Kepler-1629b , the SIMBAD biblio

Kepler-1629b , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST05:34:15

Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
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.
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.
2019RAA....19...41G viz 16       D               1 1982 17 Transit timing variations and linear ephemerides of confirmed Kepler transiting exoplanets. GAJDOS P., VANKO M. and PARIMUCHA S.
2019MNRAS.485.3999M viz 16       D               1 474 ~ Planetary magnetism as a parameter in exoplanet habitability. McINTYRE S.R.N., LINEWEAVER C.H. and IRELAND M.J.
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.
2022A&A...662A..15M viz 17       D               1 733 3 Tidally driven tectonic activity as a parameter in exoplanet habitability. McINTYRE S.R.N.
2023MNRAS.519.6210M viz 17       D               1 688 1 A rocky exoplanet classification method and its application to calculating surface pressure and surface temperature. McINTYRE S.R.N., KING P.L. and MILLS F.P.
2023ApJ...946...61L viz 17       D               1 257 ~ A Spectroscopic Analysis of a Sample of K2 Planet-host Stars: Stellar Parameters, Metallicities and Planetary Radii. LOAIZA-TACURI V., CUNHA K., SMITH V.V., et al.
2024ApJ...976..234B 45           X         1 57 ~ Ages of Stars and Planets in the Kepler Field Younger than Four Billion Years. BOUMA L.G., HILLENBRAND L.A., HOWARD A.W., et al.

goto View the references in ADS