BD+40 3638d , the SIMBAD biblio

BD+40 3638d , the SIMBAD biblio (43 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST22:57:58

Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
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               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...766..101C 96       D     X         3 18 145 Asteroseismic determination of obliquities of the exoplanet systems Kepler-50 and Kepler-65. CHAPLIN W.J., SANCHIS-OJEDA R., CAMPANTE T.L., 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.
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               1 261 190 Densities and eccentricities of 139 Kepler planets from transit time variations. HADDEN S. and LITHWICK Y.
2014ApJS..213...17P 15       D               1 19 8 Analytical solution for waves in planets with atmospheric superrotation. I. Acoustic and inertia-gravity waves. PERALTA J., IMAMURA T., READ P.L., 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.
2014A&A...569A..65B 77             C       1 17 27 Detecting the spin-orbit misalignment of the super-Earth. 55 Cancri e. BOURRIER V. and HEBRARD G.
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 133       D     X         4 105 201 Eccentricity from transit photometry: small planets in Kepler multi-planet systems have low eccentricities. VAN EYLEN V. and ALBRECHT S.
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...823...29A 16       D               1 117 7 Spin-orbit alignment for three transiting hot jupiters: WASP-103b, WASP-87b, and WASP-66b. ADDISON B.C., TINNEY C.G., WRIGHT D.J., 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..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.
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               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.
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 16       D               1 127 43 Testing exoplanet evaporation with multitransiting systems. OWEN J.E. and CAMPOS ESTRADA B.
2020A&A...634A..43O 58       D     X         2 141 104 Revisited mass-radius relations for exoplanets below 120 M⊕. OTEGI J.F., BOUCHY F. and HELLED R.
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.
2021AJ....161..246J viz 184       D     X         5 204 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.
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.
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.
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 17       D               1 122 ~ Quantitative correlation of refractory elemental abundances between rocky exoplanets and their host stars. LIU Z. and NI D.
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.
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.

goto View the references in ADS