image2xy (1)
NAME
image2xy - Source extractor.
SYNOPSIS
image2xy
[options]
fitsname.fits
DESCRIPTION
Read a FITS file, find objects, and write out X, Y, FLUX to fitsname.xy.fits.
OPTIONS
- -e extension
-
Read from a single FITS extension
- -O
-
Overwrite existing output file.
- -o file
-
Write XYlist to given filename.
- -L order
-
Lanczos order
- -8
-
Don't use optimization for byte (u8) images.
- -H
-
Downsample by a factor of 2 before running simplexy.
- -d factor
-
Downsample by an integer factor before running simplexy.
- -D factor
-
Downsample, if necessary, by this many factors of two.
- -s scale
-
Set median-filter box size (default 100 pixels)
- -w width
-
Set Gaussian PSF sigma (default 1 pixel)
- -g sigma
-
Set image noise level
- -p significance
-
Set significance level of peaks in sigmas (default 8 sigmas)
- -a saddle
-
Set "saddle" level joining peaks i sigmas (default 5 sigmas)
- -P plane
-
Pull out a single plane of a multi-color image (default: first plane)
- -b
-
Don't do (median-based) background subtraction
- -G background
-
Subtract this 'global' background value; implies -b
- -m
-
Set maximum extended object size for deblending (default 2000 pixels)
- -S file
-
Save background-subtracted image to this filename (FITS float image)
- -B file
-
Save background image to filename
- -U file
-
Save smoothed background-subtracted image to filename
- -M file
-
Save mask image to filename
- -C file
-
Save connected-components image to filename
- -v
-
Verbose. repeat for more and more verboseness
- image2xy 'file.fits[1]'
-
Process first extension.
- image2xy 'file.fits[2]'
-
Process second extension
- image2xy file.fits+2
-
Same as above
AUTHOR
The Astrometry.net team. Principal investigators are David W. Hogg (NYU) and
Dustin Lang (CMU).
SEE ALSO
astrometry.net