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Kepler-1130 , the SIMBAD biblio (59 results) | C.D.S. - SIMBAD4 rel 1.8 - 2023.09.30CEST08:26:36 |
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 |
---|---|---|---|---|---|---|---|---|---|
2013ApJS..204...24B ![]() |
16 | D | 1 | 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...770...69P ![]() |
16 | D | 1 | 245 | 238 | A plateau in the planet population below twice the size of Earth. | PETIGURA E.A., MARCY G.W. and HOWARD A.W. | ||
2013ApJ...772...74W | 40 | X | 1 | 59 | 175 | Density and eccentricity of Kepler planets. | WU Y. and LITHWICK Y. | ||
2013ApJ...774L..12S ![]() |
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 ![]() |
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 ![]() |
16 | D | 1 | 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. | ||
2013MNRAS.435.1126B | 16 | D | 1 | 72 | 20 | Exoplanet predictions based on the generalized Titius-Bode relation. | BOVAIRD T. and LINEWEAVER C.H. | ||
2013MNRAS.436.1883W ![]() |
16 | D | 1 | 961 | 136 | Rotation periods, variability properties and ages for Kepler exoplanet candidate host stars. | WALKOWICZ L.M. and BASRI G.S. | ||
2013A&A...560A...4R ![]() |
16 | D | 1 | 24132 | 291 | Rotation and differential rotation of active Kepler stars. | REINHOLD T., REINERS A. and BASRI G. | ||
2014ApJS..210...19B ![]() |
16 | 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. | ||
2014ApJ...783....4W ![]() |
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...784...45R ![]() |
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 ![]() |
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...788L...9B ![]() |
16 | D | 1 | 293 | 26 | Larger planet radii inferred from stellar "flicker" brightness variations of bright planet-host stars. | BASTIEN F.A., STASSUN K.G. and PEPPER J. | ||
2014ApJ...791..111W | 16 | D | 3 | 56 | 105 | Influence of stellar multiplicity on planet formation. II. Planets are less common in multiple-star systems with separations smaller than 1500 AU. | WANG J., FISCHER D.A., XIE J.-W., 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. | ||
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. | ||
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...807..170H ![]() |
16 | D | 1 | 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...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. | ||
2015ApJ...813..130W ![]() |
16 | D | 2 | 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 ![]() |
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. | ||
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. | ||
2016AJ....152....8K ![]() |
16 | D | 1 | 389 | 203 | The impact of stellar multiplicity on planetary systems. I. The ruinous influence of close binary companions. | KRAUS A.L., IRELAND M.J., HUBER D., et al. | ||
2016ApJS..225....9H ![]() |
16 | D | 1 | 2132 | 124 | Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set. | HOLCZER T., MAZEH T., NACHMANI G., et al. | ||
2016ApJS..225...32B ![]() |
16 | D | 1 | 1473 | 266 | Spectral properties of cool stars: extended abundance analysis of 1,617 planet-search stars. | BREWER J.M., FISCHER D.A., VALENTI J.A., et al. | ||
2016A&A...594A..39F ![]() |
16 | D | 2 | 51410 | 86 | Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra. | FRASCA A., MOLENDA-ZAKOWICZ J., DE CAT P., et al. | ||
2016AJ....152..181H ![]() |
16 | D | 1 | 9279 | 22 | SETI observations of exoplanets with the Allen Telescope Array. | HARP G.R., RICHARDS J., TARTER J.C., et al. | ||
2016AJ....152..187M ![]() |
16 | D | 4 | 471 | 74 | A super-solar metallicity for stars with hot rocky exoplanets. | MULDERS G.D., PASCUCCI I., APAI D., et al. | ||
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. | ||
2017MNRAS.465.2634A ![]() |
16 | D | 3 | 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. | ||
2017A&A...603A..30S ![]() |
16 | D | 2 | 2500 | 58 | Observational evidence for two distinct giant planet populations. | SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al. | ||
2018AJ....155...68W ![]() |
17 | D | 1 | 509 | 18 | Elemental abundances of Kepler Objects of Interest in APOGEE. I. Two distinct orbital period regimes inferred from host star iron abundances. | WILSON R.F., TESKE J., MAJEWSKI S.R., et al. | ||
2018AJ....155...94S | 20 | D | 1 | 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. | ||
2018ApJ...855..115B ![]() |
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 ![]() |
17 | D | 1 | 1073 | 143 | Inferring probabilistic stellar rotation periods using Gaussian processes. | ANGUS R., MORTON T., AIGRAIN S., et al. | ||
2018AJ....155..161Z ![]() |
142 | D | X | 4 | 1274 | 24 | Robo-AO Kepler survey. IV. The effect of nearby stars on 3857 planetary candidate systems. | ZIEGLER C., LAW N.M., BARANEC C., et al. | |
2018ApJ...861..149F ![]() |
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. | ||
2018AJ....156...83Z ![]() |
17 | 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. | ||
2018ApJS..237...38B ![]() |
17 | D | 1 | 1111 | 42 | Spectral properties of cool stars: extended abundance analysis of Kepler Objects of Interest. | BREWER J.M. and FISCHER D.A. | ||
2018ApJ...866...99B ![]() |
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 ![]() |
17 | D | 2 | 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 ![]() |
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. | ||
2019MNRAS.490.5088M ![]() |
17 | D | 2 | 214 | 32 | Search for stellar companions of exoplanet host stars by exploring the second ESA-Gaia data release. | MUGRAUER M. | ||
2020ApJ...888...43C ![]() |
17 | D | 1 | 489 | 32 | Chemical evolution in the Milky Way: rotation-based ages for APOGEE-Kepler Cool dwarf stars. | CLAYTOR Z.R., VAN SADERS J.L., SANTOS A.R.G., et al. | ||
2020ApJ...890...23L ![]() |
17 | D | 4 | 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...893L...1W | 131 | X F | 2 | 51 | 33 | The Kepler peas in a pod pattern is astrophysical. | WEISS L.M. and PETIGURA E.A. | ||
2020A&A...636A..85S ![]() |
17 | D | 1 | 3696 | ~ | Derivation of parameters for 3748 FGK stars using H-band spectra from APOGEE Data Release 14. | SARMENTO P., DELGADO MENA E., ROJAS-AYALA B., et al. | ||
2020AJ....160..108B ![]() |
17 | 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. | ||
2020AJ....160..120J ![]() |
17 | D | 1 | 365761 | 238 | APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. | JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al. | ||
2021ApJ...909..115C ![]() |
18 | D | 1 | 2175 | 13 | Planets Across Space and Time (PAST). I. Characterizing the memberships of Galactic components and stellar ages: revisiting the kinematic methods and applying to planet host stars. | CHEN D.-C., XIE J.-W., ZHOU J.-L., et al. | ||
2021AJ....162...98B ![]() |
18 | D | 1 | 2175 | ~ | Seeking echoes of circumstellar disks in Kepler light curves. | BROMLEY B.C., LEONARD A., QUINTANILLA A., et al. | ||
2021ApJ...920...19G ![]() |
90 | X | 2 | 8 | 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....164...72M | 93 | F | 1 | 61 | 6 | Edge-of-the-Multis: Evidence for a Transition in the Outer Architectures of Compact Multiplanet Systems. | MILLHOLLAND S.C., HE M.Y. and ZINK J.K. | ||
2023AJ....166...36H | 300 | X C | 5 | 28 | 1 | Inner Planetary System Gap Complexity is a Predictor of Outer Giant Planets. | HE M.Y. and WEISS L.M. | ||
2023AJ....166...94M | 20 | D | 3 | 105 | ~ | exoMMR: A New Python Package to Confirm and Characterize Mean Motion Resonances. | MacDONALD M.G., POLANIA VIVAS M.S., D'ANGIOLILLO S., et al. |
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