Kepler-345b , the SIMBAD biblio

Kepler-345b , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:22:27

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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
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.
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...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...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.
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....5H viz 175       D     X         5 231 145 Kepler planet masses and eccentricities from TTV analysis. HADDEN S. and LITHWICK Y.
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...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.
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.
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.
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.
2020AJ....159..211C viz 16       D               1 351 93 Evolution of the radius valley around low-mass stars from Kepler and K2. CLOUTIER R. and MENOU K.
2022ApJS..261...26S viz 17       D               2 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.
2023A&A...669A.117L viz 235       D     X C       5 57 ~ Removing biases on the density of sub-Neptunes characterised via transit timing variations Update on the mass-radius relationship of 34 Kepler planets. LELEU A., DELISLE J.-B., UDRY 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.
2025AJ....169...90O viz 280     A D     X         7 194 ~ 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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