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Kepler-396 , the SIMBAD biblio (61 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST12:07:17 |
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 |
---|---|---|---|---|---|---|---|---|---|
2011A&A...529A..89D | 15 | D | 1 | 3298 | 98 | Global stellar variability study in the field-of-view of the Kepler satellite. | DEBOSSCHER J., BLOMME J., AERTS C., et al. | ||
2013MNRAS.429.2001H | 55 | D | X | 2 | 140 | 33 | 150 new transiting planet candidates from Kepler Q1-Q6 data. | HUANG X., BAKOS G.A. and HARTMAN J.D. | |
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 | 289 | D | X C | 7 | 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. | |
2013ApJ...778..110M | 725 | K A | X C | 18 | 23 | 0 | Eight planets in four multi-planet systems via transit timing variations in 1350 days. | MING Y., LIU H.-G., HUI Z., et al. | |
2013MNRAS.436.1883W | 16 | D | 1 | 961 | 136 | Rotation periods, variability properties and ages for Kepler exoplanet candidate host stars. | WALKOWICZ L.M. and BASRI G.S. | ||
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. | ||
2014ApJS..210...25X | 158 | A | D | X C | 4 | 17 | 67 | Transit timing variation of near-resonance planetary pairs. II. Confirmation of 30 planets in 15 multiple-planet systems. | XIE J.-W. |
2014MNRAS.437.3473A | 16 | D | 1 | 2614 | 45 | A catalogue of temperatures for Kepler eclipsing binary stars. | ARMSTRONG D.J., GOMEZ MAQUEO CHEW Y., FAEDI F., et al. | ||
2014ApJ...783....4W | 16 | 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. | ||
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. | ||
2014MNRAS.440.1753B | 55 | D | X | 2 | 32 | 4 | Stability boundaries for resonant migrating planet pairs. | BODMAN E.H.L. and QUILLEN A.C. | |
2014AJ....148...78D | 16 | D | 3 | 111 | 35 | Adaptive optics images. III. 87 Kepler objects of interest. | DRESSING C.D., ADAMS E.R., DUPREE A.K., 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...806..248W | 135 | D | X | 4 | 143 | 44 | Influence of stellar multiplicity on planet formation. III. Adaptive optics imaging of Kepler stars with gas giant planets. | WANG J., FISCHER D.A., HORCH E.P., et al. | |
2015ApJ...807..170H | 16 | D | 2 | 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...813..100O | 16 | D | 1 | 327 | 7 | Deep GALEX UV survey of the Kepler field. I. Point source catalog. | OLMEDO M., LLOYD J., MAMAJEK E.E., et al. | ||
2015ApJ...813..130W | 16 | D | 3 | 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. | ||
2015MNRAS.453.4089S | 16 | D | 1 | 103 | 3 | Tides alone cannot explain Kepler planets close to 2:1 MMR. | SILBURT A. and REIN H. | ||
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....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 | 5 | 2132 | 124 | Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set. | HOLCZER T., MAZEH T., NACHMANI G., et al. | ||
2016ApJS..225...32B | 16 | D | 1 | 1473 | 266 | Spectral properties of cool stars: extended abundance analysis of 1,617 planet-search stars. | BREWER J.M., FISCHER D.A., VALENTI J.A., et al. | ||
2016AJ....152..181H | 16 | D | 1 | 9279 | 22 | SETI observations of exoplanets with the Allen Telescope Array. | HARP G.R., RICHARDS J., TARTER J.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. | ||
2017AJ....153..117H | 16 | D | 1 | 170 | 51 | 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 | 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...66F | 16 | D | 4 | 90 | 6 | The densities of planets in multiple stellar systems. | FURLAN E. and HOWELL S.B. | ||
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. | ||
2018ApJS..234....9O | 16 | D | 2 | 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. | ||
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 | 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. | ||
2019ApJ...876...58N | 101 | D | C | 5 | 74 | 111 | Do Kepler superflare stars really include slowly rotating Sun-like stars?-Results using APO 3.5 m telescope spectroscopic observations and Gaia-DR2 data. | NOTSU Y., MAEHARA H., HONDA S., et al. | |
2019ApJ...879...69T | 17 | D | 1 | 222609 | 141 | The Payne: self-consistent ab initio fitting of stellar spectra. | TING Y.-S., CONROY C., RIX H.-W., 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. | ||
2020AJ....159..194V | 17 | D | 4 | 288 | ~ | A statistical search for star-planet interaction in the ultraviolet using GALEX. | VISWANATH G., NARANG M., MANOJ P., et al. | ||
2020A&A...636A..85S | 17 | D | 1 | 3696 | ~ | Derivation of parameters for 3748 FGK stars using H-band spectra from APOGEE Data Release 14. | SARMENTO P., DELGADO MENA E., ROJAS-AYALA B., et al. | ||
2020ApJ...898..173D | 17 | D | 1 | 194 | 11 | Rotation of solar analogs crossmatching Kepler and Gaia DR2. | DO NASCIMENTO J.-D.Jr, DE ALMEIDA L., VELLOSO E.N., et al. | ||
2020AJ....160..108B | 17 | D | 2 | 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 | 17 | D | 1 | 365761 | 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. | ||
2021ApJ...909..115C | 17 | D | 1 | 2175 | 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. | ||
2021MNRAS.503.4092B | 435 | A | D | X C | 10 | 124 | ~ | Revisiting the Kepler field with TESS: Improved ephemerides using TESS 2 min data. | BATTLEY M.P., KUNIMOTO M., ARMSTRONG D.J., et al. |
2021AJ....161..246J | 44 | X | 1 | 204 | 12 | Following up the Kepler field: masses of targets for transit timing and atmospheric characterization. | JONTOF-HUTTER D., WOLFGANG A., FORD E.B., et al. | ||
2021AJ....162...98B | 17 | D | 1 | 2175 | ~ | Seeking echoes of circumstellar disks in Kepler light curves. | BROMLEY B.C., LEONARD A., QUINTANILLA A., 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...91J | 18 | D | 1 | 248 | ~ | Physical properties and impact parameter variations of Kepler planets from analytic light-curve modeling. | JUDKOVSKY Y., OFIR A. and AHARONSON O. | ||
2022AJ....163..128W | 18 | 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....164...42J | 986 | A | D | S X C | 21 | 79 | 3 | TESS Observations of Kepler Systems with Transit Timing Variations. | JONTOF-HUTTER D., DALBA P.A. and LIVINGSTON J.H. |
2022ApJS..261...26S | 18 | D | 9 | 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. | ||
2023ApJ...946...61L | 93 | X | 2 | 39 | ~ | 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. |