IRCS

Information for S19B applicants

Observations of IRCS-AO in S19B

There are important announcements of LGS-AO mode, infrared secondary mirror re-coating, and telescope downtime in S19B CfP. Please carefully read the CfP Important Notice.

Polarimetry mode (Shared-risk)

IRCS provides several linear polarimetry modes in 0.95−4.16 μm as 'Shared-Risk' mode. Users who want to propose polarimetry observation SHOULD contact Dr. Tamura (motohide.tamura_at_nao.ac.jp; the PI of the waveplate unit). Please contact to Tae-Soo Pyo (pyo_at_naoj.org) and Hiroshi Terada(terada_at_naoj.org) for more detailed information and performance limitations in advance before the submission of their proposals. Please see "Polarimetry" section for more detailed information about polarimetry mode.

Introduction

The Infrared Camera and Spectrograph (IRCS) is installed at the Infrared Nasmyth focus of Subaru Telescope and incorporates two 10242 ALADDIN III arrays which are sensitive from 0.9−5.6 μm. IRCS is designed to deliver diffraction limited images from 2 μm and up, as well as providing spectroscopy with grisms and a cross-dispersed echelle. The camera can also be used as a slit viewer for the echelle spectroscopy.

IRCS is always operated with Adaptive Optics (AO188) attached regarldess of using adaptive optics, and relies on AO188 for guiding without a separate autoguider.

Imaging

The imaging mode of IRCS provides two plate scales, of 20 and 52 mas per pixel, producing fields of view of 21'' and 54'', respectively. The camera is equipped with a range of broad and narrow-band filters in its three filter wheels.

Grism spectroscopy

The camera section of IRCS provides a number of grisms which provide a low resolution (R = 100-2000) spectroscopic capability. Slit widths of 0.1-0.9'' are available.

Echelle spectroscopy

IRCS has a cross-dispersed echelle spectrograph, providing spectral resolution up to 20 000. The IRCS echelle provides a pixel scale of 55 mas along the slit and slit widths of 0.14'', 0.27'' (providing half the spectral resolution), or 0.54'' (providing one-quarter the spectral resolution). The camera-side detector is used as a slit viewer.

Note: We provide an NH3 gas absorption cell function for a high-precision radial velocity measurement at the 30 m s-1 level even with the spectral resolving power of IRCS. The NH3 gas cell can be used in a part of K-band with IRCS + AO188 mode. Please contact to IRCS + AO188 support astronomer for further information. The IR gas cell was provided by Andreas Seifahrt (University of Chicago) in collaboration with colleagues at the university of Goettingen (Germany) and Lund Observatory (Sweden).

Polarimetry

IRCS provides several linear polarimetry modes in 0.95−4.16 μm as 'Shared-Risk' mode. Imaging polarimetry is available for Y-, J-, H-, K(K')-, and L'-bands. Spectropolarimetry is available with zJH-, HK-, K-, and L-grisms in 52 mas mode only. Please be advised that circular polarimetry is not available. Users should contact to Dr. Tamura (motohide.tamura_at_nao.ac.jp), Tae-Soo Pyo (pyo_at_naoj.org), and Hiroshi Terada (terada_at_naoj.org) for more detailed information if they have any plan of the polarimetry mode observation.

Observation Preparation

Citations

When referring to IRCS in a paper, please use the following citation. The papers can be downloaded from links below.

Further information

Please note that all numbers on these pages are subject to change as the performance of IRCS is better determined. Questions regarding IRCS should be directed to Yuhei Takagi (takagi__at__naoj.org).

March 18 2019




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