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| Kepler-907 , the SIMBAD biblio (59 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST21:24:06 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
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. | ||
|
2013ApJS..204...24B |
15 | 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..127H |
15 | D | 1 | 189 | 246 | Fundamental properties of Kepler planet-candidate host stars using asteroseismology. | HUBER D., CHAPLIN W.J., CHRISTENSEN-DALSGAARD J., et al. | ||
| 2013AJ....145..151L | 38 | X | 1 | 12 | 19 | Planet hunters: new Kepler planet candidates from analysis of quarter 2. | LINTOTT C.J., SCHWAMB M.E., BARCLAY T., et al. | ||
|
2013ApJ...771..107E |
15 | D | 1 | 756 | 47 | Spectroscopy of faint Kepler mission exoplanet candidate host stars. | EVERETT M.E., HOWELL S.B., SILVA D.R., et al. | ||
|
2013ApJ...775L..11M |
15 | 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 |
15 | 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. | ||
|
2014ApJS..210...19B |
15 | 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. | ||
|
2014ApJ...783....4W |
15 | 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. | ||
|
2014AJ....147..119C |
15 | D | 1 | 8013 | 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...788L...9B |
15 | D | 1 | 293 | 26 | Larger planet radii inferred from stellar "flicker" brightness variations of bright planet-host stars. | BASTIEN F.A., STASSUN K.G. and PEPPER J. | ||
|
2014ApJ...791...35L |
15 | D | 1 | 800 | 137 | Robotic laser adaptive optics imaging of 715 Kepler exoplanet candidates using Robo-AO. | LAW N.M., MORTON T., BARANEC C., et al. | ||
| 2015AJ....149...18K | 133 | D | X C | 3 | 97 | 61 | Detection of stars within : ∼0.8 in of Kepler objects of interest. | KOLBL R., MARCY G.W., ISAACSON H., 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 | 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...808..187B |
16 | D | 1 | 540 | 73 | The metallicities of stars with and without transiting planets. | BUCHHAVE L.A. and LATHAM D.W. | ||
| 2015AJ....150..144T | 952 | D | X C | 24 | 12 | 13 | A comparison of spectroscopic versus imaging techniques for detecting close companions to Kepler objects of interest. | TESKE J.K., EVERETT M.E., HIRSCH L., et al. | |
|
2015ApJ...813..130W |
16 | D | 4 | 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. | ||
|
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. | ||
|
2016AJ....151...68K |
16 | D | 1 | 2915 | 316 | Kepler eclipsing binary stars. VII. The catalog of eclipsing binaries found in the entire Kepler data set. | KIRK B., CONROY K., PRSA A., 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. | ||
|
2016AJ....152....8K |
212 | D | X C | 5 | 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 | 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. | ||
|
2016A&A...594A..39F |
16 | D | 1 | 51408 | 86 | Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra. | FRASCA A., MOLENDA-ZAKOWICZ J., DE CAT P., et al. | ||
|
2016AJ....152..187M |
16 | D | 2 | 471 | 74 | A super-solar metallicity for stars with hot rocky exoplanets. | MULDERS G.D., PASCUCCI I., APAI D., 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. | ||
|
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. | ||
| 2017RAA....17....5W | 16 | D | 2 | 180 | 4 | Stellar parameters of main sequence turn-off star candidates observed with LAMOST and Kepler. | WU Y.-Q., XIANG M.-S., ZHANG X.-F., 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..250L |
16 | D | 1 | 2281 | 72 | Tidal synchronization and differential rotation of Kepler eclipsing binaries. | LURIE J.C., VYHMEISTER K., HAWLEY S.L., et al. | ||
|
2018AJ....155...68W |
16 | D | 1 | 509 | 18 | Elemental abundances of Kepler Objects of Interest in APOGEE. I. Two distinct orbital period regimes inferred from host star iron abundances. | WILSON R.F., TESKE J., MAJEWSKI S.R., et al. | ||
|
2018ApJ...861..149F |
16 | D | 2 | 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. | ||
| 2019AJ....157...61V | 58 | D | X | 2 | 110 | 147 | The orbital eccentricity of small planet systems. | VAN EYLEN V., ALBRECHT S., HUANG X., et al. | |
|
2019ApJ...879...69T |
16 | D | 1 | 222610 | 141 | The Payne: self-consistent ab initio fitting of stellar spectra. | TING Y.-S., CONROY C., RIX H.-W., et al. | ||
|
2019ApJS..244...43Z |
16 | D | 1 | 1328 | 22 | Unbiased distribution of binary parameters from LAMOST and Kepler observations. | ZHANG J., QIAN S.-B., WU Y., et al. | ||
|
2020ApJ...890...23L |
16 | D | 3 | 4936 | 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..120J |
16 | D | 1 | 365763 | 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. | ||
|
2021AJ....161...21C |
167 | X | 4 | 17 | ~ | Identifying bound stellar companions to Kepler exoplanet host stars using speckle imaging. | COLTON N.M., HORCH E.P., EVERETT M.E., et al. | ||
| 2021MNRAS.504.5327A | 17 | D | 1 | 7000 | 19 | Exoplanet validation with machine learning: 50 new validated Kepler planets. | ARMSTRONG D.J., GAMPER J. and DAMOULAS T. | ||
|
2021AJ....162...98B |
17 | D | 2 | 2175 | ~ | Seeking echoes of circumstellar disks in Kepler light curves. | BROMLEY B.C., LEONARD A., QUINTANILLA A., et al. | ||
|
2022AJ....163..152S |
17 | D | 1 | 583193 | 11 | APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. | SPRAGUE D., CULHANE C., KOUNKEL M., et al. | ||
|
2022ApJS..259...35A |
17 | D | 1 | 611005 | 320 | The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. | ABDURRO'UF, ACCETTA K., AERTS C., et al. | ||
|
2022AJ....164...60S |
17 | D | 1 | 854 | 2 | Galactic Chemical Evolution of Exoplanet Hosting Stars: Are High-mass Planetary Systems Young? | SWASTIK C., BANYAL R.K., NARANG M., et al. | ||
|
2022ApJS..261...26S |
17 | 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. | ||
|
2022A&A...663A...4S |
17 | D | 1 | 14206 | 7 | Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys. | SOUBIRAN C., BROUILLET N. and CASAMIQUELA L. | ||
|
2023AJ....165..177S |
17 | D | 4 | 131 | ~ | Revising Properties of Planet-Host Binary Systems. III. There Is No Observed Radius Gap for Kepler Planets in Binary Star Systems. | SULLIVAN K., KRAUS A.L., HUBER D., et al. | ||
| 2023AJ....166..166L | 104 | D | C | 5 | 36 | ~ | Visual Orbits and Alignments of Planet-hosting Binary Systems. | LESTER K.V., HOWELL S.B., MATSON R.A., et al. | |
|
2024AJ....167..117D |
448 | A | D | X C | 10 | 29 | ~ | Observations with the Differential Speckle Survey Instrument. XI. First Year of Observations from Apache Point Observatory. | DAVIDSON J.W.Jr, HORCH E.P., MAJEWSKI S.R., et al. |
|
2024A&A...685A..62I |
18 | D | 1 | 2906 | ~ | Automated eccentricity measurement from raw eclipsing binary light curves with intrinsic variability. | IJSPEERT L.W., TKACHENKO A., JOHNSTON C., et al. | ||
|
2024AJ....168..129S |
18 | D | 2 | 350 | ~ | Revising Properties of Planet-Host Binary Systems. IV. The Radius Distribution of Small Planets in Binary Star Systems Is Dependent on Stellar Separation. | SULLIVAN K., KRAUS A.L., BERGER T.A., et al. | ||
| 2024MNRAS.534..575E | 18 | D | 1 | 51 | ~ | Orbital architectures of planet-hosting binaries - III. Testing mutual inclinations of stellar and planetary orbits in triple-star systems. | EVANS E.L., DUPUY T.J., SULLIVAN K., et al. | ||
|
2024A&A...689A.250C |
18 | D | 3 | 3075 | ~ | Mapping the exo-Neptunian landscape A ridge between the desert and savanna. | CASTRO-GONZALEZ A., BOURRIER V., LILLO-BOX J., et al. | ||
|
2024A&A...691A..53S |
18 | D | 1 | 4078 | ~ | SWEET-Cat: A view on the planetary mass-radius relation. | SOUSA S.G., ADIBEKYAN V., DELGADO-MENA E., et al. | ||
|
2025A&A...699A.100D |
19 | D | 1 | 2580 | ~ | The Gaia spectroscopic catalogue of exoplanets and host stars. | DE LAVERNY P., LIGI R., CRIDA A., et al. | ||
| 2025AJ....170..212S | 19 | D | 2 | 797 | ~ | A Homogeneous Catalog of Oscillating Solar-type Stars Observed by the Kepler Mission and a New Amplitude Scaling Relation Including Chromospheric Activity. | SAYEED M., HUBER D., CHONTOS A., et al. |