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MKDARK

MKDARK

Name


  mkdark

Purpose


  Collect and combine CCD dark frames into a superdark frame

Description



  The files are assumed to be named as 'root'NNN where 'root' is the
  root of the file name that you supply and NNN is a three digit number.
  If your file name has an imbedded '.' then add it to the root.
  The specified range of files are all read in from FITS files. Then each
  image has the overscan mean subtracted (if desired), cropped (as indicated),
  and then the input bias image is subtracted. These images are then
  normalized to counts per second and then averaged. The averaging
  is done with AVGCLIP.PRO which does a robust average of the image
  stack so that cosmic rays or other transient image defects are eliminated.
  When done, the resulting dark image is returned to the caller and the image
  is saved to a FITS file with the specified output filename.

Category


  CCD data processing

Calling Sequence


  mkdark,root,outsuf,start,nframes,bias,dark

Inputs


  root - Root of the file name (you must include . in the name).
  outsuf - The suffix of the final output file.
  start - First frame number to read (integer or long).
              Start can also be a vector of explicit frame numbers to load.
              In this case, nframes need not be specified and in fact will
              be ignored.
              Additionally, start can also be a string array containing the
              file names of all files to be read. In this case, set nframes
              to 0 or someother innocuous integer. Exclude is treated
              differently. In this case, exclude is a vector of the same
              length as start and is 0 if the file is to be used, 1 if not.
  nframes - Number of frames to average.
  bias - Name of bias frame image to subtract from each raw dark.

Optional Input Parameters


Keyword Input Parameters



  CROP = region of original image to save, default=no cropping.
                [x1,x2,y1,y2]
  DDIR - Path to the raw data, default = ''
  EXCLUDE - Optional vector of image numbers that should be excluded from
                average. Default is to include all frames.
  EXPKEY = String - FITS keyword to read to get exposure time, default = EXPTIME
  OVERSCAN = column overscan region to use for frame bias level,
                default=no overscan subtraction.
  RDNOISE - Read noise of CCD, e-/DN, default=10

Outputs


  dark - Final robust averaged dark image scaled to counts per second.

Keyword Output Parameters


Common Blocks


Side Effects


Restrictions


Procedure


Modification History


  95/03/09 - Initial crude version written, Marc W. Buie, Lowell Observatory
  95/08/30, MWB, added OVERSCAN and CROP keywords
  95/11/22, MWB, add EXCLUDE keyword
  99/06/10, MWB, added EXPTIME keyword and added documentation.
  2001/02/23, MWB, added option to provide input file list. Also, added
                    functions to make it consistent with mkbais,mkflat.
  2005/03/10, MWB, added DDIR keyword, converted bias input to string
  2006/07/14, MWB, added RDNOISE keyword



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