AMICA A ntarctic M ultiband I nfrared CA mera

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Telescope and Instrument Robotization at Dome C Puerto Santiago, Tenerife, March 26-29, 2007. AMICA A ntarctic M ultiband I nfrared CA mera. Favio Bortoletto INAF – Osservatorio Astronomico di Padova on behalf of the AMICA collaboration. AMICA People. - PowerPoint PPT Presentation

Transcript of AMICA A ntarctic M ultiband I nfrared CA mera

  • AMICAAntarctic Multiband Infrared CAmeraFavio Bortoletto INAF Osservatorio Astronomico di Padovaon behalf of the AMICA collaboration

  • AMICA PeopleL. Corcione, F. PorcuF.M. Zerbi, A. Riva, V. De Caprio, E. Molinari, P. ConconiF. Bortoletto, C. Bonoli, M. DAlessandro, E. Giro, D. Fantinel, D. MagrinO. Straniero (PI), M. Dolci (PM), G. Valentini, C. Giuliani, A. Di Cianno, G. Di Rico, M. Ragni, D. Pelusi, A. Valentini

  • The Camera in Summary Near- and mid-infrared photometry (2 5.5 m and 7 28 m) Two independent channels Remotely operated To be mounted at the f / 21.65 IRAIT Nasmyth focus Standard broadband plus narrow band filter set

  • AMICA Optical Layout: Medium IR ChannelSi:As BIB 128x128 array @ 8KScale Reduction : 12.18 to 17.86 /mm

  • AMICA Optical Layout: Near IR ChannelTMInSb 256x256 array @ 35 KScale Reduction : 12.18 to 17.86 /mm

  • Detectors: 7 28 m 2 5.5 mSi:As BIB MF-128 by DRS Technologies, Inc.Field Coverage: 2.86 arcmin Scale: 1.34/pix128 128 format75 m pitchTop 4 10 KQE @ 8 K > 60 %Well capacity = 9.1106 e-RON @ 255 Hz frame rate = 282 e- r.m.s.d.c. @ 8 K = 3.5 e- / sec / pixelMaximum frame rate: 500 Hz 256 256 format30 m pitchTop 25 35 KQE @ 35 K > 80 %Well Capacity 2 105 e-RON 50 e- r.m.s. (typical)d.c. @ 35 K < 3 e- / sec /pixel4 outputsInSb array by Raytheon Corp.Field Coverage: 2.29 arcmin Scale: 0.54 /pixel

  • AMICA the Cryostat

  • The AMICA Control System: Sytem supervision is assured by a PLC interfaced to the CPCI host :- vacuum system dual-stage cryocooler instrument temperature monitoring racks temperature monitoring cryogenic step-motors control

    Cable

    C-PCI CRATEHOST PENTIUM CPU

    NIR/MIR DETECTORCONTROLLER

    TEMP-CONTROLLEDAMBIENT

    -10 c / 10 c

    AMICACRYOSTAT

    - 40 c / -80 cexternal temperature

    NIRPRE-AMPCLOCKBOX

    MIRPRE-AMPCLOCKBOX

    4.2 K40 Kcryo-cooler

    CRYO-COOLERCOMPRESSOR

    DUAL-STAGESTEP-MOTORCONTROLLER

    VACUUMPUMP

    VACUUMCOMMANDEDVALVEP-GAUGE

    TEMPERATURE&STEP-MOTORCONTROL

    TEMP-CONTROLLEDAMBIENT

    -10 c / 10 c

    LAKESHORETEMPERATURECONTROLLER & MONITOR

    CONTROLPLC

    PMC DETECTORCONTROL I/F

  • The AMICA Control System: CPCI ComputerThe AMICA detector control electronics is built on a CPCI-Pentium host with a SKYTECH PMC array-control I/F. The PMC array controller drives via a dedicated fiber-link the analog unit providing detector biasing, clocking and video signal processing.Secondary chopper drive and monitoring can be done by the detector controller sequencer or, off line, by a CPCI process.

  • MIR simulation boxNIR simulation boxDetector controllerThe AMICA Control System: Detector Controller1.2 GbaudFiber Link

  • AMICA System Operation :The AMICA detector-controller commanding will be possible from threedifferent sources : Local unit (CPCI Camera Driver, Test)Remote UIF (Test, Commissioning) Build camera commands Build readout waveforms Configure detector tables- Retrieve telemetry- Retrieve data- Quick look check- Archive dataRemote Command Flow

  • Commanding, camera configuration and data exchange is based on files. So the test operator interface can reside with simple files redirection on every networked computer. Command and Data exchange :

    CORE MEMORY

    CONFIG.TABLES

    BUILDWAVEFORMS ANDPARAMETERSTABLES

    CPCI COMPUTER

    TELEMETRY FILE

    TELEMETRY RETRIEVE

    BUILDCOMMANDS

    COMMAND FILE

    RETRIEVEDATA

    IMAGE BUFFER I

    IMAGE BUFFER II

    ETHERNET

    ACCUMULATOR I

    ACCUMULATOR II

    RAM DISC

    USER INTERFACE

  • The remote test Interface with the acquisition software is based on the IDL-atv standard interfaceBoot MIRLoad bias tableLoad clock tableRead TelemetryBootOKBias table.loadedClock table.loadedTelemetry..The AMICA Test Interface :

    0.3

    100

    ON

    10

    0

    Prova

  • Telemetry retrieval :

  • Image data files are stacked in core memory buffers: object and sky for chopper assisted observations.Frames are then summed up following the selected readout mode (single, multiple sampl. Etc.) to build the final image accumulators.Images (buffers and/or accumulators) are retrieved by the remote UIF via Ethernet for quick-look analysis and archiving.Scientific Data Organization:

    Object image stack

    Sky image stack

    Star image accumulator

    Sky image accumulator