatory (Germany); E. Oliva, INAF - Osservatorio

di Arcetri (Italy); T. Löwinger, Thüringer Landessternwarte Tautenburg (Germany); G. Anglada Escude, Georg-August-Univ. Göttingen (Germany); D. Baade, P. Bristow, R. J. Dorn, European Southern Observatory (Germany); R. Follert, Thüringer

Landessternwarte Tautenburg (Germany); J. Grunhut, European Southern Observatory (Germany); A. Hatzes, Thüringer Landessternwarte Tautenburg (Germany); U. Heiter, Uppsala Univ. (Sweden); D. Ives, Y. Jung, F. Kerber, M. Lockhart, European Southern Observatory (Germany); T. Marquart, Uppsala Univ. (Sweden); L. Origlia, INAF - Osservatorio di Bologna (Italy); L. Pasquini, J. Paufique, European Southern Observatory (Germany);

N. Piskunov, Uppsala Univ. (Sweden); E. Pozna, European Southern Observatory (Germany); A. Reiners, Georg-August-Univ. Göttingen (Germany); A. Smette, J. Smoker, European Southern Observatory (Germany); U. Seemann, Georg-August-Univ. Göttingen (Germany);

E. Stempels, INAF - Osservatorio di Arcetri (Italy); E. Valenti, European Southern Observatory (Germany)

9147 7T HiJaK: the high-resolution J, H and K spectrometer [9147-291] P. S. Muirhead, Z. J. Hall, M. J. Veyette, Boston Univ. (United States)

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9147 7U Combining vector-phase coronagraphy with dual-beam polarimetry [9147-293] F. Snik, G. Otten, M. Kenworthy, Leiden Observatory, Leiden Univ. (Netherlands); D. Mawet,

European Southern Observatory (Chile); M. Escuti, North Carolina State Univ. (United States)

9147 7V An atmospheric turbulence and telescope simulator for the development of AOLI [9147-294] M. Puga, R. López, Instituto de Astrofísica de Canarias (Spain) and Univ. de La Laguna

(Spain); D. King, Univ. of Cambridge (United Kingdom); A. Oscoz, Instituto de Astrofísica de Canarias (Spain) and Univ. de La Laguna (Spain)

9147 7W Stable Imaging for Astronomy (SIA) [9147-295] M. Beaulieu, S. Ottogalli, O. Preis, Y. Bresson, J.-P. Rivet, L. Abe, F. Vakili, Univ. de Nice

Sophia-Antipolis, Observatoire de la Côte d’Azur, CNRS (France) 9147 7X Adapting a very high resolution echelle spectrograph to an 8 meter class telescope [9147-297] R. O. Reynolds, L. Dettmann, Large Binocular Telescope Observatory (United States) 9147 7Y Development of compact and ultra-high-resolution spectrograph with multi-GHz optical

frequency comb [9147-298] M. Endo, The Univ. of Tokyo (Japan) and Exploratory Research for Advanced Technology

(Japan); T. Sukegawa, Canon Inc. (Japan); A. Silva, Y. Kobayashi, The Univ. of Tokyo (Japan) and Exploratory Research for Advanced Technology (Japan)

9147 7Z The habitable-zone planet finder calibration system [9147-299] S. Halverson, S. Mahadevan, L. Ramsey, R. Terrien, A. Roy, C. Schwab, C. Bender, F. Hearty,

E. Levi, The Pennsylvania State Univ. (United States); S. Osterman, Johns Hopkins Univ. Applied Physics Lab. (United States); G. Ycas, S. Diddams, National Institute of Standards and Technology (United States)

9147 80 A stable and inexpensive wavelength reference for precise wavelength calibration of

radial velocity spectrographs [9147-300] T. Feger, Macquarie Univ. (Australia); M. J. Ireland, The Australian National Univ. (Australia);

J. Bento, C. Bacigalupo, Macquarie Univ. (Australia) 9147 81 Performance modeling of an upgraded NIRSPEC on Keck [9147-301] E. C. Martin, M. P. Fitzgerald, I. S. McLean, Univ. of California, Los Angeles (United States); S. M. Adkins, W. M. Keck Observatory (United States); T. Aliado, G. Brims, C. Johnson, K. Magnone, E. Wang, J. Weiss, Univ. of California, Los Angeles (United States) 9147 82 Optical cavity characterization of the Tor Vergata Fabry-Pérot interferometer [9147-304] L. Giovannelli, F. Berrilli, D. Del Moro, Univ. degli Studi di Roma "Tor Vergata" (Italy); V. Greco, Istituto Nazionale di Ottica Applicata - CNR (Italy); R. Piazzesi, Univ. degli Studi di

Roma "Tor Vergata" (Italy); A. Sordini, Istituto Nazionale di Ottica Applicata - CNR (Italy); M. Stangalini, INAF - Osservatorio Astronomico di Roma (Italy) 9147 83 Gemini planet imager observational calibrations VII: on-sky polarimetric performance of

the Gemini planet imager [9147-305] S. J. Wiktorowicz, Univ. of California, Santa Cruz (United States); M. Millar-Blanchaer Univ. of

Toronto (Canada); M. D. Perrin, Space Telescope Science Institute (United States);

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J. R. Graham, Univ. of California, Berkeley (United States); M. P. Fitzgerald, Univ. of California, Los Angeles (United States); J. Maire, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada); P. Ingraham, Kavli Institute for Particle Astrophysics and Cosmology, Stanford Univ. (United States) and Univ. de Montréal (Canada);

D. Savransky, Cornell Univ. (United States); B. A. Macintosh, Lawrence Livermore National Lab. (United States) and Stanford Univ. (United States); S. J. Thomas, NASA Ames Research Ctr. (United States); J. K. Chilcote, Univ. of California, Los Angeles (United States);

Z. H. Draper, Univ. of Victoria (Canada); I. Song, Univ. of Georgia (United States); A. Cardwell, Gemini Observatory (Chile); S. J. Goodsell, Gemini Observatory (United

States); M. Hartung, P. Hibon, F. Rantakyrö, N. Sadakuni, Gemini Observatory (Chile) 9147 84 Gemini planet imager observational calibrations V: astrometry and distortion [9147-306] Q. M. Konopacky, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto

(Canada); S. J. Thomas, NASA Ames Research Ctr. (United States); B. A. Macintosh, Stanford Univ. (United States) and Lawrence Livermore National Lab. (United States); D. Dillon, Univ. of California Observatories (United States); N. Sadakuni, Univ. of California Observatories (United States) and Gemini Observatory (Chile); J. Maire, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada); M. Fitzgerald, Univ. of California, Los Angeles (United States); S. Hinkley, California Institute of Technology (United States); P. Kalas, Univ. of California, Berkeley (United States); T. Esposito, Univ. of California, Los Angeles (United States); C. Marois, NRC - Dominion Astrophysical Observatory (Canada);

P. J. Ingraham, Stanford Univ. (United States); F. Marchis, SETI Institute (United States); M. D. Perrin, Space Telescope Science Institute (United States); J. R. Graham, J. J. Wang,

Univ. of California, Berkeley (United States); R. J. De Rosa, Arizona State Univ. (United States) and Univ. of Exeter (United Kingdom); K. Morzinski, Steward Observatory, The Univ. of Arizona (United States); L. Pueyo, Space Telescope Science Institute (United States);

J. K. Chilcote, J. E. Larkin, Univ. of California, Los Angeles (United States); D. Fabrycky, The Univ. of Chicago (United States); S. J. Goodsell, Gemini Observatory (Chile);

B. R. Oppenheimer, American Museum of Natural History (United States); J. Patience, Arizona State Univ. (United States); L. Saddlemyer, NRC - Dominion Astrophysical Observatory (Canada); A. Sivaramakrishnan, Space Telescope Science Institute

(United States) 9147 85 Gemini planet imager observational calibrations VI: photometric and spectroscopic

calibration for the integral field spectrograph [9147-307] J. Maire, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada); P. J. Ingraham, Kavli Institute for Particle Astrophysics and Cosmology, Stanford Univ.

(United States); R. J. De Rosa, Arizona State Univ. (United States) and Univ. of Exeter (United Kingdom); M. D. Perrin, Space Telescope Science Institute (United States); A. Rajan, Arizona State Univ. (United States); D. Savransky, Cornell Univ. (United States); J. J. Wang, Univ. of California, Berkeley (United States); J.-B. Ruffio, SETI Institute (United States); S. G. Wolff, Johns Hopkins Univ. (Canada); J. K. Chilcote, Univ. of California, Los Angeles (United States); R. Doyon, Univ. de Montréal (Canada); J. R. Graham, Univ. of California, Berkeley (United States); A. Z. Greenbaum, Johns Hopkins Univ. (United States); Q. M. Konopacky, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada); J. E. Larkin, Univ. of California, Los Angeles (United States); B. A. Macintosh, Kavli Institute for Particle Astrophysics and Cosmology, Stanford Univ. (United States) and Lawrence Livermore National Lab. (United States); C. Marois, NRC - Herzberg Institute of Astrophysics (Canada); M. Millar-Blanchaer, Univ. of Toronto (Canada); J. Patience, Arizona State Univ. (United States); L. A. Pueyo, A. Sivaramakrishnan, Space Telescope Science Institute (United States); S. J. Thomas, NASA Ames Research Ctr. (United States); J. L. Weiss, Univ. of California, Los Angeles (United States)

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9147 86 A robotic, compact, and extremely high resolution optical spectrograph for a close-in super-Earth survey [9147-308]

J. Ge, S. Powell, B. Zhao, F. Varosi, B. Ma, S. Sithajan, J. Liu, R. Li, N. Grieves, S. Schofield, L. Avner, H. Jakeman, W. A. Yoder, J. A. Gittelmacher, M. A. Singer, Univ. of Florida (United

States); M. Muterspaugh, M. Williamson, J. E. Maxwell, Tennessee State Univ. (United States) 9147 87 Characterizing instrumental effects on polarization at a Nasmyth focus using NaCo [9147-309] J. de Boer, European Southern Observatory (Chile) and Leiden Observatory, Leiden Univ.

(Netherlands); J. H. Girard, D. Mawet, European Southern Observatory (Chile); F. Snik, C. U. Keller, Leiden Observatory, Leiden Univ. (Netherlands); J. Milli, European Southern

Observatory (Chile) and IPAG, Univ. Joseph Fourier, CNRS (France) Part Five 9147 88 The upgrade of a high dispersion spectro-polarimeter, VESPolA: new circular polarimetry

mode and extremely high resolution mode [9147-310] T. Arasaki, Kyoto Sangyo Univ. (Japan); Y. Ikeda, Photocoding (Japan); N. Akika, H. Kawakita, Kyoto Sangyo Univ. (Japan) 9147 89 FIDEOS: a high resolution echelle spectrograph for the ESO 1m telescope at La Silla [9147-311] M. Tala, A. Berdja, M. Jones, L. Vanzi, S. Ropert, Pontificia Univ. Católica de Chile (Chile); M. Flores, Univ. de Santiago de Chile (Mexico); C. Viscasillas, Univ. Católica de Avila

(Spain) 9147 8C HARPS-N @ TNG, two year harvesting data: performances and results [9147-314] R. Cosentino, INAF - Telescopio Nazionale Galileo (Spain); C. Lovis, F. Pepe, Observatoire

Astronomique de l'Univ. de Genève (Switzerland); A. C. Cameron, Univ. of St. Andrews (United Kingdom); D. W. Latham, Harvard-Smithsonian Ctr. for Astrophysics (United States); E. Molinari, INAF - Telescopio Nazionale Galileo (Spain); S. Udry, Observatoire Astronomique de l'Univ. de Genève (Switzerland); N. Bezawada, UK Astronomy Technology Ctr. (United Kingdom); N. Buchschacher, Observatoire Astronomique de l'Univ. de Genève (Switzerland); P. Figueira, Natural History Museum of Denmark (Denmark); M. Fleury, Observatoire Astronomique de l'Univ. de Genève (Switzerland); A. Ghedina, INAF - Telescopio Nazionale Galileo (Spain); A. G. Glenday, Harvard-Smithsonian Ctr. for Astrophysics (United States); M. Gonzalez, J. Guerra, INAF - Telescopio Nazionale Galileo (Spain); D. Henry, UK Astronomy Technology Ctr. (United Kingdom); I. Hughes, C. Maire,

F. Motalebi, Observatoire Astronomique de l'Univ. de Genève (Switzerland); D. Phillips, Harvard-Smithsonian Ctr. for Astrophysics (United States)

9147 8D Development of infrared echelle spectrograph and mid-infrared heterodyne spectrometer

on a small telescope at Haleakala, Hawaii for planetary observation [9147-315] T. Sakanoi, Y. Kasaba, M. Kagitani, H. Nakagawa, Tohoku Univ. (Japan); J. Kuhn, S. Okano,

Institute for Astronomy, Univ. of Hawai'i (United States) 9147 8E ERIS: the exoplanet high-resolution image simulator for CHARIS [9147-316] M. A. Limbach, T. D. Groff, N. J. Kasdin, Princeton Univ. (United States); T. Brandt, Institute for

Advanced Studies (United States); K. Mede, The Univ. of Tokyo (Japan); C. Loomis, Princeton Univ. (United States); M. Hayashi, N. Takato, National Astronomical Observatory of Japan (Japan)

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9147 8F The solar system at 10 parsec: exploiting the ExAO of LBT in the visual wavelengths [9147-317] M. Stangalini, F. Pedichini, M. Centrone, INAF - Osservatorio Astronomico di Roma (Italy); S. Esposito, INAF - Osservatorio Astrofisico di Arcetri (Italy); J. Farinato, INAF - Osservatorio

Astronomico di Padova (Italy); E. Giallongo, INAF - Osservatorio Astronomico di Roma (Italy); F. Quirós-Pacheco, E. Pinna, INAF - Osservatorio Astrofisico di Arcetri (Italy)

9147 8H SPRAT: Spectrograph for the Rapid Acquisition of Transients [9147-319] A. S. Piascik, I. A. Steele, S. D. Bates, C. J. Mottram, R. J. Smith, R. M. Barnsley, B. Bolton,

Liverpool John Moores Univ. (United Kingdom) 9147 8I DIPOL-2: a double image high precision polarimeter [9147-321] V. Piirola, A. Berdyugin, Univ. of Turku (Finland); S. Berdyugina, Kiepenheuer-Institut für

Sonnenphysik (Germany) 9147 8J H.O.R.S. a new visiting instrument for G.T.C. based on the Utrecht Echelle Spectrograph

[9147-322] J. Peñate, F. Gracia, C. Allende, J. Calvo, S. Santana, Instituto de Astrofísica de Canarias

(Spain) 9147 8K ESPRESSO front end exposure meter: a chromatic approach to radial velocity correction

[9147-323] M. Landoni, M. Riva, INAF - Osservatorio Astronomico di Brera (Italy); F. Pepe, Observatoire

de Genève (Switzerland); P. Conconi, F. M. Zerbi, INAF - Osservatorio Astronomico di Brera (Italy); A. Cabral, Univ. de Lisboa (Portugal); S. Cristiani, INAF - Osservatorio Astronomico di Trieste (Italy); D. Megevand, Observatoire de Genève (Switzerland)

9147 8L First calibration and visible wavelength observations of Khayyam: a tunable spatial

heterodyne spectroscopy (SHS) [9147-324] S. Hosseini, Univ. of California, Davis (United States); W. Harris, The Univ. of Arizona (United States) 9147 8M The metrology system for the multi-object optical and near-infrared spectrograph MOONS

[9147-325] M. Torres-Torriti, L. Vanzi, R. Dünner, F. Belmar, L. Dauvin, T.-C. Chen, Pontificia Univ. Católica

de Chile (Chile); M. Cirasuolo, W. Taylor, H. Schnetler, D. Montgomery, P. Rees, UK Astronomy Technology Ctr. (United Kingdom); A. Cabral, Univ. de Lisboa (Portugal)

9147 8N Green astro-comb for HARPS-N [9147-326] N. Langellier, Harvard Univ. (United States); C.-H. Li, A. G. Glenday, Harvard-Smithsonian

Ctr. for Astrophysics (United States); G. Chang, Massachusetts Institute of Technology (United States) and Hamburg Univ. (Germany); H.-W. Chen, J. Lim, Massachusetts Institute of Technology (United States); G. Furesz, Harvard-Smithsonian Ctr. for Astrophysics (United States); F. Kärtner, Massachusetts Institute of Technology (United States) and Hamburg Univ. (Germany); D. F. Phillips, Harvard-Smithsonian Ctr. for Astrophysics (United States);

D. Sasselov, Harvard Univ. (United States) and Harvard-Smithsonian Ctr. for Astrophysics (United States); A. Szentgyorgyi, Harvard-Smithsonian Ctr. for Astrophysics (United States);

R. Walsworth, Harvard Univ. (United States) and Harvard-Smithsonian Ctr. for Astrophysics (United States)

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9147 8O A coronagraph based on two spatial light modulators for active amplitude apodizing and phase corrections [9147-328]

J. Dou, Nanjing Institute of Astronomical Optics and Technology (China); D. Ren, Nanjing Institute of Astronomical Optics and Technology (China) and California State Univ., Northridge (United States); X. Zhang, Y. Zhu, G. Zhao, Z. Wu, R. Chen, Nanjing Institute of Astronomical Optics and Technology (China); C. Liu, F. Yang, C. Yang, Nanjing Institute of Astronomical Optics and Technology (China) and Univ. of Chinese Academy of Sciences (China)

9147 8P Novel infrared polarimeter for the ESO CRIRES+ instrument [9147-329] M. Lockhart, N. Piskunov, E. Stempels, Uppsala Univ. (Sweden); M. Escuti, North Carolina

State Univ. (United States); E. Oliva, INAF - Osservatorio Astrofisico di Arcetri (Italy); H.-U. Käufl, European Southern Observatory (Germany); U. Heiter, T. Marquart, Uppsala

Univ. (Sweden); G. Anglada-Escude, Georg-August-Univ. Göttingen (Germany); D. Baade, P. Bristow, R. J. Dorn, European Southern Observatory (Germany); R. Follert, Thüringer Landessternwarte Tautenburg (Germany); D. Gojak, J. H. Grunhut, European Southern Observatory (Germany); A. Hatzes, Thüringer Landessternwarte Tautenburg (Germany);

M. Hilker, D. Ives, Y. Jung, F. Kerber, B. Klein, J.-L. Lizon, European Southern Observatory (Germany); T. Löwinger, Thüringer Landessternwarte Tautenburg (Germany); L. Origlia, INAF - Osservatorio Astrofisico di Arcetri (Italy); L. Pasquini, J. Paufique, E. Pozna, European Southern Observatory (Germany); A. Reiners, U. Seemann, Georg-August-Univ. (Germany); A. Smette, J. Smoker, E. Valenti, European Southern Observatory (Germany)

9147 8Q ESPRESSO Coudé-Train: complexities of a simultaneous optical feeding from the four VLT

unit telescopes [9147-330] A. Cabral, M. Abreu, J. Coelho, R. Gomes, Ctr. de Astronomia e Astrofísica da Univ. de

Lisboa (Portugal); M. Monteiro, Ctr. de Astrofísica da Univ. do Porto (Portugal); A. Oliveira, P. Santos, Univ. de Lisboa (Portugal); G. Ávila, B.-A. Delabre, European Southern Observatory (Germany); M. Riva, INAF - Osservatorio Astronomico di Brera (Italy);

P. Di Marcantonio, I. Coretti, INAF - Osservatorio Astronomico di Trieste (Italy); N. C. Santos, Univ. de Lisboa (Portugal) and Univ. do Porto (Portugal); F. Zerbi, INAF - Osservatorio Astronomico di Brera (Italy); D. Mégevand, Observatoire de l’Univ. de Genève (Switzerland)

9147 8R Fast multichannel astronomical photometer based on silicon photo multipliers mounted at the Telescopio Nazionale Galileo [9147-371]

F. Ambrosino, F. Meddi, C. Rossi, S. Sclavi, Univ. degli Studi di Roma La Sapienza (Italy); R. Nesci, INAF - Istituto di Astrofisica e Planetologia Spaziali (Italy); I. Bruni, INAF -

Osservatorio Astronomico di Bologna (Italy); A. Ghedina, L. Riverol, L. Di Fabrizio, INAF - Fundación Galileo Galilei (Spain)

9147 8S Photometric study of the Paranal observatory using MASS database [9147-373] A. Abahamid, Univ. Cadi Ayyad (Morocco); M. Sarazin, European Southern Observatory

(Germany); G. Lombardi, European Southern Observatory (Chile) 9147 8T First performance of the GeMS+GMOS system [9147-65] P. Hibon, Gemini South Observatory (Chile); B. Neichel, Lab. d'Astrophysique de Marseille

(France); V. Garrel, Gemini South Observatory (Chile); B. Prout, F. Rigaut, The Australian National Univ. (Australia); A. Koning, Univ. of Victoria (Canada); G. Sivo, G. Gimeno, R. Carrasco, C. Winge, P. Pessev, A. Serio, G. Arriagada, Gemini South Observatory (Chile)

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POSTER SESSION: EXTREMELY LARGE TELESCOPES AND INSTRUMENTS

9147 8U Design and analysis of a large-diameter precision optical mount for NFIRAOS [9147-303] J. Fitzsimmons, A. Hill, National Research Council Canada (Canada) 9147 8V HARMONI instrument control electronics [9147-331] J. V. Gigante, L. F. Rodríguez, Instituto de Astrofísica de Canarias (Spain); G. Zins, Institut de

Planétologie et d’Astrophysique de Grenoble (France); H. Schnetler, UK Astronomy Technology Ctr. (United Kingdom); A. Pecontal, Ctr. de Recherche Astrophysique de Lyon (France); J. M. Herreros, Instituto de Astrofísica de Canarias (Spain); F. Clarke, Univ. of Oxford (United Kingdom); I. Bryson, UK Astronomy Technology Ctr. (United Kingdom); N. Thatte, Univ. of Oxford (United Kingdom)

9147 8W A novel systems engineering approach to the design of a precision radial velocity

spectrograph: the GMT-Consortium Large Earth Finder (G-CLEF) [9147-333] W. Podgorski, Harvard-Smithsonian Ctr. for Astrophysics (United States); J. Bean, The Univ. of

Chicago (United States); H. Bergner, Harvard-Smithsonian Ctr. for Astrophysics (United States); M.-Y. Chun, Korea Astronomy and Space Science Institute (Korea, Republic of);

J. Crane, Carnegie Observatories (United States); I. Evans, J. Evans, G. Furesz, Harvard-Smithsonian Ctr. for Astrophysics (United States); D. Guzman, Pontificia Univ. Católica de Chile (Chile); K.-M. Kim, Korea Astronomy and Space Science Institute (Korea, Republic of);

K. McCracken, M. Mueller, T. Norton, Harvard-Smithsonian Ctr. for Astrophysics (United States); C. Park, Korea Astronomy and Space Science Institute (Korea, Republic of); S. Park, D. Plummer, A. Szentgyorgyi, Harvard-Smithsonian Ctr. for Astrophysics (United States);

A. Uomoto, Carnegie Observatories (United States); I.-S. Yuk, Korea Astronomy and Space Science Institute (Korea, Republic of)

9147 8X The infrared imaging spectrograph (IRIS) for TMT: volume phase holographic grating

performance testing and discussion [9147-334] S. Chen, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada);

E. Meyer, S. A. Wright, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada) and Univ. of Toronto (Canada); A. M. Moore, Caltech Optical Observatories (United States); J. E. Larkin, Univ. of California, Los Angeles (United States); J. Maire, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada); E. Mieda, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada) and Univ. of Toronto (Canada); L. Simard, NRC - Dominion Astrophysical Observatory (Canada)

9147 8Y Development of a subwavelength grating vortex coronagraph of topological charge 4

(SGVC4) [9147-335] C. Delacroix, O. Absil, B. Carlomagno, P. Piron, Univ. de Liège (Belgium); P. Forsberg, M. Karlsson, Uppsala Univ. (Sweden); D. Mawet, European Southern Observatory (Chile); S. Habraken, J. Surdej, Univ. de Liège (Belgium) 9147 8Z Integral field spectroscopy of high redshift galaxies with the HARMONI spectrograph on the

European Extremely Large Telescope [9147-336] S. Kendrew, S. Zieleniewski, N. Thatte, J. Devriendt, R. Houghton, Univ. of Oxford (United

Kingdom); T. Fusco, ONERA (France); M. Tecza, F. Clarke, K. O'Brien, Univ. of Oxford (United Kingdom)

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9147 90 Trade-off study for high resolution spectroscopy in the near infrared with ELT telescopes: seeing-limited vs. diffraction limited instruments [9147-337]

N. Sanna, E. Oliva, F. Massi, G. Cresci, INAF - Osservatorio Astrofisico di Arcetri (Italy); L. Origlia, INAF - Osservatorio Astronomico di Bologna (Italy) 9147 91 Simulations of high-z galaxy observations with an ELT-MOS [9147-338] K. Disseau, M. Puech, H. Flores, F. Hammer, Y. Yang, GEPI, Observatoire de Paris, CNRS,

Univ. Paris Diderot (France); L. Pentericci, INAF - Osservatorio Astronomico di Roma (Italy) 9147 92 All-sky homogeneity of precipitable water vapour over Paranal [9147-339] R. R. Querel, National Institute of Water and Atmospheric Research (New Zealand) and

Univ. de Chile (Chile); F. Kerber, European Southern Observatory (Germany) 9147 93 Simulating observations with HARMONI: the integral field spectrograph for the European

Extremely Large Telescope [9147-340] S. Zieleniewski, N. Thatte, S. Kendrew, R. Houghton, M. Tecza, F. Clarke, Univ. of Oxford

(United Kingdom); T. Fusco, ONERA (France); M. Swinbank, Durham Univ. (United Kingdom) 9147 94 The MANIFEST fibre positioning system for the Giant Magellan Telescope [9147-341] J. S. Lawrence, D. M. Brown, J. Brzeski, S. Case, Australian Astronomical Observatory

(Australia); M. Colless, The Australian National Univ. (Australia); T. Farrell, L. Gers, J. Gilbert, M. Goodwin, Australian Astronomical Observatory (Australia); G. Jacoby, Giant Magellan Telescope (United States) and Carnegie Observatories (United States); A. M. Hopkins,

M. Ireland, K. Kuehn, N. P. F. Lorente, S. Miziarski, R. Muller, V. Nichani, A. Rakman, Australian Astronomical Observatory (Australia); S. Richards, The Univ. of Sydney (Australia);

W. Saunders, N. F. Staszak, J. Tims, M. Vuong, L. Waller, Australian Astronomical Observatory (Australia)

9147 95 A mechanical design concept for EAGLE on the revised E-ELT [9147-342] C. M. Dubbeldam, Durham Univ. (United Kingdom) 9147 96 Science case and requirements for the MOSAIC concept for a multi-object spectrograph

for the European Extremely Large Telescope [9147-343] C. J. Evans, UK Astronomy Technology Ctr. (United Kingdom); M. Puech, GEPI, Observatoire

de Paris, CNRS, Univ. Paris Diderot (France); B. Barbuy, Univ. de São Paulo (Brazil); P. Bonifacio, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); J.-G. Cuby, Aix

Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); E. Guenther, Thüringer Landessternwarte Tautenburg (Germany); F. Hammer, P. Jagourel, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); L. Kaper, Univ. van Amsterdam (Netherlands);

S. L. Morris, Durham Univ. (United Kingdom); J. Afonso, Observatório Astronómico de Lisboa (Portugal); P. Amram, Aix Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); H. Aussel, CEA, AIM, Service d'Astrophysique (France); A. Basden, Durham Univ. (United Kingdom); N. Bastian, Liverpool John Moores Univ. (United Kingdom); G. Battaglia, Instituto de Astrofísica de Canarias (Spain); B. Biller, The Royal Observatory, Edinburgh (United Kingdom); N. Bouché, Univ. de Toulouse, UPS-OMP, CNRS (France); E. Caffau, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); S. Charlot, UPMC-CNRS, Institut d’Astrophysique de Paris (France); Y. Clenet, LESIA, Observatoire de Paris, CNRS-UPMC, Univ. Paris-Diderot (France); F. Combes, LERMA, Observatoire de Paris, CNRS (France); C. Conselice, The Univ. of Nottingham (United Kingdom); T. Contini, Univ. de Toulouse, UPS-OMP, CNRS (France); G. Dalton, Univ. of Oxford (United Kingdom) and Rutherford Appleton Lab. (United Kingdom); B. Davies, Liverpool John Moores Univ. (United States); K. Disseau, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); J. Dunlop, The

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Royal Observatory, Edinburgh (United Kingdom); F. Fiore, INAF - Osservatorio Astronomico di Roma (Italy); H. Flores, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); T. Fusco, ONERA (France); D. Gadotti, European Southern Observatory (Chile); A. Gallazzi, INAF - Osservatorio Astrofisico di Arcetri (Italy); E. Giallongo, INAF - Osservatorio Astronomico di Roma (Italy); T. Gonçalves, Observatório do Valongo (Brazil); D. Gratadour, LESIA, Observatoire de Paris, CNRS-UPMC, Univ. Paris-Diderot (France); V. Hill, Observatoire de la Côte d’Azur (France); M. Huertas-Company, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); R. Ibata, Observatoire de Strasbourg (France); S. Larsen, Radboud Univ. Nijmegen (Netherlands); O. Le Fèvre, Aix Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); B. Lemasle, Univ. von Amsterdam (Netherlands); C. Maraston, Univ. of Portsmouth (United Kingdom); S. Mei, GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot (France); Y. Mellier, UPMC-CNRS, Institut d’Astrophysique de Paris (France); G. Östlin, Stockholm Univ. (Sweden); T. Paumard, LESIA, Observatoire de Paris, CNRS-UPMC, Univ. Paris-Diderot (France); R. Pello, Univ. de Toulouse, UPS-OMP, CNRS (France); L. Pentericci, INAF - Osservatorio Astronomico di Roma (Italy); P. Petitjean, UPMC-CNRS, Institut d’Astrophysique de Paris (France); M. Roth, Leibniz-Institut für Astrophysik Potsdam (Germany); D. Rouan, LESIA, Observatoire de Paris, CNRS-UPMC, Univ. Paris-Diderot (France); D. Schaerer, Observatoire de Genève, Univ. de Genève (Switzerland); E. Telles, Observatorio Nacional (Brazil); S. Trager, Univ. of Groningen (Netherlands); N. Welikala, Univ. of Oxford (United Kingdom); S. Zibetti, INAF - Osservatorio Astrofisico di Arcetri (Italy); B. Ziegler, Univ. Wien (Austria)

9147 97 The spectrograph units for the HARMONI integral field spectrograph [9147-344] K. O'Brien, J. R. Allen, J. D. Lynn, N. A. Thatte, Univ. of Oxford (United Kingdom); I. Bryson, UK

Astronomy Technology Ctr. (United Kingdom); F. Clarke, Univ. of Oxford (United Kingdom); H. Schnetler, UK Astronomy Technology Ctr. (United Kingdom); M. Tecza, Univ. of Oxford (United Kingdom)

9147 99 Mid-IR AGPMs for ELT applications [9147-346] B. Carlomagno, C. Delacroix, O. Absil, Univ. de Liège (Belgium); P. Forsberg, Uppsala Univ.

(Sweden); S. Habraken, A. Jolivet, Univ. de Liège (Belgium); M. Karlsson, Uppsala Univ. (Sweden); D. Mawet, European Southern Observatory (Chile); P. Piron, J. Surdej, Univ. de Liège (Belgium); E. Vargas Catalan, Uppsala Univ. (Sweden)

9147 9A The opto-mechanical design of the GMT-consortium large earth finder (G-CLEF) [9147-347] M. Mueller, D. Baldwin, Harvard-Smithsonian Ctr. for Astrophysics (United States); J. Bean,

The Univ. of Chicago (United States); H. Bergner, Harvard-Smithsonian Ctr. for Astrophysics (United States); B. Bigelow, GMTO Corp. (United States); M.-Y. Chun, Korea Astronomy and Space Science Institute (Korea, Republic of); J. Crane, Carnegie Observatories (United States); J. Foster, G. Fűrész, T. Gauron, Harvard-Smithsonian Ctr. for Astrophysics (United States); D. Guzman, Pontificia Univ. Católica de Chile (Chile); E. Hertz, Harvard-Smithsonian Ctr. for Astrophysics (United States); A. Jordán, Pontificia Univ. Católica de Chile (Chile);

K.-M. Kim, Korea Astronomy and Space Science Institute (Korea, Republic of); K. McCracken, T. Norton, M. Ordway, Harvard-Smithsonian Ctr. for Astrophysics (United

States); C. Park, Korea Astronomy and Space Science Institute (Korea, Republic of); S. Park, W. Podgorski, A. Szentgyorgyi, Harvard-Smithsonian Ctr. for Astrophysics (United States); A. Uomoto, Carnegie Observatories (United States); I.-S. Yuk, Korea Astronomy and Space

Science Institute (Korea, Republic of)

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9147 9B SKA pulsar search: technological challenges and best algorithms development [9147-348] C. Baffa, INAF - Osservatorio Astrofisico di Arcetri (Italy) 9147 9C The infrared imaging spectrograph (IRIS) for TMT: reflective ruled diffraction grating

performance testing and discussion [9147-349] E. Meyer, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada) and

Univ. of Toronto (Canada); S. Chen, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada); S. A. Wright, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada) and Univ. of Toronto (Cambodia); A. M. Moore, Caltech Optical Observatories (United States); J. E. Larkin, Univ. of California, Los Angeles (United States);

L. Simard, NRC – Dominion Astrophysical Observatory (Canada); J. Maire, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada); E. Mieda, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada) and Univ. of Toronto (Canada);

J. Gordon, Univ. of Toronto (Canada) 9147 9D Three possible types of coronagraphs for the E-ELT PCS instrument [9147-350] A. Carlotti, IPAG, CNRS (France); M. N'Diaye, L. Pueyo, Space Telescope Science Institute

(United States); D. Mawet, European Southern Observatory (Chile) 9147 9E The high contrast imaging modes of MICADO [9147-351] P. Baudoz, A. Boccaletti, S. Lacour, R. Galicher, Y. Clénet, D. Gratadour, É. Gendron, T. Buey, G. Rousset, Lab. d'Etudes Spatiales et d'Instrumentation en Astrophysique,

Observatoire de Paris-Meudon (France); M. Hartl, R. Davies, Max-Planck-Institut für extraterrestrische Physik (Germany)

9147 9F An aperture masking mode for the MICADO instrument [9147-352] S. Lacour, P. Baudoz, E. Gendron, A. Boccaletti, R. Galicher, Y. Clénet, D. Gratadour, T. Buey, G. Rousset, LESIA, Observatoire de Paris (France); M. Hartl, R. Davies, Max-Planck-

Institut für extraterrestrische Physik (Germany) 9147 9G The G-CLEF spectrograph optical design [9147-353] G. Fűrész, Harvard-Smithsonian Ctr. for Astrophysics (United States); H. Epps, Univ. of

California Observatories, Lick Observatory (United States) and Univ. of California Santa Cruz (United States); S. Barnes, Stuart Barnes Optical Design (Netherlands); W. Podgorski,

A. Szentgyorgyi, M. Mueller, D. Baldwin, Harvard-Smithsonian Ctr. for Astrophysics (United States); J. Bean, The Univ. of Chicago (United States); H. Bergner, Harvard-Smithsonian Ctr. for Astrophysics (United States); M.-Y. Chun, Korea Astronomy and Space Science Institute (Korea, Republic of); J. Crane, Carnegie Observatories (United States); J. Evans, I. Evans,

J. Foster, T. Gauron, Harvard-Smithsonian Ctr. for Astrophysics (United States); D. Guzman, Pontificia Univ. Católica de Chile (Chile); E. Hertz, Harvard-Smithsonian Ctr. for Astrophysics (United States); A. Jordán, Pontificia Univ. Catolica de Chile (Chile); K.-M. Kim, Korea Astronomy and Space Science Institute (Korea, Republic of); K. McCracken, T. Norton,

M. Ordway, Harvard-Smithsonian Ctr. for Astrophysics (United States); C. Park, Korea Astronomy and Space Science Institute (Korea, Republic of); S. Park, D. Plummer, Harvard-Smithsonian Ctr. for Astrophysics (United States); A. Uomoto, Carnegie Observatories (United States); I.-S. Yuk, Korea Astronomy and Space Science Institute (Korea, Republic of)

9147 9H On-instrument wavefront sensor design for the TMT infrared imaging spectrograph (IRIS)

update [9147-354] J. Dunn, V. Reshetov, J. Atwood, J. Pazder, B. Wooff, D. Loop, L. Saddlemyer, NRC -

Herzberg Institute of Astrophysics (Canada); A. M. Moore, Caltech Optical Observatories (United States); J. E. Larkin, Univ. of California, Los Angeles (United States)

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9147 9I DKIST visible broadband imager interference filters [9147-355] F. Wöger, National Solar Observatory (United States) 9147 9J Optical and mechanical design of the fore-optics of HARMONI [9147-356] J. Sánchez-Capuchino, E. Hernández, A. Bueno, J. M. Herreros, Instituto de Astrofísica de

Canarias (Spain); N. Thatte, Univ. of Oxford (United Kingdom); I. Bryson, UK Astronomy Technology Ctr. (United Kingdom); F. Clarke, M. Tecza, Univ. of Oxford (United Kingdom)

9147 9K Beating the heat! Automated characterization of piezoelectric tubes for Starbugs

[9147-357] R. Piersiak, Stony Brook Univ. (United States); M. Goodwin, J. Gilbert, R. Muller, Australian

Astronomical Observatory (Australia) 9147 9L Wireless software update system based on Zigbee for LAMOST [9147-358] S. Li, Y. Gu, Y. Jin, C. Zhai, Univ. of Science and Technology of China (China) 9147 9M Cryogenic testing of components for the HARMONI spectrograph [9147-359] J. R. Allen, K. O'Brien, J. D. Lynn, N. A. Thatte, Univ. of Oxford (United Kingdom); I. Bryson, UK

Astronomy Technology Ctr. (United Kingdom); F. Clarke, Univ. of Oxford (United Kingdom); H. Schnetler, UK Astronomy Technology Ctr. (United Kingdom); M. Tecza, Univ. of Oxford (United Kingdom)

9147 9N The fiber-fed preslit of GIANO at T.N.G. [9147-360] A. Tozzi, E. Oliva, INAF - Osservatorio Astrofisico di Arcetri (Italy); L. Origlia, INAF -

Osservatorio Astronomico di Bologna (Italy); C. Baffa, V. Biliotti, G. Falcini, E. Giani, M. Iuzzolino, F. Massi, N. Sanna, INAF - Osservatorio Astrofisico di Arcetri (Italy); S. Scuderi,

INAF - Osservatorio Astrofisico di Catania (Italy); M. Sozzi, INAF - Osservatorio Astrofisico di Arcetri (Italy)

9147 9O Simultaneous phase and amplitude retrieval with COFFEE: from theory to laboratory results

[9147-363] B. Paul, ONERA (France), Lab. d'Astrophysique de Marseille, Univ. Aix-Marseille, CNRS

(France), and PHASE, Observatoire de Paris, CNRS, Univ. Diderot (France); J.-F. Sauvage, L. M. Mugnier, ONERA (France) and PHASE, Observatoire de Paris, CNRS, Univ. Diderot

(France); K. Dohlen, Lab. d'Astrophysique de Marseille, Univ. Aix-Marseille, CNRS (France) and PHASE, Observatoire de Paris, CNRS, Univ. Diderot (France); T. Fusco, ONERA (France), Lab. d'Astrophysique de Marseille, Univ. Aix-Marseille, CNRS (France), and PHASE, Observatoire de Paris, CNRS, Univ. Diderot (France); M. Ferrari, Lab. d'Astrophysique de Marseille, Univ. Aix-Marseille, CNRS (France) and PHASE, Observatoire de Paris, CNRS, Univ. Diderot (France)

9147 9P Infrared differential imager and spectrograph for SPHERE: performance assessment for on-

sky operation [9147-365] M. Langlois, Ctr. de Recherche Astronomique de Lyon, Observatoire de Lyon, CNRS, Univ.

de Lyon 1 (France) and Ecole Normale Supérieure de Lyon (France); A. Vigan, K. Dohlen, C. Moutou, Aix-Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France);

J.-L. Beuzit, Institut de Planétologie et d’Astrophysique de Grenoble (France); A. Boccaletti, LESIA, Observatoire de Paris (France); M. Carle, A. Costille, Aix-Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); R. Dorn, European Southern Observatory (Germany); L. Gluck, Institut de Planétologie et d’Astrophysique de Grenoble (France);

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C. Gry, Aix-Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); N. Hubin, European Southern Observatory (Germany); M. Feldt, Max-Planck-Institut für Astronomie (Germany); M. Kasper, European Southern Observatory (Germany); F. Madec,

D. Le Mignant, Aix-Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); J.-L. Lizon, European Southern Observatory (Germany); D. Mouillet, Institut de Planétologie

et d’Astrophysique de Grenoble (France); A. Origné, Aix-Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France); P. Puget, Institut de Planétologie et d’Astrophysique de Grenoble (France); J.-F. Sauvage, ONERA (France); F. Wildi, Observatoire Astronomique de l’Univ. de Genève (Switzerland); A. Zurlo, Aix-Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France)

9147 9Q Fully cryogenic phased array prototype camera for the Arecibo radio telescope [9147-366] G. Cortes-Medellin, A. Vishwas, S. C. Parshley, D. B. Campbell, Cornell Univ. (United States) 9147 9R LOTUCE2: a dome-seeing instrument for the E-ELT [9147-367] A. Berdja, D. Guzman, N. Saez, N. David, N. Dubost, Pontificia Univ. Católica de Chile

(Chile); M. Sarazin, European Southern Observatory (Germany); A. Ziad, Lab. J.L. Lagrange, Univ. Nice Sophia-Antipolis, CNRS, OCA (France)

9147 9S The infrared imaging spectrograph (IRIS) for TMT: overview of innovative science programs

[9147-369] S. A. Wright, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada)

and Univ. of Toronto (Canada); J. E. Larkin, Univ. of California, Los Angeles (United States); A. M. Moore, Caltech Optical Observatories (United States); T. Do, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto (Canada); L. Simard, NRC - Herzberg Institute of Astrophysics (Canada); M. Adamkovics, Univ. of California, Berkeley (United States);

L. Armus, California Institute of Technology (United States); A. J. Barth, E. Barton, Univ. of California, Irvine (United States); H. Boyce, Dunlap Institute for Astronomy and Astrophysics, Univ. of Toronto, (Canada) and Univ. of Saskatchewan (Canada); J. Cooke, Swinburne Univ. of Technology (Australia); P. Cote, T. Davidge, NRC - Herzberg Institute of Astrophysics (Canada); B. Ellerbroek, Thirty Meter Telescope Observatory Corp. (United States);

A. Ghez, Univ. of California, Los Angeles (United States); M. C. Liu, J. R. Lu, Institute for Astronomy, Univ. of Hawai'i (United States); B. A. Macintosh, Standford Univ. (United States); S. Mao, National Astronomical Observatories (China); C. Marois, NRC - Herzberg Institute of Astrophysics (Canada); M. Schoeck, Thirty Meter Telescope Observatory Corp. (United States); R. Suzuki, National Astronomical Observatory of Japan (Japan); J. C. Tan, Univ. of Florida (United States); T. Treu, Univ. of California, Santa Barbara (United States); L. Wang, Thirty Meter Telescope Observatory Corp. (United States); J. Weiss, Univ. of California, Los Angeles (United States)

9147 9T Drift scanning technique for mid-infrared background subtraction [9147-372] S. Heikamp, B. R. Brandl, C. U. Keller, Leiden Observatory (Netherlands); L. Venema,

ASTRON (Netherlands); E. Pantin, CEA-Ctr. de SACLAY (France); R. Siebenmorgen, D. Ives, F. Kerber, European Southern Observatory (Germany)

Author Index

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Conference Committee Symposium Chairs

Gillian S. Wright, UK Astronomy Technology Centre (United Kingdom) Luc Simard, National Research Council Canada (Canada)

Symposium Co-chairs

Colin Cunningham UK Astronomy Technology Centre (United Kingdom)

Masanori Iye National Astronomical Observatory of Japan (Japan)

Conference Chairs

Suzanne K. Ramsay, European Southern Observatory (Germany) Ian S. McLean, University of California, Los Angeles (United States) Hideki Takami, Subaru Telescope, National Astronomical Observatory of Japan (United States)

Conference Program Committee

Julia J. Bryant, The University of Sydney (Australia) Stephen S. Eikenberry, University of Florida (United States) Chris J. Evans, UK Astronomy Technology Centre (United Kingdom) Ramón J. García López, Instituto de Astrofísica de Canarias (Spain) Maureen L. Savage, SOFIA / USRA (United States) Luc Simard, National Research Council Canada (Canada) Oskar von der Lühe, Kiepenheuer-Institut für Sonnenphysik (Germany)

Session Chairs

1 Instrument Programs at Major Observatories Hideki Takami, Subaru Telescope, National Astronomical Observatory of Japan (United States)

2 New Instruments and Upgrades to Existing Instruments

Oskar von der Lühe, Kiepenheuer-Institut für Sonnenphysik (Germany)

3 High Multiplex and Survey Instruments I Stephen S. Eikenberry, University of Florida (United States)

4 High Multiplex and Survey Instruments II

Ian S. McLean, University of California, Los Angeles (United States)

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5 High Multiplex and Survey Instruments III Julia J. Bryant, The University of Sydney (Australia)

6 High Spectral Resolution Instruments I

Suzanne K. Ramsay, European Southern Observatory (Germany)

7 High Spectral Resolution Instruments II Ramón J. García López, Instituto de Astrofísica de Canarias (Spain)

8 High Spatial Resolution Instruments I

Hideki Takami, Subaru Telescope, National Astronomical Observatory of Japan (United States)

9 High Spatial Resolution Instruments II

Maureen L. Savage, SOFIA / USRA (United States)

10 Instruments for Extremely Large Telescopes Luc Simard, National Research Council Canada (Canada)

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Introduction This conference, the fifth in the series on Ground-based and Airborne Instrumentation for Astronomy, attracted a very rich programme of papers discussing all aspects of the design and delivery of complete instrument systems. The range of innovation in the instrument building community was particularly remarkable at this meeting. Instrument concepts matched to the ~1000m2 collecting area of the extremely large telescopes were discussed alongside highly scientifically focused instruments for telescopes with ~1m2 apertures. Meanwhile, the current large telescope observatories are considering their instrument suites in the light of future new developments. Survey instruments are becoming an enduring and significant theme at our meeting, whether designed for observing hundreds of galaxies, or hundreds of points on a radial velocity curve to reveal exo-planetary systems. At this meeting, ~350 papers were presented, either as oral or poster contributions. Six invited reviews were requested on major existing facilities or planned new ones. The presentations were arranged into 10 sessions over the five days of the meeting. The major topics were:

• Instrument Programmes at Major Observatories • New instruments and Upgrades to Existing Instruments • High Multiplex and Survey Instruments • High Spectral Resolution Instruments • High Spatial Resolution Instruments • Instruments for Extremely Large Telescopes

On behalf of the program committee, it is a pleasure to acknowledge the contribution of all participants in making this a busy and very productive meeting.

Suzanne K. Ramsay Hideki Takami Ian S. McLean

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Proc. of SPIE Vol. 9147 914701-66


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