Figure 1 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 1.

Candidate radii as a function of their orbital periods (black point) for all the KOIs presented in Batalha et al. (2013). Overplotted in red are the 51 KOIs that we targeted to estimate the FPR from Kepler and that are presented in this paper. We observe these 51 objects during transit in the near-infrared with Spitzer. Our selected sample spans a wide range of periods and sizes.

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