Kepler-1229 , the SIMBAD biblio

Kepler-1229 , the SIMBAD biblio (51 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST15:25:42

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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
2012ApJ...756..185F viz 15       D               1 1856 44 Transit timing observations from Kepler. V. Transit timing variation candidates in the first sixteen months from polynomial models. FORD E.B., RAGOZZINE D., ROWE J.F., et al.
2013ApJS..204...24B viz 16       D               1 3274 922 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...767...94S viz 16       D               1 267 74 A 1.1-1.9 GHz SETI survey of the Kepler field. I. A search for narrow-band emission from select targets. SIEMION A.P.V., DEMOREST P., KORPELA E., et al.
2013ApJ...767...95D viz 17       D               1 164 581 The occurrence rate of small planets around small stars. DRESSING C.D. and CHARBONNEAU D.
2013ApJ...770...43M viz 16       D               1 202 41 Testing the metal of late-type Kepler planet hosts with iron-clad methods. MANN A.W., GAIDOS E., KRAUS A., et al.
2013ApJ...770...90G viz 16       D               1 74 60 Candidate planets in the habitable zones of Kepler stars. GAIDOS E.
2013ApJ...775L..11M viz 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.
2013ApJS..208...16M viz 16       D               1 1518 139 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 viz 16       D               1 961 136 Rotation periods, variability properties and ages for Kepler exoplanet candidate host stars. WALKOWICZ L.M. and BASRI G.S.
2013ApJ...779..188M viz 16       D               1 342 155 Spectro-thermometry of M dwarfs and their candidate planets: too hot, too cool, or just right? MANN A.W., GAIDOS E. and ANSDELL M.
2013A&A...560A...4R viz 16       D               1 24132 291 Rotation and differential rotation of active Kepler stars. REINHOLD T., REINERS A. and BASRI G.
2014ApJS..210...19B viz 16       D               1 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.
2014AJ....147..119C viz 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.
2014ApJ...788..114R viz 16       D               1 184 17 M-dwarf rapid rotators and the detection of relatively young multiple M-star systems. RAPPAPORT S., SWIFT J., LEVINE A., et al.
2014ApJS..213....5M viz 16       D               1 111 51 Characterizing the cool KOIs. VI. H- and K-band spectra of Kepler M dwarf planet-candidate hosts. MUIRHEAD P.S., BECKER J., FEIDEN G.A., et al.
2015ApJ...801....3M viz 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 viz 56       D     X         2 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.
2015ApJS..218...26S viz 16       D               1 275 13 Characterizing the cool KOIs. VIII. Parameters of the planets orbiting Kepler's coolest dwarfs. SWIFT J.J., MONTET B.T., VANDERBURG A., et al.
2015ApJ...807..170H viz 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...807...45D viz 56       D     X         2 2707 726 The occurrence of potentially habitable planets orbiting M dwarfs estimated from the full Kepler dataset and an empirical measurement of the detection sensitivity. DRESSING C.D. and CHARBONNEAU D.
2015ApJ...814...91B viz 16       D               1 524 24 Comparative habitability of transiting exoplanets. BARNES R., MEADOWS V.S. and EVANS N.
2015ApJ...814..130M viz 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.
2016MNRAS.457.1851R 177       D     X   F     4 95 3 Search for pulsations in M dwarfs in the Kepler short-cadence data base. RODRIGUEZ E., RODRIGUEZ-LOPEZ C., LOPEZ-GONZALEZ M.J., et al.
2016ApJ...822...86M viz 136       D     X C       3 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..224...12C viz 16       D               1 1110 211 Planetary candidates observed by Kepler VII. The first fully uniform catalog based on the entire 48-month data set (Q1-Q17 DR24). COUGHLIN J.L., MULLALLY F., THOMPSON S.E., et al.
2016MNRAS.457.2877G viz 16       D               1 4245 141 They are small worlds after all: revised properties of Kepler M dwarf stars and their planets. GAIDOS E., MANN A.W., KRAUS A.L., et al.
2016AJ....152....8K viz 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.
2016ApJS..225....9H viz 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.
2016ApJ...830....1K 44           X         1 30 122 A catalog of Kepler habitable zone exoplanet candidates. KANE S.R., HILL M.L., KASTING J.F., et al.
2017ApJ...834...92C 16       D               1 57 4 LAMOST observations of flaring M dwarfs in the Kepler field. CHANG H.-Y., SONG Y.-H., LUO A.-L., et al.
2017AJ....153...71F viz 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 viz 57       D     X         2 170 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 viz 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.
2017A&A...603A..30S viz 16       D               2 2500 58 Observational evidence for two distinct giant planet populations. SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al.
2017AJ....154..264T 16       D               7 51 17 Validation of small Kepler transiting planet candidates in or near the habitable zone. TORRES G., KANE S.R., ROWE J.F., et al.
2018ApJ...866...99B viz 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.
2019A&A...627A..49Z viz 90             C       1 16 98 The CARMENES search for exoplanets around M dwarfs. Two temperate Earth-mass planet candidates around Teegarden's Star. ZECHMEISTER M., DREIZLER S., RIBAS I., et al.
2019A&A...630A..52R 142       D     X         4 63 ~ Erosion of an exoplanetary atmosphere caused by stellar winds. RODRIGUEZ-MOZOS J.M. and MOYA A.
2020ApJ...890...23L viz 17       D               1 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..253L viz 17       D               1 3432 12 An increase in small-planet occurrence with metallicity for late-type dwarf stars in the Kepler field and its implications for planet formation. LU C.X., SCHLAUFMAN K.C. and CHENG S.
2021MNRAS.505.3329C 17       D               1 19 ~ Efficiency of the oxygenic photosynthesis on Earth-like planets in the habitable zone. COVONE G., IENCO R.M., CACCIAPUOTI L., et al.
2021AJ....162...98B viz 17       D               2 2175 ~ Seeking echoes of circumstellar disks in Kepler light curves. BROMLEY B.C., LEONARD A., QUINTANILLA A., et al.
2022ApJ...928...12D 45           X         1 12 7 The Contribution of M-dwarf Flares to the Thermal Escape of Potentially Habitable Planet Atmospheres. DO AMARAL L.N.R., BARNES R., SEGURA A., et al.
2022ApJS..261...26S viz 18       D               4 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.
2022AJ....164..138S 18       D               2 32 1 Revising Properties of Planet-Host Binary Systems. II. Apparent Near-Earth-analog Planets in Binaries Are Often Sub-Neptunes. SULLIVAN K. and KRAUS A.L.
2023A&A...670A..84K viz 47           X         1 38 5 The CARMENES search for exoplanets around M dwarfs Wolf 1069 b: Earth-mass planet in the habitable zone of a nearby, very low-mass star. KOSSAKOWSKI D., KURSTER M., TRIFONOV T., et al.
2023A&A...675A.114C 93               F     1 25 ~ Chasing extreme planetary architectures I. HD 196885 Ab, a super-Jupiter dancing with two stars? CHAUVIN G., VIDELA M., BEUST H., et al.
2023MNRAS.525.5168M 19       D               1 68 ~ Impact of M-dwarf stellar wind and photoevaporation on the atmospheric evolution of small planets. MODI A., ESTRELA R. and VALIO A.
2023ApJ...954L..50E 19       D               1 205 ~ Living with a Red Dwarf: The Rotation-Age Relationships of M Dwarfs. ENGLE S.G. and GUINAN E.F.
2023ApJ...956...29Q 19       D               1 40 ~ Prospects for Cryovolcanic Activity on Cold Ocean Planets. QUICK L.C., ROBERGE A., MENDOZA G.T., et al.
2023ApJ...959L...1H 47           X         1 12 ~ Separated Twins or Just Siblings? A Multiplanet System around an M Dwarf Including a Cool Sub-Neptune. HARRIS M., DRAGOMIR D., MIRELES I., et al.

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