Figure 14 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 14.

Histogram distribution of the FPP of the Kepler candidates (KOIs) that we observed with Spitzer. Half of the overall sample has an FPP ﹩\lt \;1\%﹩. The vertical dashed line shows the 3σ upper limit of the FPR (8.8%) of the KOIs we present in this project (see Section 8.2).

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