Figure 15 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 15.

Top: FPP for each Kepler candidate (KOI) that we followed up with Spitzer as a function of the target star’s Galactic latitude. Bottom: FPP as a function of the Kepler magnitude. The overall FPPs increase as the Kepler magnitude increases and the Galactic latitude decreases.

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