Transit timing observations from Kepler – III . Confirmation of four multiple planet systems by a Fourier - domain study of anticorrelated transit timing variations

نویسندگان

  • Jason H. Steffen
  • Daniel C. Fabrycky
  • Eric B. Ford
  • Joshua A. Carter
  • Jean-Michel Désert
  • Francois Fressin
  • Matthew J. Holman
  • Jack J. Lissauer
  • Althea V. Moorhead
  • Jason F. Rowe
  • Darin Ragozzine
  • William F. Welsh
  • Natalie M. Batalha
  • William J. Borucki
  • Lars A. Buchhave
  • Steve Bryson
  • Douglas A. Caldwell
  • David Charbonneau
  • David R. Ciardi
  • William D. Cochran
  • Michael Endl
  • Mark E. Everett
  • Thomas N. Gautier
  • Ron L. Gilliland
  • Forrest R. Girouard
  • Jon M. Jenkins
  • Elliott Horch
  • Steve B. Howell
  • Howard Isaacson
  • Todd C. Klaus
  • David G. Koch
  • David W. Latham
  • Jie Li
  • Philip Lucas
  • Phillip J. MacQueen
  • Geoffrey W. Marcy
  • Sean McCauliff
  • Christopher K. Middour
  • Robert L. Morris
  • Fergal R. Mullally
  • Samuel N. Quinn
  • Elisa V. Quintana
  • Avi Shporer
  • Martin Still
  • Peter Tenenbaum
  • Susan E. Thompson
  • Joseph D. Twicken
  • Jeffery Van Cleve
چکیده

We present a method to confirm the planetary nature of objects in systems with multiple transiting exoplanet candidates. This method involves a Fourier-domain analysis of the E-mail: [email protected] †Hubble Fellow. C © 2012 Fermi Research Alliance LLC, Contractor for the U.S. Dept of Energy Monthly Notices of the Royal Astronomical Society C © 2012 RAS Kepler planetary systems 25–28 2343 deviations in the transit times from a constant period that result from dynamical interactions within the system. The combination of observed anticorrelations in the transit times and mass constraints from dynamical stability allow us to claim the discovery of four planetary systems, Kepler-25, Kepler-26, Kepler-27 and Kepler-28, containing eight planets and one additional planet candidate.

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تاریخ انتشار 2012