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| Kepler-1542 , the SIMBAD biblio (66 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST14:00:57 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2014ApJ...783....4W |
15 | 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. | ||
|
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. | ||
|
2014ApJ...788L...9B |
15 | 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. | ||
|
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 | 5 | 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...813..130W |
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 |
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 | 3 | 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. | ||
|
2016A&A...594A..39F |
16 | D | 1 | 51408 | 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..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 | 8 | 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. | ||
|
2018MNRAS.474.2094A |
16 | D | 1 | 1073 | 143 | Inferring probabilistic stellar rotation periods using Gaussian processes. | ANGUS R., MORTON T., AIGRAIN S., 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. | ||
|
2018ApJS..237...38B |
16 | D | 2 | 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...872...72C | 97 | D | X | 3 | 15 | ~ | On the 9:7 mean motion resonance capture in a system of two equal-mass super-Earths. | CUI Z., PAPALOIZOU J.C.B. and SZUSZKIEWICZ E. | |
|
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. | ||
|
2019ApJS..241...29Y |
16 | D | 1 | 3420 | 70 | The flare catalog and the flare activity in the Kepler mission. | YANG H. and LIU J. | ||
|
2020ApJ...890...23L |
16 | D | 5 | 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. | ||
|
2020ApJ...890L..31L |
16 | D | 1 | 85 | ~ | Mutual inclination excitation by stellar oblateness. | LI G., DAI F. and BECKER J. | ||
| 2020ApJ...893L...1W | 123 | X F | 2 | 51 | 33 | The Kepler peas in a pod pattern is astrophysical. | WEISS L.M. and PETIGURA E.A. | ||
| 2020AJ....159..207B | 16 | D | 1 | 150 | ~ | Transit duration variations in multiplanet systems. | BOLEY A.C., VAN LAERHOVEN C. and GRANADOS CONTRERAS A.P. | ||
|
2020AJ....160..108B |
16 | D | 5 | 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. | ||
|
2021ApJ...909..115C |
17 | D | 1 | 2176 | 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. | ||
| 2020PASJ...72...24L | 16 | D | 1 | 90 | ~ | The reliability of the Titius-Bode relation and its implications for the search for exoplanets. | LARA P., CORDERO-TERCERO G. and ALLEN C. | ||
| 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. | ||
|
2021ApJ...919..138T |
17 | D | 1 | 531 | 12 | Further evidence for tidal spin-up of hot Jupiter host stars. | TEJADA AREVALO R.A., WINN J.N. and ANDERSON K.R. | ||
|
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. | ||
| 2021ApJ...920L..34M | 84 | F | 1 | 48 | 16 | Split peas in a pod: intra-system uniformity of super-Earths and sub-Neptunes. | MILLHOLLAND S.C. and WINN J.N. | ||
|
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. | ||
|
2022A&A...661A..23F |
17 | D | 4 | 267 | 15 | Exoplanet X-ray irradiation and evaporation rates with eROSITA. | FOSTER G., POPPENHAEGER K., ILIC N., et al. | ||
|
2022AJ....164...60S |
17 | D | 4 | 854 | 2 | Galactic Chemical Evolution of Exoplanet Hosting Stars: Are High-mass Planetary Systems Young? | SWASTIK C., BANYAL R.K., NARANG M., et al. | ||
| 2022AJ....164...72M | 85 | 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. | ||
|
2022ApJS..261...26S |
17 | D | 32 | 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. | ||
|
2022A&A...664A..78F |
17 | D | 1 | 7452 | 7 | Characterization of Kepler targets based on medium-resolution LAMOST spectra analyzed with ROTFIT,. | FRASCA A., MOLENDA-ZAKOWICZ J., ALONSO-SANTIAGO J., et al. | ||
|
2023AJ....165..177S |
17 | D | 6 | 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. | ||
|
2023ApJ...946...61L |
61 | D | X | 2 | 257 | ~ | A Spectroscopic Analysis of a Sample of K2 Planet-host Stars: Stellar Parameters, Metallicities and Planetary Radii. | LOAIZA-TACURI V., CUNHA K., SMITH V.V., et al. | |
| 2023AJ....166...58Q | 435 | A | D | X C | 10 | 25 | ~ | Confirming Resonance in Three Transiting Systems. | QUINN T. and MacDONALD M.G. |
|
2023AJ....166...94M |
17 | 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. | ||
| 2023ApJ...954..137S | 87 | F | 1 | 64 | ~ | Can Cold Jupiters Sculpt the Edge-of-the-multis? | SOBSKI N. and MILLHOLLAND S.C. | ||
|
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....167..122H | 18 | D | 1 | 4 | ~ | Automated Scheduling of Doppler Exoplanet Observations at Keck Observatory. | HANDLEY L.B., PETIGURA E.A., MISIC V.V., et al. | ||
|
2024AJ....167..271V |
242 | D | X | 6 | 165 | ~ | Differences between Stable and Unstable Architectures of Compact Planetary Systems. | VOLK K. and MALHOTRA R. | |
| 2024ApJ...968L...4G | 90 | F | 1 | 48 | ~ | Peas-in-a-pod across the Radius Valley: Rocky Systems Are Less Uniform in Mass but More Uniform in Size and Spacing. | GOYAL A.V. and WANG S. | ||
|
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..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. | ||
| 2024ApJ...973L...4R | 134 | X | 3 | 49 | ~ | The Distribution of Planet Radius in Kepler Multiplanet Systems Depends on Gap Complexity. | RICE D.R., STEFFEN J.H. and VAZAN A. | ||
|
2024A&A...689A.250C |
18 | D | 5 | 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. | ||
| 2025MNRAS.536.3123J | 19 | D | 4 | 37 | ~ | FCN4Flare: fully convolution neural networks for flare detection. | JIA M., LUO A.-L. and QIU B. | ||
| 2025ApJ...980L..46H | 19 | D | 1 | 92 | ~ | Short-period Small Planets with High Mutual Inclinations are More Common around Metal-rich Stars. | HUA X., WANG S.X., AN D., et al. | ||
| 2025ApJS..277...15J | 19 | D | 2 | 136 | ~ | Half a Million Binary Stars Identified from the Low-resolution Spectra of LAMOST. | JING Y., MAO T.-X., WANG J., et al. | ||
| 2025ApJ...986..178Q | 19 | D | 1 | 450 | ~ | Revisiting the Li Abundances of Stars with and without Detected Planets from High-resolution Spectroscopy. | QIN J., YAN H.-L., CUI W., 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. | ||
| 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. |