In this case, sky lines in Object.fits would be used instead. Data output: Object_wc.fits (wavelength-calibrated Object files) ...

An example of spectral format using the cross-dispersing grating for the blue region. ORDER WAVEMIN WAVECEN WAVEMAX FSR LD CDMIN CDCEN CDMAX ORDSEP (nm) (nm) (nm) (nm) (nm/mm) (mm) (mm) (mm) (mm) 199 ...

Calibration Data Up: Observing Previous: Data Acquisition Contents Observation Procedure Observation procedure is a file that describes the sequence of observations using abstract commands explained ...

The HDS data unit includes the output of one CCD with 2048 (slit direction) by 4100 (dispersion direction) pixels (in the case without binning) and the over-scan region. Over-scan indicates the ...

Four types of data for calibration are usually obtained. These are the bias level, the dark level, flat fielding, and wavelength calibration exposures. The abstract commands used to obtain calibration ...

The setting of the cross disperser determines the spectral orders observed. One cross disperser for the blue or red region is selected for higher efficiency in the wavelength region of interest. The ...

国立天文台ハワイ観測所・光赤外研究部・天文データセンターは共催で 「すばる春の学校2008」を開催致します。 開催日時 2008年5月7日（水）～ 5月9日（金）16:00 開催場所 国立天文台・三鷹 ...

This document describes Subaru FITS rules.

the PDF edition of the PI Document has now been incorporated into the HTML version. free short (30-s) exposures have now been eliminated (the ob tab no longer contains calib_tgtcfg and calib_inscfg ...

The Call for Proposals for Semester S00 saw 114 submitted proposals, requesting a total of 223 nights. The available 36 nights were awarded to the following 26 proposals: ...

The Call for Proposals for Semester S10A received 139 and 2 submitted proposals for the Normal and Intensive Programs, respectively, requesting a total of 412.1 nights. After screening by TAC, 79 + 4 ...