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Timestamp:
Mar 6, 2008, 10:47:50 AM (18 years ago)
Author:
Paul Price
Message:

Adding multi-darks --- fitting dark current with multi-dimensional polynomial. This allows the dark current to be a function of temperature, or time since PON. To do this, added new file type, DARK. A DARK file is just like an IMAGE, except that it has a table per FITS file that contains the parameters to use in applying the dark. It's kinda like a FRINGE, but there's only one table per file, instead of one table per extension.

File:
1 edited

Legend:

Unmodified
Added
Removed
  • trunk/psModules/src/camera/pmFPAfile.h

    r16355 r16841  
    44 * @author EAM, IfA
    55 *
    6  * @version $Revision: 1.28 $ $Name: not supported by cvs2svn $
    7  * @date $Date: 2008-02-07 23:45:56 $
     6 * @version $Revision: 1.29 $ $Name: not supported by cvs2svn $
     7 * @date $Date: 2008-03-06 20:47:50 $
    88 * Copyright 2004-2005 Institute for Astronomy, University of Hawaii
    99 */
     
    2828    PM_FPA_FILE_RAW,
    2929    PM_FPA_FILE_IMAGE,
     30    PM_FPA_FILE_MASK,
     31    PM_FPA_FILE_WEIGHT,
     32    PM_FPA_FILE_FRINGE,
     33    PM_FPA_FILE_DARK,
    3034    PM_FPA_FILE_PSF,
    3135    PM_FPA_FILE_JPEG,
    3236    PM_FPA_FILE_KAPA,
    33     PM_FPA_FILE_MASK,
    34     PM_FPA_FILE_WEIGHT,
    35     PM_FPA_FILE_FRINGE,
    3637    PM_FPA_FILE_HEADER,
    3738    PM_FPA_FILE_ASTROM,
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