MOIRCS




The Update for S19A Applicants

2018-08-06

MOIRCS is in Regular Operation

    MOIRCS will be operated under the "regular" status during S19A Semester.

    However, we note that currently the Subaru telescope cannot offer the Arc lamp function due to the trouble on its circuit. Thus we cannot use it for the wavelength calibration of spectroscopy observation. The fixing plan is still TBD and it may take long time. Note that we can still do the wavelength calibration using the OH night lines. Please contact the SA if you have any concern.

    Please carefully read the following MOIRCS webpages before you design your observing strategy. If you have any question, please contact the primary support astronmer (see the bottom of the page).

For MOS Applicants




Introduction

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 2048×2048 infrared detector arrays with the spatial resolution of 0.116 arcsec/pixel. The detector has been updated to the Hawaii2 RG in late 2015.

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 aluminum slit masks, MOIRCS can acquire 40 ~ 60 object spectra simultaneously across 0.9~2.5 micron wavelength range. The low-resolution (R~500) and high-resolution (R~3000) grisms are available (the R1300 medium-resolution grism is also available but have some issues). See the Spectroscopy Page for more details. All MOS observers/applicants should carefully read the MOS observation pages.

If you are interested in the current status of the nuMOIRCS IFU development, please contact Ichi Tanaka (primary SA: email info can be found below).

Instrument and Detector

Imaging mode

Spectroscopy mode



Instrument Citation

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

For the MOIRCS Upgrade 2015 works, you may refer these papers below.

"The NuMOIRCS Project: Detector Upgrade Overview and Early Commissioning Results"
Walawender, J. et al. 2016, Proc. of SPIE, Vol. 9908, doi: 10.1117/12.2231812
"Detector Upgrade of Subaru's Multi-Object Infrared Camera and Spectrograph (MOIRCS)"
Fabricius, M. et al. 2016, Proc. of SPIE, Vol. 9908, doi: 10.1117/12.2231417


MOIRCS Management Structure

  • Observation Support Astronomers
    • Primary: Dr. Ichi Tanaka (email: )
    • Secondary: Dr. Kentaro Aoki (email: )
  • Primary Instrument Operator / Documentation Responsible
    • Joshua Williams (email: jcwilliams_AT_naoj.org)
  • Data Distribution Resonsible
    • Tom Winegar and Computer Division (email: helpdesk_AT_naoj.org)
  • Instrument Hardware and Software Resonsible
    • Koji Omata on behalf of Instrument Division (email: instdiv_AT_naoj.org)
* Please change _AT_ to @ for email address.

Note that any data on the pages are subject to change.

Contact:
Dr. Ichi Tanaka (MOIRCS Support Astronomer: email )

Updated 2018-08-06


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