KOI-7546 , the SIMBAD biblio

KOI-7546 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST01:54:07


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Bibcode/DOI Score in Title|Abstract|
Keywords
in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
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Title First 3 Authors
2013MNRAS.431.2240B viz 15       D               1 899 128 Activity in A-type stars. BALONA L.A.
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.
2018AJ....155..161Z viz 16       D               2 1274 24 Robo-AO Kepler survey. IV. The effect of nearby stars on 3857 planetary candidate systems. ZIEGLER C., LAW N.M., BARANEC C., et al.
2018AJ....156...83Z viz 16       D               1 337 14 Robo-AO Kepler Survey. V. The effect of physically associated stellar companions on planetary systems. ZIEGLER C., LAW N.M., BARANEC C., 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.
2018ApJ...866...99B viz 16       D               1 7129 233 Revised radii of Kepler stars and planet's using Gaia Data Release 2. BERGER T.A., HUBER D., GAIDOS E., et al.
2019MNRAS.485.2380M viz 16       D               1 14330 108 Gaia-derived luminosities of Kepler A/F stars and the pulsator fraction across the δ Scuti instability strip. MURPHY S.J., HEY D., VAN REETH T., et al.
2020ApJ...890...23L viz 16       D               1 4936 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 16       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.
2021AJ....162..204H 17       D               2 46 5 A search for transits among the delta Scuti variables in Kepler. HEY D.R., MONTET B.T., POPE B.J.S., et al.

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