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Kepler-1035 , the SIMBAD biblio (34 results) | C.D.S. - SIMBAD4 rel 1.8 - 2023.06.06CEST21:03:30 |
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 |
---|---|---|---|---|---|---|---|---|---|
2012ApJS..199...24T ![]() |
16 | D | 1 | 5394 | 51 | Detection of potential transit signals in the first three quarters of Kepler mission data. | TENENBAUM P., CHRISTIANSEN J.L., JENKINS J.M., et al. | ||
2013ApJS..204...24B ![]() |
16 | D | 1 | 3274 | 779 | 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...775L..11M ![]() |
16 | D | 1 | 2010 | 107 | 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 | 92 | 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.436.1883W ![]() |
16 | D | 1 | 961 | 86 | Rotation periods, variability properties and ages for Kepler exoplanet candidate host stars. | WALKOWICZ L.M. and BASRI G.S. | ||
2014ApJS..210...19B ![]() |
16 | D | 1 | 5860 | 162 | Planetary candidates observed by Kepler IV: planet sample from Q1-Q8 (22 months). | BURKE C.J., BRYSON S.T., MULLALLY F., et al. | ||
2014AJ....147..119C ![]() |
16 | D | 1 | 8010 | 55 | 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...35L ![]() |
16 | D | 1 | 800 | 96 | Robotic laser adaptive optics imaging of 715 Kepler exoplanet candidates using Robo-AO. | LAW N.M., MORTON T., BARANEC C., et al. | ||
2015ApJ...801....3M ![]() |
16 | D | 1 | 3357 | 52 | 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 | 84 | Planetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months). | ROWE J.F., COUGHLIN J.L., ANTOCI V., et al. | ||
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 | 139 | Terrestrial planet occurrence rates for the Kepler GK dwarf sample. | BURKE C.J., CHRISTIANSEN J.L., MULLALLY F., et al. | ||
2015ApJ...814..130M ![]() |
16 | D | 1 | 2846 | 46 | An increase in the mass of planetary systems around lower-mass stars. | MULDERS G.D., PASCUCCI I. and APAI D. | ||
2016ApJ...822...86M ![]() |
16 | D | 1 | 6130 | 192 | 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. | ||
2016ApJS..225....9H ![]() |
16 | D | 1 | 2132 | 33 | Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set. | HOLCZER T., MAZEH T., NACHMANI G., et al. | ||
2016A&A...594A..39F ![]() |
16 | D | 1 | 51410 | 21 | 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 | 1 | 471 | 33 | A super-solar metallicity for stars with hot rocky exoplanets. | MULDERS G.D., PASCUCCI I., APAI D., et al. | ||
2017AJ....153...25A ![]() |
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. | |||||
2017AJ....153...71F ![]() |
16 | D | 1 | 3575 | 46 | 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. | ||
2017AJ....153..117H ![]() |
16 | D | 1 | 170 | 15 | 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. | ||
2017MNRAS.465.2634A ![]() |
16 | D | 1 | 5400 | 9 | 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 | 56 | 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 | 46 | 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 | 14 | Observational evidence for two distinct giant planet populations. | SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al. | ||
2018ApJ...855..115B ![]() |
17 | D | 1 | 1305 | 2 | 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 | 17 | Inferring probabilistic stellar rotation periods using Gaussian processes. | ANGUS R., MORTON T., AIGRAIN S., et al. | ||
2018ApJ...861..149F ![]() |
17 | D | 1 | 2261 | ~ | 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 ![]() |
17 | D | 1 | 1111 | ~ | 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 | 101 | 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 | 1 | 647 | ~ | 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 | ~ | 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 ![]() |
17 | D | 1 | 4935 | ~ | 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...919..138T | 18 | D | 1 | 531 | ~ | Further evidence for tidal spin-up of hot Jupiter host stars. | TEJADA AREVALO R.A., WINN J.N. and ANDERSON K.R. |
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