# The Hunt for Exomoons with Kepler (HEK): V. A Survey of 41 Planetary Candidates for Exomoons

## Author(s): Kipping, DM; Schmitt, AR; Huang, X; Torres, G; Nesvorný, D; et al

To refer to this page use: http://arks.princeton.edu/ark:/88435/pr1nq59
DC FieldValueLanguage
dc.contributor.authorKipping, DM-
dc.contributor.authorSchmitt, AR-
dc.contributor.authorHuang, X-
dc.contributor.authorTorres, G-
dc.contributor.authorNesvorný, D-
dc.contributor.authorBuchhave, LA-
dc.contributor.authorHartman, J-
dc.contributor.authorBakos, Gaspar Aron-
dc.date.accessioned2019-04-10T19:30:45Z-
dc.date.available2019-04-10T19:30:45Z-
dc.date.issued2015-11en_US
dc.identifier.citationKipping, DM, Schmitt, AR, Huang, X, Torres, G, Nesvorný, D, Buchhave, LA, Hartman, J, Bakos, GÁ. (2015). The Hunt for Exomoons with Kepler (HEK): V. A Survey of 41 Planetary Candidates for Exomoons. \apj, 813 (14 - 14. doi:10.1088/0004-637X/813/1/14en_US
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr1nq59-
dc.description.abstractWe present a survey of 41 Kepler Objects of Interest (KOIs) for exomoons using Bayesian photodynamics, more than tripling the number of KOIs surveyed with this technique. We find no compelling evidence for exomoons although 13 KOIs yield spurious detections driven by instrumental artifacts, stellar activity, and/or perturbations from unseen bodies. Regarding the latter, we find seven KOIs exhibiting >5 σ evidence of transit timing variations, including the “mega-Earth” Kepler-10c, likely indicating an additional planet in that system. We exploit the moderately large sample of 57 unique KOIs surveyed to date to infer several useful statistics. For example, although there is a diverse range in sensitivities, we find that we are sensitive to Pluto–Charon mass-ratio systems for ;40% of KOIs studied and Earth–Moon mass-ratios for 1 in 8 cases. In terms of absolute mass, our limits probe down to 1.7 Ganymede masses, with a sensitivity to Earth-mass moons for 1 in 3 cases studied and to the smallest moons capable of sustaining an Earth-like atmosphere (0.3 M⊕) for 1 in 4. Despite the lack of positive detections to date, we caution against drawing conclusions yet, since our most interesting objects remain under analysis. Finally, we point out that had we searched for the photometric transit signals of exomoons alone, rather than using photodynamics, we estimate that 1 in 4 KOIs would have erroneously been concluded to harbor exomoons due to residual time correlated noise in the Kepler data, posing a serious problem for alternative methods.en_US
dc.language.isoen_USen_US
dc.relation.ispartofAstrophysical Journalen_US
dc.rightsFinal published version. Article is made available in OAR by the publisher's permission or policy.en_US
dc.titleThe Hunt for Exomoons with Kepler (HEK): V. A Survey of 41 Planetary Candidates for Exomoonsen_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.1088/0004-637X/813/1/14-
dc.date.eissued2015-10-22en_US
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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