Kepler-396b , the SIMBAD biblio

Kepler-396b , the SIMBAD biblio (40 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST05:23:35

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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
2013ApJ...778..110M 576       S   X C       13 23 0 Eight planets in four multi-planet systems via transit timing variations in 1350 days. MING Y., LIU H.-G., HUI Z., et al.
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.
2014ApJ...784...45R viz 15       D               1 1691 388 Validation of Kepler's multiple planet candidates. III. Light curve analysis and announcement of hundreds of new multi-planet systems. ROWE J.F., BRYSON S.T., MARCY G.W., et al.
2015ApJ...798...66D 39           X         1 296 60 The photoeccentric effect and proto-hot jupiters. III. A paucity of proto-hot jupiters on super-eccentric orbits. DAWSON R.I., MURRAY-CLAY R.A. and JOHNSON J.A.
2015ApJ...799..180S viz 16       D               1 431 118 A statistical reconstruction of the planet population around Kepler solar-type stars. SILBURT A., GAIDOS E. and WU Y.
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.
2015ApJS..217...31M viz 16       D               1 2033 213 Planetary candidates observed by Kepler. VI. Planet sample from Q1–Q16 (47 months). MULLALLY F., COUGHLIN J.L., THOMPSON S.E., et al.
2015ApJ...809....8B viz 16       D               1 112329 282 Terrestrial planet occurrence rates for the Kepler GK dwarf sample. BURKE C.J., CHRISTIANSEN J.L., MULLALLY F., et al.
2015MNRAS.453.4089S 16       D               1 103 3 Tides alone cannot explain Kepler planets close to 2:1 MMR. SILBURT A. and REIN H.
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....5H viz 95       D     X         3 231 145 Kepler planet masses and eccentricities from TTV analysis. HADDEN S. and LITHWICK Y.
2017AJ....154...66F 214       D     X         6 90 6 The densities of planets in multiple stellar systems. FURLAN E. and HOWELL S.B.
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.
2017A&A...603A..30S viz 16       D               4 2500 58 Observational evidence for two distinct giant planet populations. SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., 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.
2018A&A...615A..79V viz 83 9 Kepler Object of Interest Network. I. First results combining ground- and space-based observations of Kepler systems with transit timing variations. VON ESSEN C., OFIR A., DREIZLER 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.
2019ApJ...874L..31T viz 16       D               1 403 62 Connecting giant planet atmosphere and interior modeling: constraints on atmospheric metal enrichment. THORNGREN D. and FORTNEY J.J.
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.
2019AJ....157..171K viz 16       D               1 4069 2 Visual analysis and demographics of Kepler transit timing variations. KANE M., RAGOZZINE D., FLOWERS X., et al.
2019AJ....157..174O viz 16       D               1 176 61 Discovery of a third transiting planet in the Kepler-47 circumbinary system. OROSZ J.A., WELSH W.F., HAGHIGHIPOUR N., et al.
2019AJ....157..235C viz 16       D               2 415 7 Observations of the Kepler field with TESS: predictions for planet yield and observable features. CHRIST C.N., MONTET B.T. and FABRYCKY D.C.
2020AJ....159...41T viz 16       D               1 564 ~ Estimating planetary mass with deep learning. TASKER E.J., LANEUVILLE M. and GUTTENBERG N.
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.
2021MNRAS.503.4092B 309       D     X C       7 124 ~ Revisiting the Kepler field with TESS: Improved ephemerides using TESS 2 min data. BATTLEY M.P., KUNIMOTO M., ARMSTRONG D.J., et al.
2021MNRAS.505.1293S viz 17       D               1 573 7 Systematic search for long-term transit duration changes in Kepler transiting planets. SHAHAF S., MAZEH T., ZUCKER S., et al.
2022AJ....163...91J viz 17       D               2 504 ~ Physical properties and impact parameter variations of Kepler planets from analytic light-curve modeling. JUDKOVSKY Y., OFIR A. and AHARONSON O.
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..128W viz 17       D               1 1570 6 The influence of 10 unique chemical elements in shaping the distribution of Kepler planets. WILSON R.F., CANAS C.I., MAJEWSKI S.R., et al.
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.
2022AJ....164...42J 1039       D     X C       24 79 3 TESS Observations of Kepler Systems with Transit Timing Variations. JONTOF-HUTTER D., DALBA P.A. and LIVINGSTON J.H.
2022ApJS..261...26S viz 17       D               7 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.
2023AJ....165..125A viz 17       D               1 578 ~ Planetary Orbit Eccentricity Trends (POET). I. The Eccentricity-Metallicity Trend for Small Planets Revealed by the LAMOST-Gaia-Kepler Sample. AN D.-S., XIE J.-W., DAI Y.-Z., et al.
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.
2024AJ....167...20Z viz 18       D               1 230 ~ The Breakthrough Listen Search for Intelligent Life: Detection and Characterization of Anomalous Transits in Kepler Lightcurves. ZUCKERMAN A., DAVENPORT J.R.A., CROFT S., et al.
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.

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