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.|
|Trouble Shooting||Technical Pages||Index|
|Trouble Shooting pages and links.||Portal to the technical pages: for the initiated only!||A listing of the instrument pages.|
NIRES (Near-Infrared Echellette Spectrometer) is a prism cross dispersed near-infrared spectrograph to be mounted on the Keck 2 telescope at right bent Cassegrain port. It has a separate slit-viewing channel to enable real-time source identification and guiding in the near-infrared (K'). In addition, an optical camera (FOV 1.8' x 1.8') is available for offset guiding. NIRES is very similar to TripleSpec at APO 3.5m, Palomar 5m, and ARCoIRIS at CTIO . In addition, NIRES is fitted with a Flexure Control System (FCS) to minimize the effects of flexure. Led by PIs Keith Matthews and Tom Soifer, NIRES is developed at Caltech. Commissioning is planned to start in 2017B. A general overview of this family of instruments is described in Wilson et al. 2004, SPIE, 5492, 1295.
NIRES optical layout.
NIRES installed at the RBC port.