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COMICS FITS informationData structureOdd numbers are assigned to imaging data (for imaging observations or slit-viewer images for spectroscopy), while even numbers are reserved for the spectrograph (i.e., they contain no data and only the FITS headers for imaging observations and spectra for spectroscopy). COMA FITS files: raw dataCOMICS FITS files are 4-dimensional: X × Y × Z × W
COMA files consist of a series of A1,B1,A2,B2,A3,B3,...i.e., (co-added) images taken at each chop position (in each beam) in turn. In one of the examples provided below (COMA00102607.fits), there are 11 images each taken at each chop position (beamA or beamB) and so there are 22 images in total. At mid-infrared wavelengths, sky is usually much brighter than an object and each of these images will probably not show anything. That is why we employ the chopping technique and what we should now do is subtract the beamB image from each preceding beamA frame. i.e., (A1-B1), (A2-B2), (A3-B3), etc. COMA files are provided for more thorough/rigorous data reduction/analysis. Sample FITS files
Sample FITS headers
COMQ FITS files: quick-look dataCOMQ files contain the results of a quick background subtraction, i.e., (A1-B1) + (A2-B2) + (A3-B3) + ... This is what is displayed on the quick-look viewer at the summit during observations. Sample FITS files
Note that the third dimension of each of the above FITS files is now 1. Sample FITS headers
COMICS specific FITS header keyword dictionaryCopyright © 2000-2019 Subaru Telescope, NAOJ. All rights reserved. |