IMAGE2XY - Online Linux Manual Page

Section : 1
Updated : July 2015
Source : 0.56
Note : astrometry.net

NAMEimage2xy − Source extractor.

SYNOPSISimage2xy [options] fitsname.fits

DESCRIPTIONRead 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

AUTHORThe Astrometry.net team. Principal investigators are David W. Hogg (NYU) and Dustin Lang (CMU).

SEE ALSOhttp://astrometry.net
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