Figure 11 from LOW FALSE POSITIVE RATE OF KEPLER CANDIDATES ESTIMATED FROM A COMBINATION OF SPITZER AND FOLLOW-UP OBSERVATIONS

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LOW FALSE POSITIVE RATE OF KEPLER CANDIDATES ESTIMATED FROM A COMBINATION OF SPITZER AND FOLLOW-UP OBSERVATIONS

Authors: Jean-Michel Désert, David Charbonneau, Guillermo Torres, François Fressin, Sarah Ballard, Stephen T. Bryson, Heather A. Knutson, Natalie M. Batalha, William J. Borucki, Timothy M. Brown, Drake Deming, Eric B. Ford, Jonathan J. Fortney, Ronald L. Gilliland, David W. Latham, and Sara Seager

2015 The Astrophysical Journal 804 59.

Provider: AAS Journals

Caption: Figure 11.

Transiting planet frequency distribution as a function of period bins (in logarithmic scale). The distribution is derived from the list of KOIs published in Batalha et al. (2013), assuming that all the detected signals are of planetary origin.

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