Modeling Kepler transit light curves as false positives: Rejection of blend scenarios for Kepler-9, and validation of Kepler-9d, a super-Earth-size planet in a multiple system
Guillermo Torres (1), Fran\c{c}ois Fressin (1), Natalie M. Batalha, (2), William J. Borucki (3), Timothy M. Brown (4), Stephen T. Bryson (3),, Lars A. Buchhave (5), David Charbonneau (1), David R. Ciardi (6), Edward W., Dunham (7), Daniel C. Fabrycky (1), Eric B. Ford (8)

TL;DR
This paper introduces the BLENDER method to analyze Kepler light curves, effectively distinguishing true planets from false positives, and validates Kepler-9d as a super-Earth in a multi-planet system.
Contribution
The study develops and applies the BLENDER technique to validate small exoplanets and rule out false positives in Kepler data, especially for super-Earth candidates.
Findings
Validated Kepler-9b and Kepler-9c as planets.
Confirmed Kepler-9d as a super-Earth-size planet.
Ruled out most false positive scenarios for the signals.
Abstract
Light curves from the Kepler Mission contain valuable information on the nature of the phenomena producing the transit-like signals. To assist in exploring the possibility that they are due to an astrophysical false positive, we describe a procedure (BLENDER) to model the photometry in terms of a "blend" rather than a planet orbiting a star. A blend may consist of a background or foreground eclipsing binary (or star-planet pair) whose eclipses are attenuated by the light of the candidate and possibly other stars within the photometric aperture. We apply BLENDER to the case of Kepler-9, a target harboring two previously confirmed Saturn-size planets (Kepler-9b and Kepler-9c) showing transit timing variations, and an additional shallower signal with a 1.59-day period suggesting the presence of a super-Earth-size planet. Using BLENDER together with constraints from other follow-up…
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