hpxcvt(1) [debian man page]

HPXCVT(1)							   User Commands							 HPXCVT(1)

NAME

       HPXcvt - Reorganise HEALPix data into a 2-D FITS image

SYNOPSIS

       HPXcvt [-C<col>] [-c<sys>] [-n|-r] [-q<quad>] [-x<n|s>]

DESCRIPTION

	      [<infile> [<outfile>]]

       HPXcvt reorganises HEALPix data into a 2-D FITS image with HPX coordinate system.  The input data may be stored in a FITS file as a primary
       image or image extension, or as a binary table extension.  Both NESTED and RING pixel indices are supported.  The input	and  output  files
       may be omitted or specified as "-" to indicate stdin and stdout respectively.

OPTIONS

       -C<col>
	      Binary table column number from which to read data, default 1 (n.b. WMAP exclusion masks are in column 2).

       -c<sys>
	      Specify  the  coordinate	system	to  be	used to label the output map if the COORDSYS keyword is absent from the input FITS header.
	      Recognised values are g (galactic), e (ecliptic) or q (equatorial).

       -n|-r  Assume n(ested) or r(ing) organization if the ORDERING keyword is absent from the input FITS header.

       -q<quad>
	      Recentre longitude at quad(mod 4) x 90 degrees, where quad(rant) is an integer.

       -x<n|s>
	      Use a north-polar or south-polar layout.

HPXcvt 4.13.4							    April 2012								 HPXCVT(1)

WCSREMAP(1)							   User Commands						       WCSREMAP(1)

NAME

       wcsremap - AME

SYNOPSIS

       remap [-vf][-a rot][[-b][-j] ra dec][-i bits][-l num] file1.fit file2.fit ... filen.fit

DESCRIPTION

       Remap FITS or IRAF images into single FITS image using WCS

	      or  :  remap  [-vf][-a  rot][[-b][-j] ra dec][-i bits][-l num] @filelist -a: Output rotation angle in degrees (default 0) -b ra dec:
	      Output center in B1950 (FK4) RA and Dec -e long lat: Output center in ecliptic longitude and latitude -f file:  Use  WCS	from  this
	      file as output WCS -g long lat: Output center in galactic longitude and latitude -i num: Number of bits per output pixel (default is
	      input) -j ra dec: center in J2000 (FK5) RA and Dec -l num: Log every num rows of output image -m mode:  c  closest  pixel  (more	to
	      come)  -n  num:  integer	pixel  value  for blank pixel -o name: Name for output image -p secpix: Output plate scale in arcsec/pixel
	      (default =input) -s: Set BZERO and BSCALE in output file from input file -t: Number of samples per linear output	pixel  -u:  Delete
	      distortion  keywords from output file -v: Verbose -w type: Output WCS type (input is default) -x x y: Output image reference X and Y
	      coordinates (default is center) -y nx ny: Output image dimensions (default is first input image)

wcsremap 3.8.4							     June 2012							       WCSREMAP(1)