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| Kepler-1530 , the SIMBAD biblio (44 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:24:55 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
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. | ||
|
2014A&A...566A.103L |
15 | D | 2 | 359 | 102 | High-resolution imaging of Kepler planet host candidates. A comprehensive comparison of different techniques. | LILLO-BOX J., BARRADO D. and BOUY H. | ||
|
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 | 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. | ||
|
2015ApJ...814..130M |
16 | D | 3 | 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 | 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. | ||
|
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 | 4 | 2500 | 58 | Observational evidence for two distinct giant planet populations. | SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., 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. | ||
|
2018ApJS..237...38B |
16 | 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 |
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. | ||
|
2018AJ....156..292T |
16 | 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 |
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 | 3 | 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. | ||
|
2020AJ....160..108B |
16 | D | 3 | 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 |
16 | D | 1 | 365763 | 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. | ||
| 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. | ||
|
2021ApJS..255...17S |
17 | D | 1 | 39591 | 57 | Surface rotation and photometric activity for Kepler targets. II. G and F main-sequence stars and cool subgiant stars. | SANTOS A.R.G., BRETON S.N., MATHUR S., 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..128W |
17 | D | 1 | 1570 | 6 | The influence of 10 unique chemical elements in shaping the distribution of Kepler planets. | WILSON R.F., CANAS C.I., MAJEWSKI S.R., et al. | ||
|
2022AJ....163..152S |
17 | D | 1 | 583193 | 11 | APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. | SPRAGUE D., CULHANE C., KOUNKEL M., 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. | ||
| 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. | ||
|
2022ApJS..259...35A |
17 | D | 1 | 611005 | 320 | The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. | ABDURRO'UF, ACCETTA K., AERTS C., et al. | ||
|
2022AJ....164...60S |
17 | D | 2 | 854 | 2 | Galactic Chemical Evolution of Exoplanet Hosting Stars: Are High-mass Planetary Systems Young? | SWASTIK C., BANYAL R.K., NARANG M., et al. | ||
|
2022ApJS..261...26S |
17 | D | 2 | 1893 | 2 | Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys. | SU T., ZHANG L.-Y., LONG L., 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. | ||
|
2023ApJS..265...50C |
17 | D | 1 | 2291 | ~ | Characterization of Low-mass Companions to Kepler Objects of Interest Observed with APOGEE-N. | CANAS C.I., BENDER C.F., MAHADEVAN S., et al. | ||
|
2024AJ....167...55H |
18 | D | 6 | 586 | ~ | Kepler-discovered Multiple-planet Systems near Period Ratios Suggestive of Mean-motion Resonances Are Young. | HAMER J.H. and SCHLAUFMAN K.C. | ||
|
2024MNRAS.533.1290S |
18 | D | 1 | 7737 | ~ | The impact of stellar metallicity on rotation and activity evolution in the Kepler field using gyro-kinematic ages. | SEE V., LU Y., AMARD L., et al. | ||
|
2024AJ....168..109S |
18 | D | 2 | 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. | ||
| 2024AJ....168..154V | 18 | D | 4 | 210 | ~ | Modeling Multiple Radius Valley Emergence Mechanisms with Multitransiting Systems. | VANWYNGARDEN M. and CLOUTIER R. | ||
|
2024A&A...689A.250C |
18 | D | 3 | 3075 | ~ | Mapping the exo-Neptunian landscape A ridge between the desert and savanna. | CASTRO-GONZALEZ A., BOURRIER V., LILLO-BOX J., et al. | ||
|
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. | ||
| 2025ApJ...978...18F | 19 | D | 1 | 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. | ||
|
2025A&A...699A.100D |
19 | D | 1 | 2580 | ~ | The Gaia spectroscopic catalogue of exoplanets and host stars. | DE LAVERNY P., LIGI R., CRIDA A., et al. |