BD+44 3020c , the SIMBAD biblio

BD+44 3020c , the SIMBAD biblio (51 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST08:12:40

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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
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.
2013Natur.494..452B 250           X   F     5 4 167 A sub-Mercury-sized exoplanet. BARCLAY T., ROWE J.F., LISSAUER J., 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.
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...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.
2014ApJS..210...20M viz 172       D     X C       4 94 394 Masses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planets. MARCY G.W., ISAACSON H., HOWARD A.W., et al.
2014ApJ...783L...6W 18       D               1 66 499 The mass-radius relation for 65 exoplanets smaller than 4 earth radii. WEISS L.M. and MARCY G.W.
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.
2014A&A...562A..80K 39           X         1 18 8 Impact of photo-evaporative mass loss on masses and radii of water-rich sub/super-Earths. KUROSAKI K., IKOMA M. and HORI Y.
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.
2014A&A...570A..36M 41           X         1 5 26 From planetesimals to planets: volatile molecules. MARBOEUF U., THIABAUD A., ALIBERT Y., et al.
2015ApJ...801...41R 122           X         3 52 558 Most 1.6 Earth-radius planets are not rocky. ROGERS L.A.
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 16       D               2 105 201 Eccentricity from transit photometry: small planets in Kepler multi-planet systems have low eccentricities. VAN EYLEN V. and ALBRECHT S.
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.
2015ApJ...815....5S viz 39           X         1 31 18 Detailed abundances of stars with small planets discovered by Kepler. I. The first sample. SCHULER S.C., VAZ Z.A., KATIME SANTRICH O.J., 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.
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.
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...853..163J 19       D               1 57 202 Compositional imprints in Density-Distance-Time: a rocky composition for close-in low-mass exoplanets from the location of the valley of evaporation. JIN S. and MORDASINI C.
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.
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.
2020MNRAS.491.5287O viz 16       D               1 127 43 Testing exoplanet evaporation with multitransiting systems. OWEN J.E. and CAMPOS ESTRADA B.
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.
2021A&A...645A...7K viz 17       D               1 1569 17 Determining the true mass of radial-velocity exoplanets with Gaia. Nine planet candidates in the brown dwarf or stellar regime and 27 confirmed planets. KIEFER F., HEBRARD G., LECAVELIER DES ETANGS A., et al.
2021MNRAS.507.1847R viz 268       D S   X   F     5 11 9 A HARPS-N mass for the elusive Kepler-37d: a case study in disentangling stellar activity and planetary signals. RAJPAUL V.M., BUCHHAVE L.A., LACEDELLI G., et al.
2022AJ....163..128W viz 17       D               1 1570 6 The influence of 10 unique chemical elements in shaping the distribution of Kepler planets. WILSON R.F., CANAS C.I., MAJEWSKI S.R., et al.
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.
2022RAA....22g2003J 85               F     1 114 7 CHES: A Space-borne Astrometric Mission for the Detection of Habitable Planets of the Nearby Solar-type Stars. JI J.-H., LI H.-T., ZHANG J.-B., et al.
2022A&A...662A..15M viz 17       D               1 733 3 Tidally driven tectonic activity as a parameter in exoplanet habitability. McINTYRE S.R.N.
2022AJ....164...42J 60       D     X         2 79 3 TESS Observations of Kepler Systems with Transit Timing Variations. JONTOF-HUTTER D., DALBA P.A. and LIVINGSTON J.H.
2022AJ....164..139S 468           X C       10 25 ~ Mass Upper Bounds for Over 50 Kepler Planets Using Low-S/N Transit Timing Variations. SIEGEL J.C. and ROGERS L.A.
2023MNRAS.519.6210M viz 17       D               1 688 1 A rocky exoplanet classification method and its application to calculating surface pressure and surface temperature. McINTYRE S.R.N., KING P.L. and MILLS F.P.
2023AJ....165..168O viz 17       D               1 281 1 The Demographics of Terrestrial Planets in the Venus Zone. OSTBERG C., KANE S.R., LI Z., et al.
2023A&A...677A..33B viz 17       D               1 120 ~ Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities No excess of cold Jupiters in small planet systems. BONOMO A.S., DUMUSQUE X., MASSA A., et al.
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.
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.
2025MNRAS.537.1268M 47           X         1 30 ~ Investigation of oscillations above the acoustic cut-off frequency for a sample of Kepler stars. II. Identifying temporal frequency shifts. MILLSON L.J., BROOMHALL A.-M., SANTOS A.R.G., et al.

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