Kepler-1312c , the SIMBAD biblio

Kepler-1312c , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:23:41

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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
2014ApJS..210...19B viz 15       D               1 5860 211 Planetary candidates observed by Kepler IV: planet sample from Q1-Q8 (22 months). BURKE C.J., BRYSON S.T., MULLALLY F., et al.
2014ApJ...783....4W viz 15       D               1 487 103 Influence of stellar multiplicity on planet formation. I. Evidence of suppressed planet formation due to stellar companions within 20 AU and validation of four planets from the Kepler multiple planet candidates. WANG J., XIE J.-W., BARCLAY T., et al.
2015ApJS..217...16R viz 16       D               1 8625 149 Planetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months). ROWE J.F., COUGHLIN J.L., ANTOCI V., et al.
2016AJ....152..158T viz 16       D               1 4388 37 Detection of potential transit signals in 17 quarters of Kepler data: results of the final Kepler mission transiting planet search (DR25). TWICKEN J.D., JENKINS J.M., SEADER S.E., et al.
2017AJ....154..108J viz 16       D               1 3237 137 The California-Kepler Survey. II. Precise physical properties of 2025 Kepler planets and their host stars. JOHNSON J.A., PETIGURA E.A., FULTON B.J., et al.
2017AJ....154..109F viz 16       D               1 900 847 The California-Kepler Survey. III. A gap in the radius distribution of small planets. FULTON B.J., PETIGURA E.A., HOWARD A.W., et al.
2018AJ....155...48W viz 16       D               1 911 204 The California-Kepler survey. V. Peas in a pod: planets in a Kepler multi-planet system are similar in size and regularly spaced. WEISS L.M., MARCY G.W., PETIGURA E.A., et al.
2018AJ....155...68W viz 16       D               1 509 18 Elemental abundances of Kepler Objects of Interest in APOGEE. I. Two distinct orbital period regimes inferred from host star iron abundances. WILSON R.F., TESKE J., MAJEWSKI S.R., 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.
2018AJ....156..254W viz 16       D               2 1269 42 The California-Kepler Survey. VI. Kepler multis and singles have similar planet and stellar properties indicating a common origin. WEISS L.M., ISAACSON H.T., MARCY G.W., et al.
2018AJ....156..264F viz 16       D               1 1909 365 The California-Kepler Survey. VII. Precise planet radii leveraging Gaia DR2 reveal the stellar mass dependence of the Planet radius gap. FULTON B.J. and PETIGURA E.A.
2019ApJ...875...29M viz 16       D               1 2918 72 A spectroscopic analysis of the California-Kepler Survey sample. I. Stellar parameters, planetary radii, and a slope in the radius gap. MARTINEZ C.F., CUNHA K., GHEZZI L., et al.
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.
2022MNRAS.510.3449B viz 17       D               1 508 7 Exoplanets in the Galactic context: planet occurrence rates in the thin disc, thick disc, and stellar halo of Kepler stars. BASHI D. and ZUCKER S.
2022AJ....163..179P viz 17       D               1 2962 39 The California-Kepler Survey. X. The Radius Gap as a Function of Stellar Mass, Metallicity, and Age. PETIGURA E.A., ROGERS J.G., ISAACSON H., et al.
2022ApJ...926..120V 17       D               1 645 13 ExoMiner: A Highly Accurate and Explainable Deep Learning Classifier That Validates 301 New Exoplanets. VALIZADEGAN H., MARTINHO M.J.S., WILKENS L.S., et al.
2022A&A...662A..15M viz 17       D               2 733 3 Tidally driven tectonic activity as a parameter in exoplanet habitability. McINTYRE S.R.N.
2023MNRAS.519.6210M viz 17       D               2 688 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.
2024ApJ...976..234B 90           X         2 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.

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