KOI-5942 , the SIMBAD biblio

KOI-5942 , the SIMBAD biblio (16 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST13:35:10


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Title First 3 Authors
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.
2015ApJS..217...31M viz 16       D               1 2033 213 Planetary candidates observed by Kepler. VI. Planet sample from Q1–Q16 (47 months). MULLALLY F., COUGHLIN J.L., THOMPSON S.E., et al.
2015ApJ...807..170H viz 16       D               1 2117 10 Time variation of Kepler transits induced by stellar Spots–A way to distinguish between prograde and retrograde motion. II. Application to KOIs. HOLCZER T., SHPORER A., MAZEH T., et al.
2016A&A...588A..87V viz 16       D               1 6115 133 Period spacings in red giants. II. Automated measurement. VRARD M., MOSSER B. and SAMADI R.
2016AJ....152....6W viz 16       D               1 3060 13 Calibration of LAMOST stellar surface gravities using the Kepler asteroseismic data. WANG L., WANG W., WU Y., et al.
2016ApJS..225....9H viz 16       D               2 2132 124 Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set. HOLCZER T., MAZEH T., NACHMANI G., et al.
2016A&A...594A..39F viz 16       D               2 51408 86 Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra. FRASCA A., MOLENDA-ZAKOWICZ J., DE CAT P., et al.
2017A&A...600A...1M viz 16       D               1 5166 19 Period spacings in red giants. III. Coupling factors of mixed modes. MOSSER B., PINCON C., BELKACEM K., 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.
2018MNRAS.475.3633W viz 16       D               1 3727 38 Mass and age of red giant branch stars observed with LAMOST and Kepler. WU Y., XIANG M., BI S., et al.
2018MNRAS.476.3233H viz 16       D               1 15009 17 Deep learning classification in asteroseismology using an improved neural network: results on 15 000 Kepler red giants and applications to K2 and TESS data. HON M., STELLO D. and YU J.
2018ApJS..236...42Y viz 16       D               1 16097 158 Asteroseismology of 16,000 Kepler red giants: global oscillation parameters, masses, and radii. YU J., HUBER D., BEDDING T.R., et al.
2018A&A...616A..24G viz 16       D               1 1140 108 Core rotation braking on the red giant branch for various mass ranges. GEHAN C., MOSSER B., MICHEL E., 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.
2020AJ....160..108B viz 17       D               1 6855 109 The Gaia-Kepler stellar properties catalog. II. Planet radius demographics as a function of stellar mass and age. BERGER T.A., HUBER D., GAIDOS E., et al.
2021A&A...645A.124G viz 17       D               2 1202 13 Automated approach to measure stellar inclinations: validation through large-scale measurements on the red giant branch. GEHAN C., MOSSER B., MICHEL E., et al.

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