BD+44 3020e , the SIMBAD biblio

BD+44 3020e , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST08:40:25


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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               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...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.
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...787...80H viz 15       D               1 261 190 Densities and eccentricities of 139 Kepler planets from transit time variations. HADDEN S. and LITHWICK Y.
2014MNRAS.442..674H 39           X         1 40 10 Testing the Titius-Bode law predictions for Kepler multiplanet systems. HUANG C.X. and BAKOS G.A.
2015ApJS..217...16R viz 55       D     X         2 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..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....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.
2019ApJ...872...72C 16       D               1 15 ~ On the 9:7 mean motion resonance capture in a system of two equal-mass super-Earths. CUI Z., PAPALOIZOU J.C.B. and SZUSZKIEWICZ E.
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.
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.
2021MNRAS.507.1847R viz 1672     A D S   X C F     38 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....164...42J 213           X         5 79 3 TESS Observations of Kepler Systems with Transit Timing Variations. JONTOF-HUTTER D., DALBA P.A. and LIVINGSTON J.H.
2022AJ....164..139S 85           X         2 25 ~ Mass Upper Bounds for Over 50 Kepler Planets Using Low-S/N Transit Timing Variations. SIEGEL J.C. and ROGERS L.A.
2024ApJS..270....8W viz 108       D     X         3 250 ~ 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.
2025AJ....169..149H 47           X         1 222 ~ Architecture Classification for Extrasolar Planetary Systems. HOWE A.R., BECKER J.C., STARK C.C., et al.

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