Kepler-100d , the SIMBAD biblio

Kepler-100d , the SIMBAD biblio (50 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:19:33

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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
2012Natur.486..375B viz 15       D               1 378 520 An abundance of small exoplanets around stars with a wide range of metallicities. BUCHHAVE L.A., LATHAM D.W., JOHANSEN A., et al.
2012ApJ...756..185F viz 15       D               1 1856 44 Transit timing observations from Kepler. V. Transit timing variation candidates in the first sixteen months from polynomial models. FORD E.B., RAGOZZINE D., ROWE J.F., et al.
2011PASP..123..412W viz 15       D               1 2897 398 The Exoplanet Orbit Database. WRIGHT J.T., KAKHOURI O., MARCY G.W., et al.
2013ApJS..204...24B viz 15       D               2 3274 922 Planetary candidates observed by Kepler. III. Analysis of the first 16 months of data. BATALHA N.M., ROWE J.F., BRYSON S.T., et al.
2013ApJ...767..127H viz 15       D               1 189 246 Fundamental properties of Kepler planet-candidate host stars using asteroseismology. HUBER D., CHAPLIN W.J., CHRISTENSEN-DALSGAARD J., et al.
2013ApJ...770...69P viz 15       D               1 245 238 A plateau in the planet population below twice the size of Earth. PETIGURA E.A., MARCY G.W. and HOWARD A.W.
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.
2014ApJS..210...20M viz 95       D       C       3 94 394 Masses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planets. MARCY G.W., ISAACSON H., HOWARD A.W., et al.
2014ApJ...783L...6W 96       D       C       2 66 499 The mass-radius relation for 65 exoplanets smaller than 4 earth radii. WEISS L.M. and MARCY G.W.
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               2 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.
2014A&A...566A.103L viz 15       D               3 359 102 High-resolution imaging of Kepler planet host candidates. A comprehensive comparison of different techniques. LILLO-BOX J., BARRADO D. and BOUY H.
2014ApJ...790..146F viz 15       D               1 918 579 Architecture of Kepler's multi-transiting systems. II. New investigations with twice as many candidates. FABRYCKY D.C., LISSAUER J.J., RAGOZZINE D., et al.
2014AJ....148..108B 15       D               1 129 5 A technique to derive improved proper motions for Kepler Objects of Interest. BENEDICT G.F., TANNER A.M., CARGILE P.A., 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.
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.
2015ApJ...815....5S viz 39           X         1 31 18 Detailed abundances of stars with small planets discovered by Kepler. I. The first sample. SCHULER S.C., VAZ Z.A., KATIME SANTRICH O.J., et al.
2016MNRAS.456..119C 16       D               2 51 42 Rotation periods and seismic ages of KOIs - comparison with stars without detected planets from Kepler observations. CEILLIER T., VAN SADERS J., GARCIA R.A., et al.
2016ApJ...825...19W viz 17       D               1 99 221 Probabilistic mass-radius relationship for sub-Neptune-sized planets. WOLFGANG A., ROGERS L.A. and FORD E.B.
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...66F 16       D               2 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.
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.
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               2 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.
2018AJ....156..292T viz 40           X         1 647 8 The effects of stellar companions on the observed transiting exoplanet radius distribution. TESKE J.K., CIARDI D.R., HOWELL S.B., 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.
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.
2019A&A...624A..71W 41           X         1 69 2 Comparative analysis of the influence of Sgr A* and nearby active galactic nuclei on the mass loss of known exoplanets. WISLOCKA A.M., KOVACEVIC A.B. and BALBI A.
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.
2019MNRAS.490.1509K 16       D               1 54 ~ Asteroseismic investigation of 20 planet and planet-candidate host stars. KAYHAN C., YILDIZ M. and CELIK ORHAN Z.
2020MNRAS.491.5287O viz 305       D     X C       7 127 43 Testing exoplanet evaporation with multitransiting systems. OWEN J.E. and CAMPOS ESTRADA B.
2020AJ....159..239G viz 16       D               1 1408 ~ Updated parameters and a new transmission spectrum of HD 97658b. GUO X., CROSSFIELD I.J.M., DRAGOMIR D., et al.
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.
2022AJ....163...91J viz 230       D     X         6 504 ~ Physical properties and impact parameter variations of Kepler planets from analytic light-curve modeling. JUDKOVSKY Y., OFIR A. and AHARONSON O.
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..139S 17       D               1 25 ~ Mass Upper Bounds for Over 50 Kepler Planets Using Low-S/N Transit Timing Variations. SIEGEL J.C. and ROGERS L.A.
2022ApJ...941..175L 43           X         1 99 2 Meta-analysis of Photometric and Asteroseismic Measurements of Stellar Rotation Periods: The Lomb-Scargle Periodogram, Autocorrelation Function, and Wavelet and Rotational Splitting Analysis for 92 Kepler Asteroseismic Targets. LU Y., BENOMAR O., KAMIAKA S., 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.
2024ApJS..270....8W viz 18       D               2 250 ~ The Kepler Giant Planet Search. I. A Decade of Kepler Planet-host Radial Velocities from W. M. Keck Observatory. WEISS L.M., ISAACSON H., HOWARD A.W., 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.
2024AJ....168..115B viz 18       D               1 224 ~ Different Planetary Eccentricity-period (PEP) Distributions of Small and Giant Planets. BASHI D., MAZEH T. and FAIGLER S.
2024A&A...692A.238L viz 18       D               1 39 ~ Characterisation of TOI-406 as a showcase of the THIRSTEE program A two-planet system straddling the M-dwarf density gap. LACEDELLI G., PALLE E., LUQUE R., et al.
2025AJ....170..109B 47           X         1 26 ~ The Compositions of Rocky Planets in Close-in Orbits Tend to Be Earth-like. BRINKMAN C.L., WEISS L.M., HUBER D., et al.

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