PLANET OCCURRENCE WITHIN 0.25 AU OF SOLAR-TYPE STARS FROM <i>KEPLER</i>

W. Howard, Andrew; W. Marcy, Geoffrey; Bryson, Steve; M. Jenkins, Jon; F. Rowe, Jason; M. Batalha, Natalie; J. Borucki, W.; Koch, David; W. Dunham, Edward; N. Gautier, T.; Van Cleve, Jeffrey; D. Cochran, William; W. Latham, David; J. Lissauer, Jack; Torres, Guillermo; M. Brown, Timothy; L. Gilliland, Ronald; A. Buchhave, Lars; A. Caldwell, Douglas; Christensen‐Dalsgaard, J.; R. Ciardi, David; Fressin, François; R. Haas, Michael; B. Howell, Steve; Kjeldsen, H.; Seager, Sara; A. Rogers, Leslie; Sasselov, Dimitar; H. Steffen, Jason; Basri, Gibor; Charbonneau, David; L. Christiansen, Jessie; Clarke, Bruce; K. Dupree, A.; C. Fabrycky, Daniel; A. Fischer, Debra; B. Ford, Eric; J. Fortney, Jonathan; Tarter, Jill; R. Girouard, Forrest; J. Holman, Matthew; Asher Johnson, John; C. Klaus, Todd; Machálek, Pavel; V. Moorhead, Althea; C. Morehead, Robert; Ragozzine, Darin; Tenenbaum, Peter; D. Twicken, Joseph; N. Quinn, Samuel; Isaacson, Howard; Shporer, Avi; W. Lucas, P.; M. Walkowicz, Lucianne; F. Welsh, William; P. Boss, Alan; DeVore, Edna; Gould, Alan; C. Smith, Jeffrey; Morris, Robert; Prša, A.; D. Morton, Timothy; Still, Martin; E. Thompson, Susan; Mullally, Fergal; Endl, Michael; J. MacQueen, Phillip

doi:10.1088/0067-0049/201/2/15

Public

PLANET OCCURRENCE WITHIN 0.25 AU OF SOLAR-TYPE STARS FROM KEPLER

Published in The Astrophysical Journal Supplement Series • Jun 25, 2012

Authors:

Andrew W. Howard

Geoffrey W. Marcy

Steve Bryson

Abstract

We report the distribution of planets as a function of planet radius, orbital period, and stellar effective temperature for orbital periods less than 50 days around solar-type (GK) stars. These results are based on the 1235 planets (formally "planet candidates") from the Kepler mission that include ...

Subject

Planet

Physics

Astrophysics

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