Kepler-450d , the SIMBAD biblio

Kepler-450d , the SIMBAD biblio (25 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST11:37:20

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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
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.
2015ApJ...808..126V 94       D     X         3 105 201 Eccentricity from transit photometry: small planets in Kepler multi-planet systems have low eccentricities. VAN EYLEN V. and ALBRECHT S.
2016AJ....152..143V 39           X         1 20 32 The K2-ESPRINT project V: a short-period giant planet orbiting a subgiant star. VAN EYLEN V., ALBRECHT S., GANDOLFI D., 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.
2017AJ....154..236W 16       D               1 34 7 Near mean-motion resonances in the system observed by Kepler: affected by mass accretion and Type I migration. WANG S. and JI J.
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.
2018ApJ...864L..38D 16       D               2 109 49 Larger mutual inclinations for the shortest-period planets. DAI F., MASUDA K. and WINN J.N.
2018MNRAS.479.4786V 18       D               1 117 318 An asteroseismic view of the radius valley: stripped cores, not born rocky. VAN EYLEN V., AGENTOFT C., LUNDKVIST M.S., 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.
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.
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.
2020MNRAS.491.5287O viz 16       D               1 127 43 Testing exoplanet evaporation with multitransiting systems. OWEN J.E. and CAMPOS ESTRADA B.
2021ApJ...908..114Y 184       D     X C       4 16 9 A simplified photodynamical model for planetary mass determination in low-eccentricity multitransiting systems. YOFFE G., OFIR A. and AHARONSON O.
2022AJ....163...91J viz 102       D     X         3 504 ~ Physical properties and impact parameter variations of Kepler planets from analytic light-curve modeling. JUDKOVSKY Y., OFIR A. and AHARONSON O.
2022A&A...662A..15M viz 17       D               1 733 3 Tidally driven tectonic activity as a parameter in exoplanet habitability. McINTYRE S.R.N.
2022ApJS..261...26S viz 17       D               4 1893 2 Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys. SU T., ZHANG L.-Y., LONG L., et al.
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.
2024A&A...685A.143M viz 18       D               1 535 ~ Planets similar in size are often dissimilar in interior. MAMONOVA E., SHAN Y., HATALOVA P., et al.
2025AJ....169...90O viz 19       D               1 194 ~ Planetary Mass Determinations from a Simplified Photodynamical Model-Application to the Complete Kepler Dataset. OFIR A., YOFFE G. and AHARONSON O.
2025ApJ...981..142X 19       D               1 94 ~ Amplifying Resonant Repulsion with Inflated Young Planets, Overlooked Inner Planets, and Nonzero Initial Δ. XU Y. and DAI F.

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