Kepler-487 , the SIMBAD biblio

Kepler-487 , the SIMBAD biblio (87 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST06:53:34


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Title First 3 Authors
2024ApJ...973L...4R 90               F     1 49 ~ The Distribution of Planet Radius in Kepler Multiplanet Systems Depends on Gap Complexity. RICE D.R., STEFFEN J.H. and VAZAN A.
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.
2014ApJ...791...35L viz 271     A D S   X         7 800 137 Robotic laser adaptive optics imaging of 715 Kepler exoplanet candidates using Robo-AO. LAW N.M., MORTON T., BARANEC C., et al.
2014ApJS..210...19B viz 15       D               4 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.
2023ApJ...954..137S 87               F     1 64 ~ Can Cold Jupiters Sculpt the Edge-of-the-multis? SOBSKI N. and MILLHOLLAND S.C.
2013ApJ...775L..11M viz 15       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.
2018AJ....155...94S 99       D S             5 51 191 Identifying exoplanets with deep learning: a five-planet resonant chain around Kepler-80 and an eighth planet around Kepler-90. SHALLUE C.J. and VANDERBURG A.
2021ApJ...919...26U 17       D               2 65 5 Radius and mass distribution of ultra-short-period planets. UZSOY A.S.M., ROGERS L.A. and PRICE E.M.
2019AJ....158...65D 82               F     1 14 22 TOI-216b and TOI-216 c: two warm, large exoplanets in or slightly wide of the 2:1 orbital resonance. DAWSON R.I., HUANG C.X., LISSAUER J.J., et al.
2020AJ....160..138H viz 16       D               1 72 17 Ultra-short-period planets are stable against tidal inspiral. HAMER J.H. and SCHLAUFMAN K.C.
2024AJ....167..103J viz 90           X         2 190 ~ Kepler Multitransiting System Physical Properties and Impact Parameter Variations. JUDKOVSKY Y., OFIR A. and AHARONSON O.
2021MNRAS.505.2500P 894       D     X C F     20 25 12 In situ formation of hot Jupiters with companion super-Earths. POON S.T.S., NELSON R.P. and COLEMAN G.A.L.
2016ApJ...825...98H 16       D               1 166 128 Warm jupiters are less lonely than hot jupiters: close neighbors. HUANG C., WU Y. and TRIAUD A.H.M.J.
2013PASP..125..793T 15       D               1 26 2 100-year DASCH light curves of Kepler planet-candidate host stars. TANG S., SASSELOV D., GRINDLAY J., et al.
2018ApJ...861..149F viz 16       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.
2022ApJ...926..120V 17       D               1 645 13 ExoMiner: A Highly Accurate and Explainable Deep Learning Classifier That Validates 301 New Exoplanets. VALIZADEGAN H., MARTINHO M.J.S., WILKENS L.S., et al.
2025AJ....169..149H 93               F     3 222 ~ Architecture Classification for Extrasolar Planetary Systems. HOWE A.R., BECKER J.C., STARK C.C., et al.
2023MNRAS.524.1113S 17       D               4 85 ~ TESS spots a mini- interior to a hot saturn in the TOI-2000 system. SHA L., VANDERBURG A.M., HUANG C.X., et al.
2025ApJ...978...18F 625       D     X C       13 41 ~ More Likely Than You Think: Inclination-driving Secular Resonances Are Common in Known Exoplanet Systems. FARIDANI T.H., NAOZ S., LI G., et al.
2020AJ....160..108B viz 16       D               4 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.
2012ApJ...756..186S viz 15       D               3 811 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.
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.
2015ApJ...812L..11S 39           X         1 12 21 A low stellar obliquity for WASP-47, a compact multiplanet system with a hot Jupiter and an ultra-short period planet. SANCHIS-OJEDA R., WINN J.N., DAI F., et al.
2013ApJS..208...16M viz 15       D               3 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.
2011ApJS..197....2F viz 15       D               4 980 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.
2018AJ....156...96W 425     A S   X C       9 31 3 TTV-determined masses for warm Jupiters and their close planetary companions. WU D.-H., WANG S., ZHOU J.-L., et al.
2013ApJ...774L..12S viz 15       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.
2020MNRAS.497.4091M 82           X         2 57 ~ Dynamical evolution of two-planet systems and its connection with white dwarf atmospheric pollution. MALDONADO R.F., VILLAVER E., MUSTILL A.J., et al.
2017AJ....153...25A viz 238           X         6 179 7 Probability of the physical association of 104 blended companions to Kepler Objects of Interest using visible and near-infrared adaptive optics photometry. ATKINSON D., BARANEC C., ZIEGLER C., et al.
2010ApJ...725.1226S 920   K   D     X C       24 22 70 Five Kepler target stars that show multiple transiting exoplanet candidates. STEFFEN J.H., BATALHA N.M., BORUCKI W.J., et al.
2011ApJ...728..117B viz 129       D     X C       3 321 310 Characteristics of Kepler planetary candidates based on the first data set. BORUCKI W.J., KOCH D.G., BASRI G., et al.
2011ApJ...738..170M viz 15       D               4 997 230 On the low false positive probabilities of Kepler planet candidates. MORTON T.D. and JOHNSON J.A.
2017NewA...55....1H 16       D               1 146 2 Multiple planetary systems: properties of the current sample. HOBSON M.J. and GOMEZ M.
2011ApJ...742L..19M viz 15       D               1 185 37 Compositions of hot super-Earth atmospheres: exploring Kepler candidates. MIGUEL Y., KALTENEGGER L., FEGLEY B., et al.
2011ApJS..197...12D 15       D               1 124 184 Lack of inflated radii for Kepler giant planet candidates receiving modest stellar irradiation. DEMORY B.-O. and SEAGER S.
2012ApJ...752...72D viz 15       D               1 229 7 A correlation between the eclipse depths of Kepler gas giant candidates and the metallicities of their parent stars. DODSON-ROBINSON S.E.
2012ApJ...756..185F viz 15       D               3 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.
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.
2013MNRAS.435.1126B 15       D               1 72 20 Exoplanet predictions based on the generalized Titius-Bode relation. BOVAIRD T. and LINEWEAVER C.H.
2015MNRAS.448.3608B viz 16       D               2 156 6 Using the inclinations of Kepler systems to prioritize new Titius-Bode-based exoplanet predictions. BOVAIRD T., LINEWEAVER C.H. and JACOBSEN S.K.
2015ApJ...814..130M viz 16       D               4 2846 162 An increase in the mass of planetary systems around lower-mass stars. MULDERS G.D., PASCUCCI I. and APAI D.
2016ApJ...821...47B viz 16       D               1 217 14 Efficient geometric probabilities of multi-transiting exoplanetary systems from CORBITS. BRAKENSIEK J. and RAGOZZINE D.
2015ApJ...807..170H viz 16       D               3 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.
2019AJ....158...59S viz 301       D     X C       7 109 ~ Autoregressive planet search: feasibility study for irregular time series. STUHR A.M., FEIGELSON E.D., CACERES G.A., et al.
2020ApJ...890L..31L viz 16       D               1 85 ~ Mutual inclination excitation by stellar oblateness. LI G., DAI F. and BECKER J.
2014A&A...566A.103L viz 480       D     X C       12 359 102 High-resolution imaging of Kepler planet host candidates. A comprehensive comparison of different techniques. LILLO-BOX J., BARRADO D. and BOUY H.
2019A&A...631A.152A 16       D               2 121 ~ Dusty phenomena in the vicinity of giant exoplanets. ARKHYPOV O.V., KHODACHENKO M.L. and HANSLMEIER A.
2013ApJ...763...41C viz 15       D               2 97 40 On the relative sizes of planets within Kepler multiple-candidate systems. CIARDI D.R., FABRYCKY D.C., FORD E.B., et al.
2023AJ....165..177S viz 17       D               5 131 ~ Revising Properties of Planet-Host Binary Systems. III. There Is No Observed Radius Gap for Kepler Planets in Binary Star Systems. SULLIVAN K., KRAUS A.L., HUBER D., 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.
2018AJ....156...83Z viz 16       D               1 337 14 Robo-AO Kepler Survey. V. The effect of physically associated stellar companions on planetary systems. ZIEGLER C., LAW N.M., BARANEC C., et al.
2014ApJ...783....4W viz 39           X         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.
2025AJ....169..191G 93               F     1 50 ~ Statistical Reevaluation of the Ultra-short-period Planet Classification Boundary: Smaller Planets within 1 Day, Larger Period Ratios below 2 Days. GOYAL A.V. and WANG S.
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.
2014ApJ...787...47S viz 15       D               1 222 160 A study of the shortest-period planets found with Kepler. SANCHIS-OJEDA R., RAPPAPORT S., WINN J.N., 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.
2017AJ....153..117H viz 16       D               1 170 51 Assessing the effect of stellar companions from high-resolution imaging of Kepler Objects of Interest. HIRSCH L.A., CIARDI D.R., HOWARD A.W., et al.
2016ApJS..225....9H viz 16       D               6 2132 124 Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set. HOLCZER T., MAZEH T., NACHMANI G., et al.
2015ApJ...812L..18B 51           X         1 8 202 WASP-47: a hot Jupiter system with two additional planets discovered by K2. BECKER J.C., VANDERBURG A., ADAMS F.C., et al.
2017AJ....154...60W 16       D               1 95 50 Absence of a metallicity effect for ultra-short-period planets. WINN J.N., SANCHIS-OJEDA R., ROGERS L., et al.
2014ApJ...794..133S 15       D               1 41 21 Statistical eclipses of close-in Kepler sub-saturns. SHEETS H.A. and DEMING D.
2019AJ....157..145M viz 41           X         1 16 5 Long-period giant companions to three compact, multiplanet systems. MILLS S.M., HOWARD A.W., WEISS L.M., et al.
2018ApJ...869...66H viz 16       D               1 99 ~ The application of autocorrelation SETI search techniques in an ATA survey. HARP G.R., ACKERMANN R.F., ASTORGA A., et al.
2012ApJS..199...24T viz 15       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.
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.
2020ApJ...890...23L viz 16       D               4 4936 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.
2021ApJ...920...19G viz 17       D               1 807 5 A spectroscopic analysis of the California-Kepler Survey sample. II. Correlations of stellar metallicities with planetary architectures. GHEZZI L., MARTINEZ C.F., WILSON R.F., 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.
2022A&A...663A...4S viz 17       D               1 14206 7 Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys. SOUBIRAN C., BROUILLET N. and CASAMIQUELA L.
2024AJ....168..129S viz 18       D               2 350 ~ Revising Properties of Planet-Host Binary Systems. IV. The Radius Distribution of Small Planets in Binary Star Systems Is Dependent on Stellar Separation. SULLIVAN K., KRAUS A.L., BERGER T.A., et al.
2024A&A...689A.250C viz 18       D               4 3075 ~ Mapping the exo-Neptunian landscape A ridge between the desert and savanna. CASTRO-GONZALEZ A., BOURRIER V., LILLO-BOX J., et al.
2018MNRAS.474.2094A viz 16       D               1 1073 143 Inferring probabilistic stellar rotation periods using Gaussian processes. ANGUS R., MORTON T., AIGRAIN S., et al.
2014AJ....147..119C viz 15       D               1 8013 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.
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...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.
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.
2021MNRAS.504.5327A 17       D               1 7000 19 Exoplanet validation with machine learning: 50 new validated Kepler planets. ARMSTRONG D.J., GAMPER J. and DAMOULAS T.
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.
2018ApJ...855..115B viz 16       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.
2017MNRAS.465.2634A viz 16       D               4 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..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.
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.
2024AJ....167...55H viz 18       D               20 586 ~ Kepler-discovered Multiple-planet Systems near Period Ratios Suggestive of Mean-motion Resonances Are Young. HAMER J.H. and SCHLAUFMAN K.C.
2024AJ....168..109S viz 108       D       C       3 702 ~ Resonant and Ultra-short-period Planet Systems Are at Opposite Ends of the Exoplanet Age Distribution. SCHMIDT S.P., SCHLAUFMAN K.C. and HAMER J.H.
2024A&A...691A..53S viz 18       D               1 4078 ~ SWEET-Cat: A view on the planetary mass-radius relation. SOUSA S.G., ADIBEKYAN V., DELGADO-MENA E., et al.
2026ApJ...998..301G 20       D               1 561 ~ A Comprehensive Study of the Relations between the Properties of Planetary Systems and the Chemical Compositions of Their Host Stars. GHEZZI L., COSTA-ALMEIDA E., LOAIZA-TACURI V., et al.

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