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Kepler-277 , the SIMBAD biblio

Kepler-277 , the SIMBAD biblio (50 results) C.D.S. - SIMBAD4 rel 1.8 - 2023.10.05CEST04:42:55

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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
2011ApJ...736...19B viz 15       D               1 1507 867 Characteristics of planetary candidates observed by Kepler. II. Analysis of the first four months of data. BORUCKI W.J., KOCH D.G., BASRI G., et al.
2011ApJ...738..170M viz 15       D               2 997 230 On the low false positive probabilities of Kepler planet candidates. MORTON T.D. and JOHNSON J.A.
2011ApJS..197....2F viz 15       D               2 980 66 Transit timing observations from Kepler. I. Statistical analysis of the first four months. FORD E.B., ROWE J.F., FABRYCKY D.C., et al.
2011ApJS..197....8L viz 16       D               1 177 608 Architecture and dynamics of Kepler's candidate multiple transiting planet systems. LISSAUER J.J., RAGOZZINE D., FABRYCKY D.C., et al.
2012MNRAS.420L..23V viz 16       D               1 94 22 Identifying non-resonant Kepler planetary systems. VERAS D. and FORD E.B.
2012ApJS..199...24T viz 16       D               1 5394 66 Detection of potential transit signals in the first three quarters of Kepler mission data. TENENBAUM P., CHRISTIANSEN J.L., JENKINS J.M., et al.
2012Natur.486..375B viz 16       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 16       D               2 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.
2012ApJ...756..186S viz 16       D               2 811 35 Transit timing observations from Kepler. VI. Potentially interesting candidate systems from fourier-based statistical tests. STEFFEN J.H., FORD E.B., ROWE J.F., et al.
2012A&A...547A..36A viz 16       D               1 87 98 Exploring the α-enhancement of metal-poor planet-hosting stars. The Kepler and HARPS samples. ADIBEKYAN V.Zh., DELGADO MENA E., SOUSA S.G., et al.
2013ApJ...772...74W 158           X C       3 59 175 Density and eccentricity of Kepler planets. WU Y. and LITHWICK Y.
2013ApJ...774L..12S viz 16       D               1 469 25 A lack of short-period multiplanet systems with close-proximity pairs and the curious case of Kepler-42. STEFFEN J.H. and FARR W.M.
2013ApJ...775L..11M viz 16       D               1 2010 189 Stellar rotation periods of the Kepler Objects of Interest: a dearth of close-in planets around fast rotators. McQUILLAN A., MAZEH T. and AIGRAIN S.
2013ApJS..208...16M viz 16       D               2 1518 139 Transit timing observations from Kepler. VIII. Catalog of transit timing measurements of the first twelve quarters. MAZEH T., NACHMANI G., HOLCZER T., et al.
2014ApJS..210...19B viz 16       D               2 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...25X viz 96       D       C       2 17 67 Transit timing variation of near-resonance planetary pairs. II. Confirmation of 30 planets in 15 multiple-planet systems. XIE J.-W.
2014ApJ...783....4W viz 16       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...783..123C viz 16       D               1 221 18 Limits on surface gravities of Kepler planet-candidate host stars from non-detection of solar-like oscillations. CAMPANTE T.L., CHAPLIN W.J., LUND M.N., et al.
2014ApJ...784...45R viz 16       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.
2014AJ....147..119C viz 16       D               1 8010 91 Contamination in the Kepler field. Identification of 685 KOIs as false positives via ephemeris matching based on Q1-Q12 data. COUGHLIN J.L., THOMPSON S.E., BRYSON S.T., et al.
2014ApJ...787...80H viz 16       D               1 261 190 Densities and eccentricities of 139 Kepler planets from transit time variations. HADDEN S. and LITHWICK Y.
2015ApJ...801....3M viz 16       D               1 3357 109 Photometric amplitude distribution of stellar rotation of KOIs–Indication for spin-orbit alignment of cool stars and high obliquity for hot stars. MAZEH T., PERETS H.B., McQUILLAN A., 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...807..170H viz 16       D               2 2117 10 Time variation of Kepler transits induced by stellar Spots–A way to distinguish between prograde and retrograde motion. II. Application to KOIs. HOLCZER T., SHPORER A., MAZEH T., et al.
2015ApJ...813..100O viz 16       D               1 327 7 Deep GALEX UV survey of the Kepler field. I. Point source catalog. OLMEDO M., LLOYD J., MAMAJEK E.E., et al.
2015ApJ...813..130W viz 16       D               1 211 27 Influence of stellar multiplicity on planet formation. IV. Adaptive optics imaging of Kepler stars with multiple transiting planet candidates. WANG J., FISCHER D.A., XIE J.-W., et al.
2015ApJ...814..130M viz 16       D               2 2846 162 An increase in the mass of planetary systems around lower-mass stars. MULDERS G.D., PASCUCCI I. and APAI D.
2016ApJ...822...86M viz 16       D               1 6130 337 False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives. MORTON T.D., BRYSON S.T., COUGHLIN J.L., et al.
2016ApJS..225....9H viz 16       D               5 2132 124 Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set. HOLCZER T., MAZEH T., NACHMANI G., et al.
2017AJ....153...71F viz 16       D               1 3575 164 The Kepler follow-up observation program. I. A catalog of companions to Kepler stars from high-resolution imaging. FURLAN E., CIARDI D.R., EVERETT M.E., et al.
2017MNRAS.465.2634A viz 16       D               2 5400 21 Transit shapes and self-organizing maps as a tool for ranking planetary candidates: application to Kepler and K2. ARMSTRONG D.J., POLLACCO D. and SANTERNE A.
2017AJ....154....5H viz 41           X         1 231 145 Kepler planet masses and eccentricities from TTV analysis. HADDEN S. and LITHWICK Y.
2017AJ....154..107P viz 16       D               1 1306 226 The California-Kepler Survey. I. High-resolution spectroscopy of 1305 stars hosting Kepler transiting planets. PETIGURA E.A., HOWARD A.W., MARCY G.W., 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.
2017A&A...603A..30S viz 16       D               4 2500 58 Observational evidence for two distinct giant planet populations. SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al.
2018ApJS..234....9O viz 17       D               1 436 14 A spectral approach to transit timing variations. OFIR A., XIE J.-W., JIANG C.-F., et al.
2018ApJ...855..115B viz 17       D               1 1305 5 Identifying young Kepler planet host stars from Keck-HIRES spectra of lithium. BERGER T.A., HOWARD A.W. and BOESGAARD A.M.
2018MNRAS.474.2094A viz 17       D               1 1073 143 Inferring probabilistic stellar rotation periods using Gaussian processes. ANGUS R., MORTON T., AIGRAIN S., et al.
2018ApJ...861..149F viz 17       D               1 2261 6 The Kepler Follow-up Observation Program. II. Stellar parameters from medium- and high-resolution spectroscopy. FURLAN E., CIARDI D.R., COCHRAN W.D., et al.
2018ApJ...866...99B viz 17       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..292T viz 17       D               1 647 8 The effects of stellar companions on the observed transiting exoplanet radius distribution. TESKE J.K., CIARDI D.R., HOWELL S.B., et al.
2019ApJ...875...29M viz 17       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....158..239T viz 273       D     X         7 25 32 Do metal-rich stars make metal-rich planets? New insights on giant planet formation from host star abundances. TESKE J.K., THORNGREN D., FORTNEY J.J., et al.
2020ApJ...890...23L viz 17       D               2 4935 35 Current population statistics do not favor photoevaporation over core-powered mass loss as the dominant cause of the exoplanet radius gap. LOYD R.O.P., SHKOLNIK E.L., SCHNEIDER A.C., et al.
2020ApJ...890L..31L viz 17       D               1 85 ~ Mutual inclination excitation by stellar oblateness. LI G., DAI F. and BECKER J.
2020AJ....160..108B viz 17       D               2 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.
2020A&A...640A..32H viz 88           X         2 13 17 Discovery and characterization of the exoplanets WASP-148b and c. A transiting system with two interacting giant planets. HEBRARD G., DIAZ R.F., CORREIA A.C.M., et al.
2021AJ....161...68L viz 18       D               2 253 24 Hot stars with Kepler planets have high obliquities. LOUDEN E.M., WINN J.N., PETIGURA E.A., et al.
2021AJ....162...98B viz 18       D               1 2175 ~ Seeking echoes of circumstellar disks in Kepler light curves. BROMLEY B.C., LEONARD A., QUINTANILLA A., et al.
2022AJ....163...91J 93           X         2 248 ~ Physical properties and impact parameter variations of Kepler planets from analytic light-curve modeling. JUDKOVSKY Y., OFIR A. and AHARONSON O.

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2023.10.05-04:42:55

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