V/133               Kepler Input Catalog             (Kepler Mission Team, 2009)
The following files can be converted to FITS (extension .fit or fit.gz)
Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=V/133

drwxr-xr-x 138 cats archive 4096 Dec 13 14:19 [Up] drwxr-xr-x 3 cats archive 4096 Jan 29 17:15 [TAR file] -rw-r--r-- 1 cats archive 453 Nov 22 2012 .message -r--r--r-- 1 cats archive 6652 Nov 21 2012 ReadMe -rw-r--r-- 1 cats archive 1180 Nov 22 2012 +footg5.gif -rw-r--r-- 1 cats archive 3753 Nov 22 2012 +footg5.png -rw-r--r-- 1 cats archive 4394 Nov 22 2012 +footg8.gif -rw-r--r-- 1 cats archive 16720 Nov 22 2012 +footg8.png drwxr-xr-x 2 cats archive 4096 Sep 12 2010 kic
Beginning of ReadMe : V/133 Kepler Input Catalog (Kepler Mission Team, 2009) ================================================================================ Kepler Input Catalog Kepler Mission Team <Kepler Mission Team, NASA (2009)> =2009yCat.5133....0K ================================================================================ ADC_Keywords: Proper motions ; Effective temperatures ; Abundances, [Fe/H] Mission_Name: Kepler Description: The Kepler Mission, NASA Discovery mission #10, is specifically designed to survey our region of the Milky Way galaxy to discover hundreds of Earth-size and smaller planets in or near the habitable zone and determine how many of the billions of stars in our galaxy have such planets. The KIC, or Kepler Input Catalog, is the primary source of information about objects observed as part of the ground-based Kepler Spectral Classification Program (SCP) in preparation for the selection of Kepler PI and GO targets. The KIC lists objects down to 21mag, but it is not complete to this limit. Light from only about 1/3 of these objects falls on the Kepler CCD detector. A small number of the KIC objects are calibration objects distributed across the sky. For this reason the full KIC should never be used for Kepler target selection.