The Update for S15A Applicants
Due to the MOIRCS Upgrade Project (replacing detectors to H2RG), MOIRCS will be unavailable from around May 2015 untill early S15B. The start date of the actual closure will be announced in late 2014. We are sorry for any inconvenience.
All observations after the upgrade will be executed under shared-risk policy.
R1300 Grism Issue → Updated 2013-08-13.
Recently it is recognized that the R1300 grism shows slight image degradation. The symptom has been already there at least since early 2013. Degradation seems to have a position-dependence (at least for channel-2). As the advance speed is apparently slow, we don't close the grism for now. The investigation has just started and the result will be uploaded to the dedicated website. The use of the R1300 grism will be under shared-risk policy.
For MOS Applicants
When you apply to the MOS observation, you must explicitly specify the required number of MOS masks (both for the Full and the Minimum Number of Nights) in the Sect 11 of the application form. And also, please justify why you need the requested number in the technical detail part in Sect 14. The number of MOS mask will be fixed once it is assigned by TAC's critical reviewing. The request for any backup mask is basically not permitted, unless there are any special reasons.
Please note that the maximum number of MOS mask available for one contiguous observing period is 15.
ANNOUNCEMENT on "nuMOIRCS" Project
We will have two instrument closure periods for "nuMOIRCS" Project during 2015-2016.
The detectors are to be changed to Hawaii2-RG. All electronics related to the detector readout will also be replaced (to SIDECAR ASIC + SAM System). The benefit is the significant reduction of the readout noise as well as the overhead for detector readout. Current plan is to execute the engineering work around May to July 2015. Some nights in August 2015 will then be used for the evaluation of the new system. Thus MOIRCS will be unavailable during next May to early S15B.
We are also planning to introduce the IFU spectroscopy function to MOIRCS, as well as the upgrade of the current MOS system and the control computers. The date of the downtime is still TBD, though it might happen in late 2015 to early 2016. We will update the schedule soon via this website.
MOIRCS (Multi-Object InfraRed Camera and Spectrograph) provides wide-field imaging and long-slit / multi-object (MOS) spectroscopic capabilities in the 0.9 ~ 2.5 µm spectral range under the natural seeing condition. The 4'×7' field of view is covered by two Hawaii-2 2048×2048 arrays with the spatial resolution of 0.117 arcsec/pixel.
For the imaging mode, the standard MKO YJHKs filters as well as some narrow-band filters are available. See the Imaging Mode Page for more details.
The MOS performance of MOIRCS spectroscopy mode is the most notable feature of the instrument. Using the cooled aluminium slit masks, MOIRCS can acquire about 40 object spectra simultaneously across 0.9~2.5 micron wavelength range. Currently low-resolution (R~500), medium-resolution (R~1300), and high-resolution (R~3000) modes are available. See the Spectroscopy Page for more details. All MOS observers/applicants should carefully read the MOS observation pages.
Instrument and Detector
Please cite the following papers when you refer MOIRCS in your publication.
- "Multi-Object Infrared Camera and Spectrograph (MOIRCS) for the Subaru Telescope I. Imaging"
- Suzuki, R. et al. Publications of the Astronomical Society of Japan, 2008, Vol.60, No.6, pp.1347--1362.
- "MOIRCS: Multi-Object Infrared Camera and Spectrograph for SUBARU"
- Ichikawa, T. et al. 2006, in Proc. of SPIE, Vol. 6269, 38
Note that any data on the pages are subject to change.
Dr. Ichi Tanaka (MOIRCS Support Astronomer: email )