Figure 8 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 8.

Same as Figure 6, but the eclipsing binary system is now blended with a primary star. These ratios are computed for an eclipsing binary stellar system composed of a secondary star of mass M₂ eclipsed by a tertiary stellar component that is blended with a primary star of solar mass (M₁ = 1). See Equation (4) for more details.

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