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HASTROM

HASTROM

Name


      HASTROM

Purpose


      Transformation of an image to align it with a reference image

Explanation


      A transformation is applied (using POLY_2D) to an image so that
      its astrometry is identical with that in a reference header. This
      procedure can be used to align two images.

Calling Sequence


      HASTROM, oldim, oldhd, newim, newhd, refhd, [MISSING =, INTERP = ]
                            or
      HASTROM, oldim, oldhd, refhd, [MISSING =, INTERP ={0,1,2}, NGRID =,
                                      CUBIC =, DEGREE = ]

Inputs


      OLDIM - Image array to be manipulated. If only 3 parameters are
              supplied then OLDIM and OLDHD will be modified to contain
              the output image array and header
      OLDHD - FITS header array for OLDIM, containing astrometry parameters
      REFHD - Reference header, containing astrometry parameters. OLDIM
              will be rotated, shifted, and compressed or expanded until
              its astrometry matches that in REFHD.

Outputs


      NEWIM - Image array after transformation has been performed.
              The dimensions of NEWIM will be identical to the NAXIS1 and
              NAXIS2 keywords specified in REFHD. Regions on the reference
              image that do not exist in OLDIM can be assigned a value with
              the MISSING keyword.
      NEWHD - Updated FITS image header associated with NEWIM

Optional Input Keywords


      CUBIC - a scalar value between -1 and 0 specifying cubic interpolation
              with the specified value as the cubic interpolation parameter.
              (see poly_2d for info). Setting CUBIC to a value greater
              than zero is equivalent to setting CUBIC = -1.
      DEGREE - Integer scalar specifying the degree of the transformation.
              See the routine POLYWARP for more info. Default =
              1 (linear transformation) unless polynomial ('SIP') distortion
              parameters are present in either the input or reference FITS
              header. In that case, the default degree is equal to the
              degree of the distortion polynomial.
      INTERP - Scalar, one of 0, 1, or 2 determining type of interpolation
              0 nearest neighbor, 1 (default) bilinear interpolation,
              2 cubic interpolation.
      MISSING - Set this keyword to a scalar value which will be assigned
              to pixels in the output image which are out of range of the
              supplied imput image. If not supplied, then linear
              extrapolation is used. See the IDL manual on POLY_2D.
              ***NOTE: A bug was introduced into the POLY_2D function in IDL
              V5.5 (fixed in V6.1) such that the MISSING keyword
              may not work properly with floating point data***
      NGRID - Integer scalar specifying the number of equally spaced grid
              points on each axis to use to specify the transformation.
              The value of NGRID must always be greater than DEGREE + 1.
              The default is DEGREE + 2 which equals 3 (9 total points) for
              DEGREE=1 (linear warping).
      SILENT - If set, then some informational error messages are suppressed.

Optional Output Keyword


      ERRMSG - If this keyword is supplied, then any error messages will be
              returned to the user in this parameter rather than depending on
              on the MESSAGE routine in IDL. If no errors are encountered
              then a null string is returned.

Notes


      (1) The 3 parameter calling sequence is less demanding on virtual
              memory.
      (2) The astrometry in OLDHD will be precessed to match the equinox
                given in REFHD.
      (3) If an ST Guidestar image is used for the reference header, then the
                output header will be converted to standard astrometry.

Example


      Suppose one has an image array, IM, and an associated FITS header H.
      One desires to warp the image array so that it is aligned with another
      image with a FITS header, HREF. Both headers contain astrometry info.
      Set pixel values to 0 where there is no overlap between the input and
      reference image, and use linear interpolation (default)
      IDL> hastrom, IM, H, HREF, MISSING = 0

Procedures Used


      ad2xy, check_FITS, extast, get_EQUINOX(), gsssextast, hprecess,
      putast, sxaddpar, sxaddhist, sxpar(), xy2ad, zparcheck

Revision History


      Written W. Landsman, STX Co. Feb, 1989
      Updated to CHECK_FITS Dec, 1991
      New astrometry keywords Mar, 1994
      Recognize GSSS header W. Landsman June, 1994
      Added CUBIC keyword W. Landsman March, 1997
      Accept INTERP=0, Convert output GSS header to standard astrometry
                              W. Landsman June 1998
      Remove calls to obsolete !ERR system variable March 2000
      Added ERRMSG output keyword W. Landsman April 2000
      Need to re-extract astrometry after precession W. Landsman Nov. 2000
      Check for distortion parameters in headers, add more FITS HISTORY
      information W. Landsman February 2005
      Use different coefficient for nearest neighbor to avoid half-pixel
      shift with POLY_2D W. Landsman Aug 2006
      Return ERRMSG if no overlap between images W. Landsman Nov 2007
      Use V6.0 notation W. Landsman Jan 2012
     



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