Secondary Instrument Master:
|Follow this link for information about pre-observing activities: proposal preparation, mask design and submission, pre-run activities, etc.||Follow this link for information about your observing run: instrument and telescope setups, scripts, software, procedures, etc.||Follow this link for information about your post-observing activities: backups, comment forms, data reduction, etc.|
|Toolbox (DRP)||Technical Pages|
|Trouble Shooting pages and links.||Information on the DRP and rectification metricies.||Portal to the technical pages: for the initiated only!|
OSIRIS is a near-infrared integral field spectrograph designed for the Keck Adaptive Optics System.
The instrument uses a lenslet array to sample a small rectangular patch of the sky at resolutions approaching the diffraction limit of the 10-meter Keck Telescope. OSIRIS will provide moderate spectral resolution (R~3800), and full broadband (z, J, H, and K) spectral coverage at over 1000 spatial locations in the AO-corrected field. The integral field design makes optimal use of new large-format (2048x2048) infrared arrays, and is well matched to the compact nature of AO targets.
|Principal Investigator:||James Larkin (UCLA)||OSIRIS References|
|Co-Principal Investigator:||Alfred Krabbe (UC Berkeley)|
|Project Scientist:||Andreas Quirrenbach (UCSD)|
SPEC lightpath cartoon.
OSIRIS on the K2 Nasmyth Deck