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| Kepler-487 , the SIMBAD biblio (87 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST06:53:34 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 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 |
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 |
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 |
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 |
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 |
16 | D | 1 | 72 | 17 | Ultra-short-period planets are stable against tidal inspiral. | HAMER J.H. and SCHLAUFMAN K.C. | ||
|
2024AJ....167..103J |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
16 | D | 1 | 217 | 14 | Efficient geometric probabilities of multi-transiting exoplanetary systems from CORBITS. | BRAKENSIEK J. and RAGOZZINE D. | ||
|
2015ApJ...807..170H |
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 |
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 |
16 | D | 1 | 85 | ~ | Mutual inclination excitation by stellar oblateness. | LI G., DAI F. and BECKER J. | ||
|
2014A&A...566A.103L |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
16 | D | 1 | 1073 | 143 | Inferring probabilistic stellar rotation periods using Gaussian processes. | ANGUS R., MORTON T., AIGRAIN S., et al. | ||
|
2014AJ....147..119C |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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. |