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We provide updates to the Kepler planet candidate sample based upon nearlytwo years of high-precision photometry (i.e., Q1-Q8). From an initial list ofnearly 13,400 Threshold Crossing Events (TCEs), 480 new host stars areidentified from their flux time series as consistent with hosting transitingplanets. Potential transit signals are subjected to further analysis using thepixel-level data, which allows background eclipsing binaries to be identifiedthrough small image position shifts during transit. We also re-evaluate KeplerObjects of Interest (KOI) 1-1609, which were identified early in the mission,using substantially more data to test for background false positives and tofind additional multiple systems. Combining the new and previous KOI samples,we provide updated parameters for 2,738 Kepler planet candidates distributedacross 2,017 host stars. From the combined Kepler planet candidates, 472 arenew from the Q1-Q8 data examined in this study. The new Kepler planetcandidates represent ~40% of the sample with Rp~1 Rearth and represent ~40% ofthe low equilibrium temperature (Teq<300 K) sample. We review the known biasesin the current sample of Kepler planet candidates relevant to evaluating planetpopulation statistics with the current Kepler planet candidate sample.

Planetary Candidates Observed by Kepler IV: Planet Sample From Q1-Q8 (22 Months)