Man page - fit-wcs(1)
Packages contains this manual
- fits-flip-endian(1)
- an-pnmtofits(1)
- wcs-rd2xy(1)
- tabsort(1)
- plot-constellations(1)
- solve-field(1)
- an-fitstopnm(1)
- wcsinfo(1)
- fits-guess-scale(1)
- query-starkd(1)
- wcs-match(1)
- wcs-to-tan(1)
- fitsgetext(1)
- fit-wcs(1)
- wcs-xy2rd(1)
- astrometry-engine(1)
- get-wcs(1)
- subtable(1)
- fits-column-merge(1)
- hpsplit(1)
- image2xy(1)
- coadd(1)
- wcs-pv2sip(1)
- wcs-grab(1)
- plotxy(1)
- downsample-fits(1)
- build-astrometry-index(1)
- pad-file(1)
- get-healpix(1)
- plotquad(1)
- new-wcs(1)
- wcs-resample(1)
apt-get install astrometry.net
Manual
FIT-WCS
NAMESYNOPSIS
DESCRIPTION
OPTIONS
AUTHOR
SEE ALSO
NAME
fit-wcs - Fit a transformation from x,y and matching RA,DEC coordinates
SYNOPSIS
fit-wcs
[options]
-x
file
-r file
fit-wcs
[options]
-c
file
DESCRIPTION
Given a list of x,y coordinates and matching RA,Dec coordinates, fit a transformation and produce a WCS file
OPTIONS
-x file
XYls input file
-X name
X column name (default: FIELD_X)
-Y name
Y column name (default: FIELD_Y)
-r file
RDls input file
-R name
RA column name (default: INDEX_RA)
-D name
Dec column name (default: INDEX_DEC)
-c file
Correspondences file
-o file
WCS output file
|
-s sip |
SIP order (default is a WCS TAN solution, not SIP) |
-W width
Image width (default: max X position; used for SIP)
-H height
Image height (default: max Y position; used for SIP)
|
-C |
Set CRPIX to be the center of the field; SIP only |
|||
|
-v |
Verbose |
AUTHOR
The Astrometry.net team. Principal investigators are David W. Hogg (NYU) and Dustin Lang (CMU).
SEE ALSO
http://astrometry.net