SYNOPSES OF MOUNT HAMILTON FACILITY INSTRUMENTS: SPECTROGRAPHS
NOTES | BACK |
INSTRUMENT | TELESCOPE |
| DETECTOR | ||||||||||||||||||||||||||||||||||||||||||||
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HAMILTON ECHELLE SPECTROGRAPH A prism cross-dispersed, high-resolution instrument. Steve Vogt, UCSC |
Shane 3-m coude and Coude Auxiliary Telescope (CAT) |
| dewar #6,
2048 x 2048 thinned CCD, 15-u pixels | ||||||||||||||||||||||||||||||||||||||||||||
KAST DOUBLE SPECTROGRAPH A simultaneous red/blue, two-channel instrument, with limited imaging capability. Joe Miller, UCSC |
Shane 3-m cassegrain |
A polarimeter is available for use in both channels. | red channel: Kast Red dewar, 4096 x 1024 Hamamatsu CCD, 15-u pixels blue channel: | ||||||||||||||||||||||||||||||||||||||||||||
LEVY ESCHELLE SPECTORGRAPH An eschelle spectrometer with fixed grating and cross-disperser for improved stabiity. Steve Vogt, UCSC |
Automated Planet Finder (APF) |
| E2V CCD42-90,
2048 x 2048, 13.5-u pixels | ||||||||||||||||||||||||||||||||||||||||||||
ShARCS /
Shane Adaptive Optics The Shane AO system and ShARCS camera is primarily a direct imaging instrument, but offers low resolution spectrograph capability. |
Shane 3-m cassegrain |
See ShARCS manual | |||||||||||||||||||||||||||||||||||||||||||||
NICKEL SPECTROGRAPH
Instrument has been decomissioned, but retaining information here for
archival data reference. Richard Stover, UCSC (Decommissioned) |
Nickel 1-m cassegrain |
| dewar #9, 400 x 1200 thinned CCD, 27-u pixels | ||||||||||||||||||||||||||||||||||||||||||||
GEMINI THE UCLA TWIN-ARRAYS INFRARED CAMERA A simultaneous two-channel instrument with direct imaging capabilites. GEMINI is no longer available for use, but information retained here for archival purposes. Ian McLean, UCLA (Decommissioned) |
Shane 3-m cassegrain |
|
short wave channel: 256 x 256 NICMOS3 HgCdTe array, 40-u pixels
long wave channel: |
NOTES |
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DISPERSER: given as rulings per mm / 1st order blaze wavelength DISPERSION: Angstroms/pixel for the given detector RANGE: the useful wavelength range COVERAGE: the maximum wavelength coverage for a single exposure RESOLUTION: lambda/delta lambda at blaze wavelength; narrow slit |
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