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The 1 column in color are computed by VizieR, and are not part of the original data.

Note: This version of the GSC-II has no proper motions, but the limits on brightness which existed on GSC2.2 (F<18.5, Bj<19.5) were removed.

I/305/out The Guide Star Catalog, Version 2.3.2 (GSC2.3) (STScI, 2006)
The Full GSC2.3.2 Catalogue (945592683 objects) (945592683 rows)
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14.779NC6D010776037.910195+22.9161181991.75720.5522.03    3 1.48 0.39

Note: SDSS is also available from http://www.sdss.org/

II/294/sdss7 The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)
Data Release 7 (357,175,411 primary sources, plus 65,714,108 secondary sources) (65714108 rows) (Note)
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14.84316J023138.40+225455.4    25.982 0.54823.332 0.28222.678 0.20422.355 0.21621.681 0.376037.910004+22.9154042005.93102

Note: SDSS is also available from http://www.sdss3.org/dr9/

V/139/sdss9 The SDSS Photometric Catalog, Release 9 (Adelman-McCarthy+, 2012)
Data Release 9 (469,053,874 primary sources plus 324,960,076 secondary sources); 2,674,200 spectroscopic targets. Data Release 9 is the first release of the spectra from the SDSS-III's Baryon Oscillation Spectroscopic Survey (BOSS). The photometric part contains the same sources as the Data Release 8, with a corrected astrometry. (794013950 rows) (Note)
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10.0001  6J023138.10+225457.9  Im037.908754+22.9161002005.9310324.967 0.88823.958 0.41823.177 0.33022.377 0.22821.893 0.477  
24.8281+6J023138.40+225455.4  Im037.909998+22.9154032005.9310325.684 0.62722.727 0.16422.058 0.13322.555 0.27822.034 0.543  

Note:

V/147/sdss12 The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)
Data Release 12 (469,053,874 primary sources plus 324,960,094 secondary sources); 3,538,079 spectroscopic targets (original column names in green) (794013968 rows) (Note)
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14.828037.909998+22.9154031+6J023138.39+225455.4  2005.9311325.684 0.62722.727 0.16422.058 0.13322.555 0.27822.034 0.543        
20.000037.908754+22.9161001  6J023138.10+225457.9  2005.9311324.967 0.88823.958 0.41823.177 0.33022.377 0.22821.893 0.477        
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