Kepler-105c , the SIMBAD biblio

Kepler-105c , the SIMBAD biblio (53 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST09:39:11


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Title First 3 Authors
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               1 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...771..107E viz 15       D               1 756 47 Spectroscopy of faint Kepler mission exoplanet candidate host stars. EVERETT M.E., HOWELL S.B., SILVA D.R., 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.
2014ApJ...787...80H viz 15       D               2 261 190 Densities and eccentricities of 139 Kepler planets from transit time variations. HADDEN S. and LITHWICK Y.
2014A&A...566A.103L viz 15       D               2 359 102 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.
2015AJ....149...55E 16       D               3 48 34 High-resolution multi-band imaging for validation and characterization of small Kepler planets. EVERETT M.E., BARCLAY T., CIARDI D.R., 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.
2016ApJ...820...39J 472     A D     X C       12 107 126 Secure mass measurements from transit timing: 10 Kepler exoplanets between 3 and 8 M⊕ with diverse densities and incident fluxes. JONTOF-HUTTER D., FORD E.B., ROWE J.F., 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.
2016AJ....152..204L viz 80               F     1 23 84 Kepler-21b: a rocky planet around a V = 8.25 magnitude star. LOPEZ-MORALES M., HAYWOOD R.D., COUGHLIN J.L., et al.
2017ApJ...834...17C viz 16       D               1 290 454 Probabilistic forecasting of the masses and radii of other worlds. CHEN J. and KIPPING D.
2017AJ....153..191S viz 79               F     1 41 23 Detection of the atmosphere of the 1.6 M⊕ exoplanet GJ 1132 b. SOUTHWORTH J., MANCINI L., MADHUSUDHAN N., et al.
2017MNRAS.466.1868C viz 16       D               1 176 21 An overabundance of low-density Neptune-like planets. CUBILLOS P., ERKAEV N.V., JUVAN I., et al.
2017AJ....154....5H viz 16       D               1 231 145 Kepler planet masses and eccentricities from TTV analysis. HADDEN S. and LITHWICK Y.
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.
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.
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.
2019ApJ...880L...1A viz 16       D               1 146 ~ A gap in the mass distribution for warm Neptune and terrestrial planets. ARMSTRONG D.J., MERU F., BAYLISS D., et al.
2020AJ....159...41T viz 16       D               1 564 ~ Estimating planetary mass with deep learning. TASKER E.J., LANEUVILLE M. and GUTTENBERG N.
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.
2020PASP..132h4402Q 16       D               2 63 ~ Forecasting rates of volcanic activity on terrestrial exoplanets and implications for cryovolcanic activity on extrasolar ocean worlds. QUICK L.C., ROBERGE A., MLINAR A.B., 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.
2020MNRAS.499..932P 222       D     X   F     5 40 35 Chemical fingerprints of formation in rocky super-Earths' data. PLOTNYKOV M. and VALENCIA D.
2021AJ....161..246J viz 476       D     X         12 204 12 Following up the Kepler field: masses of targets for transit timing and atmospheric characterization. JONTOF-HUTTER D., WOLFGANG A., FORD E.B., et al.
2021AJ....162...55Y viz 17       D               1 70 13 How close are compact multiplanet systems to the stability limit? YEE S.W., TAMAYO D., HADDEN S., et al.
2021ApJ...921...24S viz 17       D               1 328 1 The occurrence-weighted median planets discovered by transit surveys orbiting solar-type stars and their implications for planet formation and evolution. SCHLAUFMAN K.C. and HALPERN N.D.
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...930L...6U 60       D     X         2 19 4 Mantle Degassing Lifetimes through Galactic Time and the Maximum Age Stagnant-lid Rocky Exoplanets Can Support Temperate Climates. UNTERBORN C.T., FOLEY B.J., DESCH S.J., et al.
2022ApJ...940..144S 128           X         3 5 ~ Rocky Histories: The Effect of High Excitations on the Formation of Rocky Planets. SCORA J., VALENCIA D., MORBIDELLI A., et al.
2023ApJ...944...42U 148       D     X         4 56 6 The Nominal Ranges of Rocky Planet Masses, Radii, Surface Gravities, and Bulk Densities. UNTERBORN C.T., DESCH S.J., HALDEMANN J., 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.
2023A&A...674A.137L 104       D     X         3 122 ~ Quantitative correlation of refractory elemental abundances between rocky exoplanets and their host stars. LIU Z. and NI D.
2024AJ....167...84H viz 3342     A S   X C F     72 5 ~ Investigating the Atmospheric Mass Loss of the Kepler-105 Planets Straddling the Radius Gap. HOUSEHOLDER A., WEISS L.M., OWEN J.E., et al.
2024ApJ...966..185C 18       D               1 140 ~ Where Are the Water Worlds? Identifying Exo-water-worlds Using Models of Planet Formation and Atmospheric Evolution. CHAKRABARTY A. and MULDERS G.D.
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 112       D     X         3 194 ~ Planetary Mass Determinations from a Simplified Photodynamical Model-Application to the Complete Kepler Dataset. OFIR A., YOFFE G. and AHARONSON O.
2025ApJ...978L..41L 19       D               1 13 ~ Most High-density Exoplanets Are Unlikely to Be Remnant Giant Planet's Cores. LIN Z., CAMBIONI S. and SEAGER S.
2025AJ....169..216T viz 47           X         1 10 ~ Utilizing Machine Learning to Predict Host Stars and the Key Elemental Abundances of Small Planets. TORRES-QUIJANO A.R., HINKEL N.R., WHEELER III C.H., et al.
2025A&A...696A.174C 252       D     X   F     5 17 ~ Can metal-rich worlds form by giant impacts? CAMBIONI S., WEISS B.P., ASPHAUG E., et al.
2025ApJ...993..235R 1521     A     X C       32 60 ~ Terrestrial Exoplanet Internal Structure Constraints Enabled by Comprehensive Host Star Characterization Reveal That Terrestrial Planets in Mean Motion Resonances Are Water Rich. ROSS A., REGGIANI H., SCHLAUFMAN K.C., et al.
2025A&A...704A.108C 65       D     X         2 111 ~ Refractory element abundances in rocky planets and their host stars: Revisiting the compositional link. CHEN X. and NI D.

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