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Basri, Guillermo Torres, Hans Kjeldsen, Howard Isaacson, Jack J. Lissauer, Jason F. Rowe, Jason H. Steffen, Jeffrey C. Smith, Jeffrey Van Cleve, Jessie Christiansen, Jill Tarter, John Asher Johnson, Jonathan J. Fortney, Jon M. Jenkins, Jorgen Christensen-Dalsgaard, Joseph D. Twicken, Lars A. Buchhave, Leslie Rogers, Lucianne M. Walkowicz, Matthew J. Holman, Michael R. Haas, Natalie M. Batalha, Pavel Machalek, Peter Tenenbaum, Philip W. Lucas, Robert C. Morehead, Robert L. Morris, Ronald L. Gilliland, Samuel N. Quinn, Sara Seager, Stephen T. Bryson, Steve B. Howell, Thomas N. Gautier III, Timothy D. Morton, Timothy M. Brown, Todd C. Klaus, William D. Cochran, William F. Welsh, William J. Borucki","submitted_at":"2011-03-13T18:51:02Z","abstract_excerpt":"We report the distribution of planets as a function of planet radius (R_p), orbital period (P), and stellar effective temperature (Teff) for P < 50 day orbits around GK stars. 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