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Kepler-974 , the SIMBAD biblio (51 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST19:38:40 |
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 | 15 | D | 1 | 5394 | 66 | Detection of potential transit signals in the first three quarters of Kepler mission data. | TENENBAUM P., CHRISTIANSEN J.L., JENKINS J.M., et al. | ||
2012ApJ...756..185F | 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. | ||
2012A&A...548A..44C | 15 | D | 1 | 137 | 22 | A study of the performance of the transit detection tool DST in space-based surveys. Application of the CoRoT pipeline to Kepler data. | CABRERA J., CSIZMADIA Sz., ERIKSON A., et al. | ||
2013ApJS..204...24B | 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...95D | 17 | D | 2 | 164 | 581 | The occurrence rate of small planets around small stars. | DRESSING C.D. and CHARBONNEAU D. | ||
2013ApJ...770...43M | 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...773L..15R | 404 | K | X C | 9 | 2 | 57 |
The roche limit for close-orbiting planets: minimum density, composition constraints, and application to the 4.2 hr planet KOI 1843.03. |
RAPPAPORT S., SANCHIS-OJEDA R., ROGERS L.A., et al. | |
2013A&A...555A..58O | 234 | A | D | S X | 6 | 171 | 53 | An independent planet search in the Kepler dataset. I. One hundred new candidates and revised Kepler objects of interest. | OFIR A. and DREIZLER S. |
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...774...54S | 45 | X | 1 | 10 | 122 | Transits and occultations of an earth-sized planet in an 8.5 hr orbit. | SANCHIS-OJEDA R., RAPPAPORT S., WINN J.N., et al. | ||
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. | ||
2013ApJS..208...16M | 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. | ||
2013ApJ...779..165J | 523 | D | S X C | 12 | 37 | 20 | A survey for very short-period planets in the Kepler data. | JACKSON B., STARK C.C., ADAMS E.R., et al. | |
2013ApJ...779..188M | 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 | 16 | D | 1 | 24132 | 291 | Rotation and differential rotation of active Kepler stars. | REINHOLD T., REINERS A. and BASRI G. | ||
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. | ||
2014ApJ...787...47S | 16 | D | 1 | 222 | 160 | A study of the shortest-period planets found with Kepler. | SANCHIS-OJEDA R., RAPPAPORT S., WINN J.N., et al. | ||
2014ApJS..213....5M | 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...800...85N | 16 | D | 2 | 525 | 94 | An empirical calibration to estimate cool dwarf fundamental parameters from H-band spectra. | NEWTON E.R., CHARBONNEAU D., IRWIN J., 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. | ||
2015ApJ...801...18M | 40 | X | 1 | 31 | 39 | Kepler-445, Kepler-446 and the occurrence of compact multiples orbiting mid-M dwarf stars. | MUIRHEAD P.S., MANN A.W., VANDERBURG 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. | ||
2015ApJS..218...26S | 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 | 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...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. | ||
2016MNRAS.457.1851R | 96 | D | F | 3 | 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 | 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. | ||
2016MNRAS.457.2877G | 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 | 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. | ||
2016AJ....152...47A | 40 | X | 1 | 130 | 29 | Ultra-short-period planets in K2 superpig results for campaigns 0-5. | ADAMS E.R., JACKSON B. and ENDL M. | ||
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. | ||
2016MNRAS.461.1413V | 65 | A | X | 2 | 6 | 9 | Dynamical mass and multiplicity constraints on co-orbital bodies around stars. | VERAS D., MARSH T.R. and GANSICKE B.T. | |
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. | ||
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. | ||
2018AJ....155..161Z | 41 | X | 1 | 1274 | 24 | Robo-AO Kepler survey. IV. The effect of nearby stars on 3857 planetary candidate systems. | ZIEGLER C., LAW N.M., BARANEC C., 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. | ||
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. | ||
2020ApJ...890L..31L | 17 | D | 1 | 85 | ~ | Mutual inclination excitation by stellar oblateness. | LI G., DAI F. and BECKER J. | ||
2020ApJ...894....8P | 128 | X | 3 | 11 | ~ | Tidally distorted, iron-enhanced exoplanets closely orbiting their stars. | PRICE E.M. and ROGERS L.A. | ||
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. | ||
2020AJ....160..253L | 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. | ||
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. | ||
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. | ||
2022MNRAS.512..648D | 45 | X | 1 | 40 | 9 | Orbital architectures of planet-hosting binaries - II. Low mutual inclinations between planetary and stellar orbits. | DUPUY T.J., KRAUS A.L., KRATTER K.M., et al. | ||
2022MNRAS.513.2732S | 90 | C | 1 | 51 | 1 | fBLS - a fast-folding BLS algorithm. | SHAHAF S., ZACKAY B., MAZEH T., et al. | ||
2022ApJS..261...26S | 18 | D | 3 | 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. |