Man page - build-astrometry-index(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
BUILD-ASTROMETRY-INDEX
NAMESYNOPSIS
DESCRIPTION
OPTIONS
AUTHOR
SEE ALSO
NAME
build-astrometry-index - Create astrometry.net index files
SYNOPSIS
build-astrometry-index [options] -i catalog -o file -P scale
DESCRIPTION
build-astrometry-index takes a FITS catalog table containing at least RA , DEC , and magnitude columns and converts it into an index file that can be used by the astrometry.net programs like solve-index (1).
OPTIONS
-i catalog
Input FITS catalog: source RA,DEC, etc.
-e extension
FITS extension to read when -i is specified.
-1 index
Share another index’s stars (alternatively to -i / -e ).
-o file
Output filename for index
-N nside
Healpix Nside for quad-building
-l size
Minimum quad size (arcminutes)
-u size
Maximum quad size (arcminutes)
-P number
Use ’preset’ values for -N , -l , and -u . The scale-number is the last two digits of the pre-cooked index filename -- eg., index-205 is -P 5 .
-P 0 should be good for images about 6 arcmin in size and it goes in steps of sqrt(2), so:
-P 2 should work for images about 12 arcmin across
-P 4 should work for images about 24 arcmin across
-P 6 should work for images about 1 degree across
-P 8 should work for images about 2 degree across
-P 10 should work for images about 4 degree across etc... up to -P 19
-S column
Sort column (default: assume the input file is already sorted)
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-f |
Sort in descending order (eg, for FLUX); default ascending (eg, for MAG) |
-A column
Specify the RA column name in the input FITS table (default "RA")
-D column
Specify the Dec column name in the input FITS table (default "Dec")
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-B val |
Cut any object whose sort-column value is less than val ; for mags this is a bright limit |
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-U |
Healpix Nside for uniformization (default: same as -n ) |
-H big healpix
Big healpix; default is all-sky
-s Nside
Big healpix Nside; default is 1
-m margin
Add a margin of margin healpixels; default 0
-n sweeps
Sweeps (ie, number of stars per fine healpix grid cell); default 10
-r radius
Deduplication radius in arcseconds; default no deduplication
-j jitter
Positional error of stars in the reference catalog (in arcsec; default 1)
-d dimquads
Number of stars in a "quad" (default 4).
-p passes
Number of rounds of quad-building (ie, number of quads per healpix cell, default 16)
-R reuse
Number of times a star can be used (default: 8)
-L max-reuses
Make extra passes through the healpixes, increasing the -r reuse limit each time, up to max-reuses .
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-E |
Scan through the catalog, checking which healpixes are occupied. |
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-I id |
Set the unique ID of this index |
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-M |
In-memory (don’t use temp files) |
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-T |
Don’t delete temp files |
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-t dir |
Use this temp directory (default: /tmp) |
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-v |
Add verbosity. |
AUTHOR
The Astrometry.net team. Principal investigators are David W. Hogg (NYU) and Dustin Lang (CMU).
SEE ALSO
hpsplit (1),
solve-field (1)
For a tutorial, see
http://astrometry.net/doc/build-index.html