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-WCSTools libwcs Subroutines (3.9.0, March 11, 2011)
-
-actread.c
-  Return stars from the USNO ACT Reference Catalog
-binread.c
-  Return stars from catalog files in the TDC binary catalog format
-catread.c
-  Return stars from catalog files in the TDC ASCII catalog format
-catutil.c
-  Subroutines for catalog identification and number range decoding
-cel.c
-  WCSLIB spherical coordinate transformation drivers
-daoread.c
-  Read x, y, and magnitude from DAOFIND output file and return x, y, and
-  flux for use by IMSTAR or IMWCS.
-dateutil.c
-  Subroutines for conversions between various date and time formats
-distort.c
-  Subroutines for conversions between image pixel and focal plane coordinates
-dsspos.c
-  dsspos() uses the WCS structure to compute sky coordinates given
-  image pixel X and Y for images with Digitized Sky Survey plate solutions
-  in their headers.  dsspix() uses the WCS structure to compute image
-  pixel X and Y given sky coordinates for DSS images.  Algorithms from
-  StSCI CASB.
-fileutil.c
-  Subroutines for finding size and contents of ASCII files
-findstar.c
-  findStars() gets the location and brightest pixel of stars in the given
-  image.  Included are subroutines to find and reject bright pixels and
-  compute a star centroid.
-fitsfile.c
-  FITS header and image reading and writing subroutines, including FITS
-  table support.
-fitswcs.c
-  GetWCSFITS() returns a WCS structure used by wcs.c subroutines from a FITS
-  or IRAF .imh image, reading only the header.
-  GetFITShead() returns a FITS header from a FITS or IRAF .imh image.
-  DelWCS() delete the WCS keywords in a FITS header.
-fortcat.c
-  Fortran wrapper subroutines for catalog reading subroutines ctgread() and ctgrnum()
-fortwcs.c
-  Fortran wrapper subroutines for all useful subroutines in wcs.c and wcsinit.c
-gscread.c
-  Return HST Guide Stars from standard CDROM format FITS table files for
-  a given RA, Dec, and magnitude range or list of star numbers.
-gsc2read.c
-  Return GSC II Stars using an HTTP query over the web for
-  a given RA, Dec, and magnitude range or list of star numbers.
-hget.c
-  Subroutines to extract values from FITS headers by keyword.
-  Subroutines for parsing RA and Dec strings are included.
-hput.c
-  Subroutines to implant values into FITS headers by keyword (and to
-  delete headers).
-iget.c
-  Subroutines to extract values from IRAF multi-keyword header parameters
-imhfile.c
-  IRAF header and image reading and writing subroutines.  IRAF headers
-  are converted to FITS headers for use by other programs and can be
-  derived from FITS headers for writing.
-imio.c
-  Subroutines to get, put, and move pixels of various data types between images
-  im memory and a program.
-imrotate.c
-  RotFITS() rotates an image by 90, 180, or 270 degrees, with an optional
-  left-right reflection before the rotation.
-imgetwcs.c
-  GetWCSFITS() reads world coordinate system header information and returns
-  the image center coordinates and size as well as the wcs data structure.
-imsetwcs.c
-  SetWCSFITS() uses findStars to find the stars in an image, gscread to
-  find the Guide Stars in the nominal image region, and findRegisration or
-  findCoords to fit plate-tangent WCS to the image.
-lin.c
-  WCSLIB linear transformation subroutines
-matchstar.c
-  StarMatch() takes a list of reference star positions and a list
-  of object coordinates from an image and finds the image pixels
-  which correspond to each of the reference stars.  It then uses these
-  matches to get an image center, plate scale, and rotation.  The actual
-  fit is based on the amoeba subroutine in Numerical Recipes, and all
-  necessary subroutines are included.
-platepos.c
-  platepos() uses the WCS structure to compute sky coordinates given
-  image pixel X and Y for images with polynomial plate solutions
-  in their headers.  platepix() uses the WCS structure to compute image
-  pixel X and Y given sky coordinates for such images.  Algorithms are based
-  on those in dsspos.c, but go straight from pixels to angles without an
-  intermediate plate coordinate.
-poly.c
-  Polynomial evaluation for SCAMP distortion correction
-proj.c
-  WCSLIB spherical map projection subroutines
-sdssread.c
-  Return Sloan Digital Sky Survey Photometry Catalog sources using an
-  HTTP query over the web for a given RA, Dec, and magnitude range.
-sortstars.c
-  Subroutines to sort lists of stars by right ascension, magnitude, or flux
-sph.c
-  WCSLIB spherical coordinate transformation subroutines
-tabread.c
-  Return stars from a tab table format catalog file for a given RA, Dec,
-  and magnitude range or list of star numbers.  Based on John Roll's
-  Starbase format.
-tmcread.c
-  Return 2MASS Point Source Catalog stars from the catalog as ungzipped from
-  the DVD into (or linked from) a common root directory for a given RA, Dec,
-  and magnitude range or list of star numbers.  Both IDR2 and All-Sky release
-  formats are supported.
-tnxpos.c
-  tnxpos() uses the WCS keywords set up for IRAF's TNX projection to compute
-  sky coordinates given image pixel X and Y.  tnxpix() uses the WCS structure
-  to compute image pixel X and Y given sky coordinates for such images.  The
-  projection is a tangent plane with corrections between the rotation and
-  scaling and the actual projection.
-uacread.c
-  Return USNO A and SA Catalog stars from their standard CDROM format
-  files for a given RA, Dec, and magnitude range or list of star numbers.
-ubcread.c
-  Return USNO B Catalog stars from their standard format files for a
-  given RA, Dec, and magnitude range or list of star numbers.
-ucacread.c
-  Return USNO UCAC1, UCAC2, or UCAC3 Catalog stars from their standard format
-  files for a given RA, Dec, and magnitude range or list of star numbers.
-ujcread.c
-  Return USNO UJ Catalog stars from its standard CDROM format files for
-  a given RA, Dec, and magnitude range or list of star numbers.
-wcs.c
-  Subroutines for using FITS or IRAF header spatial world coordinate
-  system information.
-wcsinit.c
-  Subroutines to initialize WCS structure from a FITS header
-wcscon.c
-  Subroutines for converting between B1950, J2000, and galactic
-  coordinates, mostly based on Starlink SLA_LIB subroutines.
-webread.c
-  Open Starbase files across the Internet using HTTP queries
-worldpos.c
-  worldpos() uses the WCS structure to compute sky coordinates given
-  image pixel X and Y for images with header information for any of 8
-  standard world coordinate systems.  worldpix() uses the WCS structure
-  to compute image pixel X and Y given sky coordinates for the same images.
-  Mostly from NRAO.
-zpxpos.c
-  zpxpos() uses the WCS keywords set up for IRAF's ZPX projection to
-  compute sky coordinates given image pixel X and Y.  zpxpix() uses
-  the WCS structure to compute image pixel X and Y given sky coordinates
-  for such images.  The projection is a tangent plane with corrections
-  between the rotation and scaling and the actual projection.
-
-fitshead.h
-  Declarations of FITS header access subroutines
-fitsfile.h
-  Declarations of image access subroutines and FITS table data structure.
-imio.h
-  Declarations of subroutines to convert binary formats of numbers
-lwcs.h
-  Constants used by star-finding and WCS-setting subroutines
-wcscat.h
-  Declarations for star catalog data structures
-wcs.h
-  Declaration of WCS data structure and useful conversions.
-wcslib.h
-  Declarations for WCSLIB high level driver subroutines, trig and inverse
-  trig functions, spherical map projection subroutines, spherical coordinate
-  transformation drivers, and linear transformation subroutines
-
-* Notes:
-  WCSLIB subroutines were written by Mark Calabretta of CSIRO and have
-         been modified in several ways:
-         1) His distributed wcs.h has been changed to wcslib.h, and
-         2) wcstrig.c subroutine names have been changed from <function>d()
-            to <function>deg() to avoid name conflicts on some operating
-            systems.
-         3) ifndef's at start of headers files have been named to reflect
-            the names of the header files, i.e. wcslib_h_ in wcslib.h.
-         4) All header files have been combined into wcslib.h
-	 5) Emmanuel Bertin's SCAMP distortion has been added to proj.c:1