KOI-4563 , the SIMBAD biblio

KOI-4563 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.7 - 2021.01.18CET04:52:02


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Bibcode/DOI Score in Title|Abstract|
Keywords
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Title First 3 Authors
2019AJ....157..143B viz 18       D               1 423 ~ Re-evaluating small long-period confirmed planets from Kepler. BURKE C.J., MULLALLY F., THOMPSON S.E., et al.
2018ApJ...861..149F viz 17       D               1 2261 ~ The Kepler Follow-up Observation Program. II. Stellar parameters from medium- and high-resolution spectroscopy. FURLAN E., CIARDI D.R., COCHRAN W.D., et al.
2018ApJ...866...99B viz 17       D               1 7129 101 Revised radii of Kepler stars and planet's using Gaia Data Release 2. BERGER T.A., HUBER D., GAIDOS E., et al.
2017AJ....153...71F viz 17       D               1 3575 46 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.
2016ApJ...822...86M viz 17       D               1 6129 192 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.
2015ApJ...801....3M viz 16       D               1 3357 52 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.
2015ApJ...809....8B viz 16       D               1 112329 139 Terrestrial planet occurrence rates for the Kepler GK dwarf sample. BURKE C.J., CHRISTIANSEN J.L., MULLALLY F., et al.
2015ApJ...814..130M viz 16       D               1 2846 46 An increase in the mass of planetary systems around lower-mass stars. MULDERS G.D., PASCUCCI I. and APAI D.
2015ApJS..217...16R viz 16       D               1 8625 84 Planetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months). ROWE J.F., COUGHLIN J.L., ANTOCI V., et al.
2014AJ....147..119C viz 16       D               1 8005 55 Contamination in the Kepler field. Identification of 685 KOIs as false positives via ephemeris matching based on Q1-Q12 data. COUGHLIN J.L., THOMPSON S.E., BRYSON S.T., et al.

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2021.01.18-04:52:02

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