Instrument Scientist:
Deputy Instrument Scientist:
Email Contact:
Pre-Observing | Observing | Post-Observing |
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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. |
Troubleshooting
AO Troubleshooting |
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 |