KOI-5486 , the SIMBAD biblio

KOI-5486 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.05.12CEST04:37:21


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Title First 3 Authors
2010AstL...36..338F viz 15       D               1 1150 6 Proper motions and CCD photometry of stars in the region of the open cluster NGC 6866. FROLOV V.N., ANANJEVSKAJA Y.K., GORSHANOV D.L., et al.
2011AJ....142..160S viz 15       D               1 2325 365 Kepler eclipsing binary stars. II. 2165 eclipsing binaries in the second data release. SLAWSON R.W., PRSA A., WELSH W.F., et al.
2012ApJS..199...24T viz 15       D               1 5394 66 Detection of potential transit signals in the first three quarters of Kepler mission data. TENENBAUM P., CHRISTIANSEN J.L., JENKINS J.M., et al.
2013A&A...557L..10N viz 16       D               1 12151 189 Rotation periods of 12000 main-sequence Kepler stars: dependence on stellar spectral type and comparison with v sin i observations. NIELSEN M.B., GIZON L., SCHUNKER H., et al.
2013A&A...560A...4R viz 16       D               1 24132 291 Rotation and differential rotation of active Kepler stars. REINHOLD T., REINERS A. and BASRI G.
2015ApJ...801....3M viz 16       D               1 3357 109 Photometric amplitude distribution of stellar rotation of KOIs–Indication for spin-orbit alignment of cool stars and high obliquity for hot stars. MAZEH T., PERETS H.B., McQUILLAN A., et al.
2015MNRAS.453.1095B viz 16       D               1 739 12 A comprehensive study of the open cluster NGC 6866. BOSTANCI Z.F., AK T., YONTAN T., et al.
2015ApJ...814..130M viz 16       D               1 2846 162 An increase in the mass of planetary systems around lower-mass stars. MULDERS G.D., PASCUCCI I. and APAI D.
2016AJ....151...68K viz 16       D               1 2914 316 Kepler eclipsing binary stars. VII. The catalog of eclipsing binaries found in the entire Kepler data set. KIRK B., CONROY K., PRSA A., et al.
2016ApJ...822...86M viz 16       D               1 6130 337 False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives. MORTON T.D., BRYSON S.T., COUGHLIN J.L., et al.
2017AJ....153...66Z viz 16       D               3 1663 45 Robo-AO Kepler Planetary Candidate Survey. III. Adaptive optics imaging of 1629 Kepler exoplanet candidate host stars. ZIEGLER C., LAW N.M., MORTON T., et al.
2017AJ....153...71F viz 16       D               1 3575 164 The Kepler follow-up observation program. I. A catalog of companions to Kepler stars from high-resolution imaging. FURLAN E., CIARDI D.R., EVERETT M.E., et al.
2017MNRAS.465.2634A viz 16       D               1 5400 21 Transit shapes and self-organizing maps as a tool for ranking planetary candidates: application to Kepler and K2. ARMSTRONG D.J., POLLACCO D. and SANTERNE A.
2017AJ....154..250L viz 16       D               1 2280 72 Tidal synchronization and differential rotation of Kepler eclipsing binaries. LURIE J.C., VYHMEISTER K., HAWLEY S.L., et al.
2018MNRAS.479..183B viz 16       D               1 2598 17 Gaia luminosities of pulsating A-F stars in the Kepler field. BALONA L.A.
2020MNRAS.491.3586L viz 17       D               1 609 75 Gravity-mode period spacings and near-core rotation rates of 611 γ Doradus stars with Kepler. LI G., VAN REETH T., BEDDING T.R., et al.
2020ApJ...890...23L viz 17       D               1 4935 35 Current population statistics do not favor photoevaporation over core-powered mass loss as the dominant cause of the exoplanet radius gap. LOYD R.O.P., SHKOLNIK E.L., SCHNEIDER A.C., et al.
2020MNRAS.497.4363L 230       D     X C F     4 37 23 The effect of tides on near-core rotation: analysis of 35 Kepler γ Doradus stars in eclipsing and spectroscopic binaries. LI G., GUO Z., FULLER J., et al.
2020ApJ...902..107L viz 17       D               1 106 ~ Assessing spectroscopic binary multiplicity properties using Robo-AO imaging. LAOS S., STASSUN K.G. and MATHIEU R.D.
2023A&A...671A.121V 47           X         1 12 ~ Tidally perturbed gravity-mode pulsations in a sample of close eclipsing binaries. VAN REETH T., JOHNSTON C., SOUTHWORTH J., et al.

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