SIMBAD references

2012MNRAS.421.2342S - Mon. Not. R. Astron. Soc., 421, 2342-2354 (2012/April-2)

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

STEFFEN J.H., FABRYCKY D.C., FORD E.B., CARTER J.A., DESERT J.-M., FRESSIN F., HOLMAN M.J., LISSAUER J.J., MOORHEAD A.V., ROWE J.F., RAGOZZINE D., WELSH W.F., BATALHA N.M., BORUCKI W.J., BUCHHAVE L.A., BRYSON S., CALDWELL D.A., CHARBONNEAU D., CIARDI D.R., COCHRAN W.D., ENDL M., EVERETT M.E., GAUTIER III T.N., GILLILAND R.L., GIROUARD F.R., JENKINS J.M., HORCH E., HOWELL S.B., ISAACSON H., KLAUS T.C., KOCH D.G., LATHAM D.W., LI J., LUCAS P., MacQUEEN P.J., MARCY G.W., McCAULIFF S., MIDDOUR C.K., MORRIS R.L., MULLALLY F.R., QUINN S.N., QUINTANA E.V., SHPORER A., STILL M., TENENBAUM P., THOMPSON S.E., TWICKEN J.D. and VAN CLEVE J.

Abstract (from CDS):

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 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. CFHTLenS: improving the quality of photometric redshifts with precision photometry

Abstract Copyright: 2012 Fermi Research Alliance LLC, Contractor for the U.S. Dept of Energy Monthly Notices of the Royal Astronomical Society2012 RAS

Journal keyword(s): methods: data analysis - celestial mechanics - stars: individual: KIC 4349452 - stars: individual: KIC 9757613 - stars: individual: KIC 5792202 - stars: individual: KIC 6949607

VizieR on-line data: <Available at CDS (J/MNRAS/421/2342): table2.dat table3.dat tablea1.dat table1.dat>

CDS comments: KOI-168.02 and KOI-250.03, planet candidates, are not in Simbad.

Simbad objects: 23

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