1IMAGE2XY(1) astrometry.net IMAGE2XY(1)
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6 image2xy - Source extractor.
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9 image2xy [options] fitsname.fits
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12 Read a FITS file, find objects, and write out X, Y, FLUX to fit‐
13 sname.xy.fits.
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16 -e extension
17 Read from a single FITS extension
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19 -O Overwrite existing output file.
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21 -o file
22 Write XYlist to given filename.
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24 -L order
25 Lanczos order
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27 -8 Don't use optimization for byte (u8) images.
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29 -H Downsample by a factor of 2 before running simplexy.
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31 -d factor
32 Downsample by an integer factor before running simplexy.
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34 -D factor
35 Downsample, if necessary, by this many factors of two.
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37 -s scale
38 Set median-filter box size (default 100 pixels)
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40 -w width
41 Set Gaussian PSF sigma (default 1 pixel)
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43 -g sigma
44 Set image noise level
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46 -p significance
47 Set significance level of peaks in sigmas (default 8 sigmas)
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49 -a saddle
50 Set "saddle" level joining peaks i sigmas (default 5 sigmas)
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52 -P plane
53 Pull out a single plane of a multi-color image (default: first
54 plane)
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56 -b Don't do (median-based) background subtraction
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58 -G background
59 Subtract this 'global' background value; implies -b
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61 -m Set maximum extended object size for deblending (default 2000
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64 -S file
65 Save background-subtracted image to this filename (FITS float
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68 -B file
69 Save background image to filename
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71 -U file
72 Save smoothed background-subtracted image to filename
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74 -M file
75 Save mask image to filename
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77 -C file
78 Save connected-components image to filename
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80 -v Verbose. repeat for more and more verboseness
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82 image2xy 'file.fits[1]'
83 Process first extension.
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85 image2xy 'file.fits[2]'
86 Process second extension
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88 image2xy file.fits+2
89 Same as above
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92 The Astrometry.net team. Principal investigators are David W. Hogg
93 (NYU) and Dustin Lang (CMU).
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96 http://astrometry.net
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1000.56 July 2015 IMAGE2XY(1)