PalSpec Status Review WITH NOTES RE KECK APPLICATION
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Transcript of PalSpec Status Review WITH NOTES RE KECK APPLICATION
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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
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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
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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
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OH Line PositionsPositions of atmosphere airglow (OH) lines vs. wavelength overlaid with atmospheric transmission.
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Perspective ViewsCollimatorReimagerGratingSlit viewerFocal Plane
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Perspective Views
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View with Shell
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Prototype Spectrograph CameraPrototype Camera by Jim Howard, Telic Optics
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Camera Spot Diagrams
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Encircled Energy
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Spectrum Layout in Focal PlanePossible array rotation (also rotate slit to keep on columns)
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Spectral ResolutionSpectral resolution for 1.0 arcsec slit with 2.78 pixels/arcsecond.
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Grating Efficiency
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System Throughput* includes primary through detectorAtmospheric transmissionOff the array
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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
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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
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KECK SLIT VIEWERWELL USE 256X256 ARRAY FROM EXISTING IR INSTRUMENTFOV EQUIVALENT TO NIRC FOV (40)
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Slit Viewer Detection RateSlit viewer with 2.4 arcmin FoVCounts from Glazebrook et al. 1994, MNRAS, 266, 65.
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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
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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
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PalSpec Status Review
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PalSpec Status Review