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author | William Joye <wjoye@cfa.harvard.edu> | 2016-10-26 21:13:00 (GMT) |
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committer | William Joye <wjoye@cfa.harvard.edu> | 2016-10-26 21:13:00 (GMT) |
commit | da2e3d212171bbe64c1af39114fd067308656990 (patch) | |
tree | 9601f7ed15fa1394762124630c12a792bc073ec2 /funtools/wcs/Files | |
parent | 76b109ad6d97d19ab835596dc70149ef379f3733 (diff) | |
download | blt-da2e3d212171bbe64c1af39114fd067308656990.zip blt-da2e3d212171bbe64c1af39114fd067308656990.tar.gz blt-da2e3d212171bbe64c1af39114fd067308656990.tar.bz2 |
rm funtools for update
Diffstat (limited to 'funtools/wcs/Files')
-rw-r--r-- | funtools/wcs/Files | 179 |
1 files changed, 0 insertions, 179 deletions
diff --git a/funtools/wcs/Files b/funtools/wcs/Files deleted file mode 100644 index 94d18da..0000000 --- a/funtools/wcs/Files +++ /dev/null @@ -1,179 +0,0 @@ -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 |