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Kepler-455 , the SIMBAD biblio (25 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST09:19:06 |
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 |
---|---|---|---|---|---|---|---|---|---|
2013MNRAS.429.2001H | 16 | D | 1 | 140 | 33 | 150 new transiting planet candidates from Kepler Q1-Q6 data. | HUANG X., BAKOS G.A. and HARTMAN J.D. | ||
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...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...91B | 16 | D | 1 | 524 | 24 | Comparative habitability of transiting exoplanets. | BARNES R., MEADOWS V.S. and EVANS N. | ||
2015ApJ...814..130M | 16 | D | 1 | 2846 | 162 | An increase in the mass of planetary systems around lower-mass stars. | MULDERS G.D., PASCUCCI I. and APAI D. | ||
2015ApJ...815..127W | 175 | D | X | 5 | 59 | 64 | Planet hunters. VIII. Characterization of 41 long-period exoplanet candidates from Kepler archival data. | WANG J., FISCHER D.A., BARCLAY T., et al. | |
2016ApJ...822....2U | 177 | D | S C | 6 | 38 | 26 | Transiting planet candidates beyond the snow line detected by visual inspection of 7557 Kepler Objects of Interest. | UEHARA S., KAWAHARA H., MASUDA K., et al. | |
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. | ||
2016ApJS..225....9H | 16 | D | 2 | 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...66Z | 16 | D | 1 | 1663 | 45 | Robo-AO Kepler Planetary Candidate Survey. III. Adaptive optics imaging of 1629 Kepler exoplanet candidate host stars. | ZIEGLER C., LAW N.M., MORTON T., 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 | 1 | 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. | ||
2016PASP..128g4502M | 16 | D | 1 | 305 | 14 | Identifying false alarms in the Kepler planet candidate catalog. | MULLALLY F., COUGHLIN J.L., THOMPSON S.E., et al. | ||
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...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. | ||
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..259Z | 16 | D | 1 | 231 | 80 | Measuring the recoverability of close binaries in Gaia DR2 with the Robo-AO Kepler survey. | ZIEGLER C., LAW N.M., BARANEC C., et al. | ||
2019MNRAS.483...38D | 100 | D | C | 2 | 18 | 1 | Multicomponent power-density spectra of Kepler AGNs, an instrumental artefact or a physical origin? | DOBROTKA A., BEZAK P., REVALSKI M., et al. | |
2019AJ....157..218K | 17 | D | 2 | 142 | 26 | Transiting planets near the snow line from Kepler. I. Catalog. | KAWAHARA H. and MASUDA K. | ||
2020AJ....159...38M | 231 | D | X | 6 | 23 | 34 | Mutual orbital inclinations between cold Jupiters and inner super-Earths. | MASUDA K., WINN J.N. and KAWAHARA H. | |
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. | ||
2020AJ....160..108B | 17 | D | 1 | 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. |