Example 2.
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This sample image contains world coordinate system fit by
imwcs in
Example 1.
The following header keywords define the WCS:
EQUINOX = 2000 CTYPE1 = 'RA---TAN' CRVAL1 = 243.987 CRPIX1 = 512 CDELT1 = -0.000179207 CROTA1 = -0.0727298 CTYPE2 = 'DEC--TAN' CRVAL2 = 31.4185 CRPIX2 = 512 CDELT2 = 0.000179207 CROTA2 = 0 IMWCS = 'IMWCS 1.0, 28 June 1996, Doug Mink SAO' |
To list the HST Guide Stars in the image, the threshold for a pixel to be checked out as a possible star was set to 5000, and the program was run.
$ immatch -c ua2 -d testx90mwg.sex testx90mwg.fitsgiving the results
# Arcsec/Pixel: -0.645145 0.645145 Rotation: -0.072730 degrees # Optical axis: 16:15:56.880 +31:25:06.60 J2000 at (512.00,512.00) # Optical axis: 16:13:59.776 +31:32:29.78 B1950 at (512.00,512.00) # 12 matches between gsc and testx90mwg.fits: 2580.1629 16:15:55.896 +31:19:58.40 13.91 528.5 33.5 -2.15 0.50 1.65 2580.1878 16:16:10.956 +31:21:42.41 14.92 229.8 196.1 -2.11 -0.12 1.54 2580.1909 16:15:37.282 +31:23:51.97 14.76 899.7 396.1 -0.99 -0.10 0.73 2580.1798 16:15:34.867 +31:24:43.45 14.16 947.9 475.8 -0.78 -0.03 0.57 2580.1485 16:15:52.958 +31:25:15.56 14.88 588.8 526.6 -0.87 -0.51 0.81 2580.2291 16:16:08.345 +31:26:15.76 13.81 283.5 620.5 -1.06 -0.63 0.99 2580.1943 16:15:41.477 +31:26:37.54 14.84 817.0 653.4 -0.60 -0.46 0.64 2580.1696 16:15:49.339 +31:26:42.40 13.38 661.3 661.0 -0.44 -0.45 0.55 2580.1207 16:15:45.511 +31:27:48.64 13.50 737.1 763.5 -0.61 -0.35 0.56 2580.1158 16:16:12.139 +31:28:54.01 13.99 209.4 861.3 -0.41 2.37 2.39 2580.2147 16:16:21.072 +31:29:28.82 14.47 30.2 921.7 -2.36 -1.57 2.32 2580.1403 16:15:34.330 +31:30:06.66 13.59 960.5 978.4 0.78 -1.07 1.21 # Mean dx= 1.0915/1.4499 dy= -0.3127/1.4632 dxy= 1.8041 # Mean dra= -0.9669/1.2849 ddec= -0.2007/0.9435 sep= 1.1639In the table, the first column is the star identifier. The second, third, and fourth columns are the catalog right ascension, declination, and magnitude for the star. The next two columns are the center X and Y coordinates of the center of the star in the image. The last three columns are the offset of the catalog position from the image star center in arcseconds in the right ascension and declination directions (horizontally and vertically) and radially.
The verbose mode gives more information about how the fit is going:
$ > immatch -vc gsc -i 5000 testx90mwg.fits