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 0
Johanes Gumabo
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