Kepler-289b , the SIMBAD biblio

Kepler-289b , the SIMBAD biblio (50 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST07:56:51

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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
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.
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.
2014A&A...566A.103L viz 15       D               1 359 102 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.
2014ApJ...795..167S viz 1664 T   A D S   X C       41 30 33 Planet hunters. VII. Discovery of a new low-mass, low-density planet (PH3 c) orbiting Kepler-289 with mass measurements of two additional planets (PH3 b and d). SCHMITT J.R., AGOL E., DECK K.M., 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...802..116D 118           X         3 13 44 Measurement of planet masses with transit timing variations due to synodic ''chopping'' effects. DECK K.M. and AGOL E.
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...806..248W viz 16       D               1 143 44 Influence of stellar multiplicity on planet formation. III. Adaptive optics imaging of Kepler stars with gas giant planets. WANG J., FISCHER D.A., HORCH E.P., 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.
2016ApJ...820...39J 16       D               1 107 126 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.
2016A&A...587A..64S viz 16       D               1 179 172 SOPHIE velocimetry of Kepler transit candidates. XVII. The physical properties of giant exoplanets within 400 days of period. SANTERNE A., MOUTOU C., TSANTAKI M., 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.
2016ApJ...825...98H 16       D               1 166 128 Warm jupiters are less lonely than hot jupiters: close neighbors. HUANG C., WU Y. and TRIAUD A.H.M.J.
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.
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..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.
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 81           X         2 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.
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.
2019A&A...630A.135U viz 16       D               1 501 16 Beyond the exoplanet mass-radius relation. ULMER-MOLL S., SANTOS N.C., FIGUEIRA P., 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.
2020AJ....160...96T viz 42           X         1 14 24 TESS reveals a short-period sub-Neptune sibling (HD 86226c) to a known long-period giant planet. TESKE J., DIAZ M.R., LUQUE R., 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.
2021MNRAS.503.4092B 17       D               1 124 ~ Revisiting the Kepler field with TESS: Improved ephemerides using TESS 2 min data. BATTLEY M.P., KUNIMOTO M., ARMSTRONG D.J., et al.
2021AJ....161..246J viz 309       D     X         8 204 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.
2021A&A...649L...5B 17       D               2 41 19 Dry or water world? How the water contents of inner sub-Neptunes constrain giant planet formation and the location of the water ice line. BITSCH B., RAYMOND S.N., BUCHHAVE L.A., et al.
2021A&A...650A..66B viz 84               F     1 45 28 Constraints on the mass and on the atmospheric composition and evolution of the low-density young planet DS Tucanae A b. BENATTI S., DAMASSO M., BORSA F., 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.
2022AJ....164...42J 17       D               1 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               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.
2023AJ....165...48G viz 670       D     X C       15 4 3 Constraining the Densities of the Three Kepler-289 Planets with Transit Timing Variations. GREKLEK-MCKEON M., KNUTSON H.A., VISSAPRAGADA 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.
2023AJ....165..235M viz 87           X         2 28 1 Hyades Member K2-136c: The Smallest Planet in an Open Cluster with a Precisely Measured Mass. MAYO A.W., DRESSING C.D., VANDERBURG A., 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.
2024A&A...687L...1L viz 18       D               1 140 ~ Resonant sub-Neptunes are puffier. LELEU A., DELISLE J.-B., BURN R., et al.
2025AJ....169...90O viz 65       D     X         2 194 ~ Planetary Mass Determinations from a Simplified Photodynamical Model-Application to the Complete Kepler Dataset. OFIR A., YOFFE G. and AHARONSON O.

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