On 2011 February 1 the Kepler mission released data for 156453 stars observed from the beginning of the science observations on 2009 May 2 through September 16. There are 1235 planetary candidates with transit-like signatures detected in this period. These are associated with 997 host stars. Distributions of the characteristics of the planetary candidates are separated into five class sizes: 68 candidates of approximately Earth-size (R_p_<1.25R_{earth}), 288 super-Earth-size (1.25R{earth}<=R_p<2R_{earth}), 662 Neptune-size (2R{earth}<=R_p<6R_{earth}), 165 Jupiter-size (6R{earth}<=R_p_<15R_{earth}), and 19 up to twice the size of Jupiter (15R{earth}<=R_p<22R_{earth}_). In the temperature range appropriate for the habitable zone, 54 candidates are found with sizes ranging from Earth-size to larger than that of Jupiter. Six are less than twice the size of the Earth. Over 74% of the planetary candidates are smaller than Neptune. Multi-candidate, transiting systems are frequent; 17% of the host stars have multi-candidate systems, and 34% of all the candidates are part of multi-candidate systems.

Cone search capability for table J/ApJ/736/19/table4 (Very probable false positives)

Cone search capability for table J/ApJ/736/19/table1 (Host star characteristics)

Cone search capability for table J/ApJ/736/19/table2 (List of planetary candidates and their characteristics)