Kepler-279d , the SIMBAD biblio

Kepler-279d , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:20:44

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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 614       S   X C       14 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...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.
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.
2017AJ....154....5H viz 16       D               1 231 145 Kepler planet masses and eccentricities from TTV analysis. HADDEN S. and LITHWICK Y.
2018ApJS..234....9O viz 80           X         2 436 14 A spectral approach to transit timing variations. OFIR A., XIE J.-W., JIANG C.-F., 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.
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.
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...41T viz 16       D               1 564 ~ Estimating planetary mass with deep learning. TASKER E.J., LANEUVILLE M. and GUTTENBERG N.
2020AJ....159..124K viz 41           X         1 131 ~ Searching the entirety of Kepler data. I. 17 new planet candidates including one Habitable Zone world. KUNIMOTO M., MATTHEWS J.M. and NGO H.
2020AJ....159..248K 60       D     X         2 26 62 Searching the entirety of Kepler data. II. Occurrence rate estimates for FGK stars. KUNIMOTO M. and MATTHEWS J.M.
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.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.
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.
2024AJ....167..103J viz 18       D               1 190 ~ Kepler Multitransiting System Physical Properties and Impact Parameter Variations. JUDKOVSKY Y., OFIR A. and AHARONSON O.
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.

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