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Kepler-397 , the SIMBAD biblio (30 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.03.28CET14:09:15 |
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 |
---|---|---|---|---|---|---|---|---|---|
2013ApJ...770...90G | 16 | D | 1 | 74 | 60 | Candidate planets in the habitable zones of Kepler stars. | GAIDOS E. | ||
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. | ||
2013ApJ...776...10W | 16 | D | 1 | 50 | 35 | Planet hunters. V. A confirmed jupiter-size planet in the habitable zone and 42 planet candidates from the Kepler archive data. | WANG J., FISCHER D.A., BARCLAY T., et al. | ||
2014ApJS..210...19B | 16 | D | 2 | 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...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. | ||
2015ApJ...798...66D | 40 | X | 1 | 296 | 60 | The photoeccentric effect and proto-hot jupiters. III. A paucity of proto-hot jupiters on super-eccentric orbits. | DAWSON R.I., MURRAY-CLAY R.A. and JOHNSON J.A. | ||
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. | ||
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...814..130M | 16 | D | 2 | 2846 | 162 | 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 | 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...18B | 16 | D | 4 | 1167 | 34 | Robo-AO Kepler planetary candidate survey. II. Adaptive optics imaging of 969 Kepler exoplanet candidate host stars. | BARANEC C., ZIEGLER C., LAW N.M., 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. | ||
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 | 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 | 2 | 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. | ||
2017NewA...55....1H | 16 | D | 1 | 146 | 2 | Multiple planetary systems: properties of the current sample. | HOBSON M.J. and GOMEZ M. | ||
2018ApJS..234....9O | 16 | D | 1 | 436 | 14 | A spectral approach to transit timing variations. | OFIR A., XIE J.-W., JIANG C.-F., 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. | ||
2019AJ....157..143B | 17 | D | 1 | 423 | 5 | Re-evaluating small long-period confirmed planets from Kepler. | BURKE C.J., MULLALLY F., THOMPSON S.E., 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. | ||
2020ApJ...890...23L | 17 | D | 2 | 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. | ||
2020MNRAS.497.4091M | 43 | X | 1 | 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. |