PalSpec Status Review WITH NOTES RE KECK APPLICATION

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PalSpec Status Review WITH NOTES RE KECK APPLICATION. Terry Herter, Chuck Henderson (Cornell) John Wilson, Mike Skrutskie (Univ. or Virginia) Keith Matthews (Caltech), Jim Howard (Telic) March 21, 2003. Spectrograph Requirements. Original Baseline Simultaneous coverage from 0.80 – 2.5 m m - PowerPoint PPT Presentation

Transcript of PalSpec Status Review WITH NOTES RE KECK APPLICATION

  • PalSpec Status Review

    WITH NOTES RE KECK APPLICATIONTerry Herter, Chuck Henderson (Cornell)John Wilson, Mike Skrutskie (Univ. or Virginia)Keith Matthews (Caltech), Jim Howard (Telic)

    March 21, 2003

    PalSpec Status Review

  • Spectrograph RequirementsOriginal BaselineSimultaneous coverage from 0.80 2.5 mmEmphasis on J, H, and K bandsR ~ 2500 with 30 x 0.9 arcsec slitFor keck R~2500 with slit ~ 15 x 0.45 arcsecSlit viewer with > 2x2 arcmin2 FoVKeck slit viewer ~ 40x40DeliveryDecember 2003For Keck, delivery TBD

    PalSpec Status Review

  • WHY DOES IT WORK ON KECKInstrument is being designed to study faint, small (palomar instrument will work at keck with fov reduced by factor of 2

    PalSpec Status Review

  • OH Line PositionsPositions of atmosphere airglow (OH) lines vs. wavelength overlaid with atmospheric transmission.

    PalSpec Status Review

  • Perspective ViewsCollimatorReimagerGratingSlit viewerFocal Plane

    PalSpec Status Review

  • Perspective Views

    PalSpec Status Review

  • View with Shell

    PalSpec Status Review

  • Prototype Spectrograph CameraPrototype Camera by Jim Howard, Telic Optics

    PalSpec Status Review

  • Camera Spot Diagrams

    PalSpec Status Review

  • Encircled Energy

    PalSpec Status Review

  • Spectrum Layout in Focal PlanePossible array rotation (also rotate slit to keep on columns)

    PalSpec Status Review

  • Spectral ResolutionSpectral resolution for 1.0 arcsec slit with 2.78 pixels/arcsecond.

    PalSpec Status Review

  • Grating Efficiency

    PalSpec Status Review

  • System Throughput* includes primary through detectorAtmospheric transmissionOff the array

    PalSpec Status Review

    Chart1

    0.15834679810.17231139090.10000149530.09761621420.07286072590.05700028230.350.35

    0.30265195670.25658978320.22816493880.19086983020.12296865460.041644127800

    0.06502316640.09142993860.05578069380.08014679850.03880870290.0055082862

    Order 3

    Order 4

    Order 5

    Order 6

    Order 7

    Order 8

    Microns

    Throughput

    Estimated Instrument Throughput

    throughput totals

    Palomar SpectrographTransmission Calculations

    pisco2arotate3bent.zmx

    Wavelength (microns)

    Order = 3Order = 4Order = 5Order = 6Order = 7Order = 8

    2.402.181.871.871.641.461.461.311.191.191.091.011.010.940.870.870.820.77

    estimated

    throughput

    from worksheet 20.160.300.070.170.260.090.100.230.060.100.190.080.070.120.040.060.040.01

    Wavelength (microns)

    2.42.181.871.641.461.311.191.091.010.940.870.820.77

    throughput after0.160.300.240.260.190.230.150.190.150.120.100.040.01

    summing contributions

    from adjacent orders

    1.891.89

    0.350

    1.851.85

    0.350

    throughput totals

    00000000

    00000000

    000000

    Order 3

    Order 4

    Order 5

    Order 6

    Order 7

    Order 8

    Microns

    Throughput

    Estimated Instrument Throughput

    pisco2arotate3bent.zmx

    Palomar Spectrograph

    Transmission Calculations

    pisco2arotate3bent.zmx

    Wavelength (microns)

    Order = 3Order = 4Order = 5Order = 6Order = 7Order = 8

    Source2.402.181.871.871.641.461.461.311.191.191.091.011.010.940.870.870.820.77

    Element

    Primary10.930.920.920.920.910.910.910.900.890.890.880.870.870.860.850.850.840.83

    f/16 Secondary10.930.920.920.920.910.910.910.900.890.890.880.890.890.890.880.880.880.87

    Dewar Window

    surf 1 reflectance20.990.990.990.990.990.990.990.990.990.990.990.990.990.970.950.950.920.90

    bulk transmission1.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.00

    surf 2 reflectance20.990.990.990.990.990.990.990.990.990.990.990.990.990.970.950.950.920.90

    Reimager OAP 1

    surf reflectance30.980.980.980.980.980.980.980.980.980.980.980.980.980.980.980.980.980.98

    Reimager OAP 2

    surf reflectance30.980.980.980.980.980.980.980.980.980.980.980.980.980.980.980.980.980.98

    Collimator

    surf reflectance30.980.980.980.980.980.980.980.980.980.980.980.980.980.980.980.980.980.98

    Prism 1 ZnSe

    surf 1 reflectance40.970.990.990.990.990.990.990.990.990.990.990.990.990.990.990.990.970.96

    bulk transmission1.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.00

    surf 2 reflectance40.970.990.990.990.990.990.990.990.990.990.990.990.990.990.990.990.970.96

    Prism 2 ZnSe

    surf 1 reflectance40.970.990.990.990.990.990.990.990.990.990.990.990.990.990.990.990.970.96

    bulk transmission1.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.00

    surf 2 reflectance40.970.990.990.990.990.990.990.990.990.990.990.990.990.990.990.990.970.96

    Prism 3 Infrasil

    surf 1 reflectance50.960.980.990.990.990.980.980.990.990.990.990.980.980.980.980.980.980.85

    bulk transmission1.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.00

    surf 2 reflectance50.960.980.990.990.990.980.980.990.990.990.990.980.980.980.980.980.980.85

    Fold Mirror

    surf reflectance30.980.980.980.980.980.980.980.980.980.980.980.980.980.980.980.980.980.98

    Grating

    surf reflectance30.980.980.980.980.980.980.980.980.980.980.980.980.980.980.980.980.980.98

    measured efficiency rel alum70.550.950.200.530.880.320.350.800.200.350.770.330.300.710.320.470.630.21

    charge for non-littrow (AD=30)80.950.950.950.950.950.950.950.950.950.950.950.950.950.950.950.950.950.95

    Camera Lens 1

    surf 1 reflectance20.990.990.990.990.990.990.990.990.990.990.990.990.990.970.950.950.920.90

    bulk transmission1.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.00

    surf 2 reflectance20.990.990.990.990.990.990.990.990.990.990.990.990.990.970.950.950.920.90

    Camera Lens 2

    surf 1 reflectance20.990.990.990.990.990.990.990.990.990.990.990.990.990.970.950.950.920.90

    bulk transmission1.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.00

    surf 2 reflectance20.990.990.990.990.990.990.990.990.990.990.990.990.990.970.950.950.920.90

    Camera Lens 3

    surf 1 reflectance20.990.990.990.990.990.990.990.990.990.990.990.990.990.970.950.950.920.90

    bulk transmission1.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.00

    surf 2 reflectance20.990.990.990.990.990.990.990.990.990.990.990.990.990.970.950.950.920.90

    Camera Lens 4

    surf 1 reflectance20.990.990.990.990.990.990.990.990.990.990.990.990.990.970.950.950.920.90

    bulk transmission1.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.00

    surf 2 reflectance20.990.990.990.990.990.990.990.990.990.990.990.990.990.970.950.950.920.90

    Camera Lens 5

    surf 1 reflectance20.990.990.990.990.990.990.990.990.990.990.990.990.990.970.950.950.920.90

    bulk transmission1.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.00

    surf 2 reflectance20.990.990.990.990.990.990.990.990.990.990.990.990.990.970.950.950.920.90

    Camera Lens 6

    surf 1 reflectance20.990.990.990.990.990.990.990.990.990.990.990.990.990.970.950.950.920.90

    bulk transmission1.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.00

    surf 2 reflectance20.990.990.990.990.990.990.990.990.990.990.990.990.990.970.950.950.920.90

    Camera Lens 7

    surf 1 reflectance20.990.990.990.990.990.990.990.990.990.990.990.990.990.970.950.950.920.90

    bulk transmission1.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.001.00

    surf 2 reflectance20.990.990.990.990.990.990.990.990.990.990.990.990.990.970.950.950.920.90

    Detector

    sapphire substrate90.930.930.930.930.930.930.930.930.930.930.930.930.930.930.930.930.930.93

    quantum efficiency100.600.600.600.600.550.550.550.550.550.550.500.500.500.500.500.500.500.40

    Throughput0.160.300.070.170.260.090.100.230.060.100.190.080.070.120.040.060.040.01

    Notes:

    1. Hal Petrie e-mail dtd 19 Mar 03

    2. Estimate 0.99 from 1-2.4 microns, and assume reflectance falls to 0.90 by 0.8 microns

    3. Estimate coated silver delivers 0.98 across all wavelengths

    4. Thin Film Lab estimate dtd 15 Mar 03 for 28 deg AOI on ZnSe

    5. Thin Film Lab estimate dtd 15 Mar 03 for 36 deg AOI on Infrasil

    6. Estimate from RGL Catalogue

    7. Based on measured littrow reflectances for master grating for orders 4, 6, 7, 8 by RGL, and extrapolation for non-littrow use and missing order mesurements

    8. Guess based on Loewen, Neviere & Maystre, Applied Optics, October 1977, p.2711, Fig 8

    9. Sapphire from calculating (n-1)^2/(n+1)^2, assume uncoated

    10. Estimate from Hawaii-I data found at http://www.mpia-hd.mpg.de/homes/calj/omega2000/newsletter/text.html

    P200 reflectivity

    P200 Reflectivity

    Data from H. Petrie e-mail dtd 19 Mar 03

    primary (current estimate)secondary (new coating)secondary (w/ 3 years aging)

    0.70.810.90.87

    10.870.920.89

    1.50.910.950.92

    2.50.930.960.93

    P200 reflectivity

    0

    0

    0

    0

    Microns

    Reflectance (current estimate)

    Primary Reflectance

    0

    0

    0

    0

    Microns

    Reflectance (current estimate)

    f/16 Secondary Reflectance

  • Slit ViewerDesign SpecsOperates at KsImages to ~ 0.14 arcsec/pixGiving 2.4 arcmin FoV => 5.7 sq. arcmin

    IntegrationTime (sec)Ks mag (S/N = 5)Number of GalaxiesNumber of Stars117.2311018.41513019.0271

    PalSpec Status Review

  • KECK SLIT VIEWERWELL USE 256X256 ARRAY FROM EXISTING IR INSTRUMENTFOV EQUIVALENT TO NIRC FOV (40)

    PalSpec Status Review

  • Slit Viewer Detection RateSlit viewer with 2.4 arcmin FoVCounts from Glazebrook et al. 1994, MNRAS, 266, 65.

    PalSpec Status Review

  • Spectrograph Line SensitivityAssumptionsS/N = 5, 10 pixels to extract lineSystem throughput = 0.15 in all bandsBetween OH-lines (J,H,K bkgnd = 70, 200, 70 mJy/arcsec2)RN = 5 e-, i(dark) = 0.01 e-/secKECK SHOULD BE 4x BETTERtback = integration time for RN to contribute < 20% to noise.

    Flux (10-17 ergs/cm2/s)tbackBand600 sec1800 sec3600 sec(sec)J2.11.10.75410H2.21.20.87170K3.01.71.257

    PalSpec Status Review

  • Spectrograph Continuum SensitivityAssumptionsS/N = 5 per resolution elementSystem throughput = 0.15 in all bandsBetween OH-lines (J,H,K bkgnd = 70, 200, 70 mJy/arcsec2)RN = 5 e-, i(dark) = 0.01 e-/secKECK WILL BE 1.5 MAG DEEPER FOR POINT SOURCES

    Mag in 1 resolution elementBand600 sec1800 sec3600 secJ19.720.420.8H18.819.519.8K17.718.318.7

    PalSpec Status Review

  • PalSpec Status Review

  • PalSpec Status Review