Background

This document describes the procedure for measuring the gain and readnoise of the DEIMOS science mosaic detectors. It is to be run by a WMKO Support Astronomer.

Prerequisites

• 1200G grating loaded.
• Z filter loaded.
• Instrument interface running as dmoseng.

Procedure

1. Acquire images. Execute script

   	~dmoseng/scripts/gain_check

   to acquire 3 biases and 5 flats.
2. Analyze images. Launch IDL v6.2, navigate to data directory, and run the following commands:
   1. start HQ xterm
   2. in an HQ xterm run

       start.idl62 

   3. in the IDL session run

       cdata 

   to take you to the current data dir.
   4. next run the following two cmds to take the necessary data.

       deimos_mosaic_gain_check, /direct
       deimos_mosaic_gain_check, /spectral

      This creates logfiles in the directory ~dmoseng/data/gain.
3. Update web page.
   1. login to HQ xterm as deimos
   2. change to the DEIMOS web directory,

       cd /home/www/public/realpublic/inst/deimos/ 

   3. execute the command

       gmake gain

      to regenerate the web page describing gain and readnoise.

   Description

   Acquisition

   We configure DEIMOS for a mode that provides near-uniform illumination across the entire detector plane by acquiring internal slitless flats in spectral mode. This turns out to be challenging to accomplish, because even high-resolution spectral flats with the internal quartz lamp saturate. I found that one mode which succeeds in providing generally uniform illumination is to insert the Z filter, thus blocking most of the light, and select a central wavelength of 5000 Å, which is well below the cutoff of the filter. For some reason (possibly internal scattered light) this produces relatively uniform illumination across the middle of the detector plane; at the edges there is an excess of light.

   Analysis

   We employ the "Janesick method" (employed in the IRAF findgain task) for measuring gain and readnoise simultaneously from a set of biases and flats. In this case we consider only the half of each detector which is closest to the middle of the focal plane in order to avoid the regions of nonuniform illumination near the corners. On each amplifier, we derive the gain and readnoise within numerous independent 256×256 pixel regions and compute the median value across the array to derive the adopted gain and readnoise for that amplifier. For each region, we determine which pair of the 5 flats has the closest match in terms of illumination level, and we use that pair of images to derive gain and readnoise for that region. A bootstrap analysis of the array of gain and readnoise values for individual regions provides the quoted uncertainties on each quantity.

   See Also

   • DEIMOS Detector Gain and Readnoise Values

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   Last modified: Wed Jan 21 10:04:53 HST