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Kepler-109 , the SIMBAD biblio (72 results) | C.D.S. - SIMBAD4 rel 1.8 - 2023.03.27CEST09:47:05 |
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 |
---|---|---|---|---|---|---|---|---|---|
2011ApJ...736...19B ![]() |
15 | D | 1 | 1507 | 742 | Characteristics of planetary candidates observed by Kepler. II. Analysis of the first four months of data. | BORUCKI W.J., KOCH D.G., BASRI G., et al. | ||
2011ApJ...738..170M ![]() |
15 | D | 2 | 997 | 198 | On the low false positive probabilities of Kepler planet candidates. | MORTON T.D. and JOHNSON J.A. | ||
2011ApJS..197....2F ![]() |
15 | D | 2 | 980 | 66 | Transit timing observations from Kepler. I. Statistical analysis of the first four months. | FORD E.B., ROWE J.F., FABRYCKY D.C., et al. | ||
2011ApJS..197....8L ![]() |
16 | D | 1 | 177 | 389 | Architecture and dynamics of Kepler's candidate multiple transiting planet systems. | LISSAUER J.J., RAGOZZINE D., FABRYCKY D.C., et al. | ||
2011ApJ...742L..19M ![]() |
15 | D | 1 | 185 | 37 | Compositions of hot super-Earth atmospheres: exploring Kepler candidates. | MIGUEL Y., KALTENEGGER L., FEGLEY B., et al. | ||
2012MNRAS.420L..23V ![]() |
16 | D | 1 | 94 | 22 | Identifying non-resonant Kepler planetary systems. | VERAS D. and FORD E.B. | ||
2012ApJS..199...24T ![]() |
16 | D | 1 | 5393 | 51 | 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...752...53L | 16 | D | 1 | 320 | 18 | Debris disks in Kepler exoplanet systems. | LAWLER S.M. and GLADMAN B. | ||
2012Natur.486..375B ![]() |
16 | D | 1 | 378 | 334 | An abundance of small exoplanets around stars with a wide range of metallicities. | BUCHHAVE L.A., LATHAM D.W., JOHANSEN A., et al. | ||
2012AJ....144...42A ![]() |
16 | D | 5 | 90 | 84 | Adaptive optics images of Kepler Objects of Interest. | ADAMS E.R., CIARDI D.R., DUPREE A.K., et al. | ||
2012ApJ...756..185F ![]() |
16 | D | 2 | 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. | ||
2012ApJ...756..186S ![]() |
16 | D | 2 | 811 | 35 | Transit timing observations from Kepler. VI. Potentially interesting candidate systems from fourier-based statistical tests. | STEFFEN J.H., FORD E.B., ROWE J.F., et al. | ||
2012A&A...547A..36A ![]() |
16 | D | 1 | 87 | 61 | Exploring the α-enhancement of metal-poor planet-hosting stars. The Kepler and HARPS samples. | ADIBEKYAN V.Zh., DELGADO MENA E., SOUSA S.G., et al. | ||
2013ApJ...763...41C ![]() |
16 | D | 1 | 97 | 40 | On the relative sizes of planets within Kepler multiple-candidate systems. | CIARDI D.R., FABRYCKY D.C., FORD E.B., et al. | ||
2013ApJ...767..127H ![]() |
16 | D | 1 | 189 | 177 | Fundamental properties of Kepler planet-candidate host stars using asteroseismology. | HUBER D., CHAPLIN W.J., CHRISTENSEN-DALSGAARD J., et al. | ||
2013ApJ...770...69P ![]() |
16 | D | 1 | 245 | 158 | A plateau in the planet population below twice the size of Earth. | PETIGURA E.A., MARCY G.W. and HOWARD A.W. | ||
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 | 107 | 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 | 2 | 1518 | 92 | 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 ![]() |
16 | D | 2 | 5860 | 162 | 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...20M ![]() |
613 | D | S X C | 14 | 94 | 251 | Masses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planets. | MARCY G.W., ISAACSON H., HOWARD A.W., et al. | |
2014ApJ...783....4W ![]() |
16 | D | 1 | 487 | 55 | 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 | 227 | 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 | 8008 | 55 | 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 ![]() |
16 | 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..111W | 16 | D | 5 | 56 | 53 | Influence of stellar multiplicity on planet formation. II. Planets are less common in multiple-star systems with separations smaller than 1500 AU. | WANG J., FISCHER D.A., XIE J.-W., et al. | ||
2014AJ....148...78D | 79 | C | 1 | 111 | 35 | Adaptive optics images. III. 87 Kepler objects of interest. | DRESSING C.D., ADAMS E.R., DUPREE A.K., et al. | ||
2014MNRAS.444.2525C | 16 | D | 1 | 95 | 172 | Improving PARSEC models for very low mass stars. | CHEN Y., GIRARDI L., BRESSAN A., et al. | ||
2015ApJ...801....3M ![]() |
16 | D | 1 | 3357 | 52 | 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 | 84 | Planetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months). | ROWE J.F., COUGHLIN J.L., ANTOCI V., et al. | ||
2015ApJS..217...18S ![]() |
81 | X | 2 | 16 | 16 | Detection of potential transit signals in 17 quarters of Kepler mission data. | SEADER S., JENKINS J.M., TENENBAUM 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...808..126V | 80 | X | 2 | 105 | 85 | Eccentricity from transit photometry: small planets in Kepler multi-planet systems have low eccentricities. | VAN EYLEN V. and ALBRECHT S. | ||
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 | 2 | 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 | 46 | An increase in the mass of planetary systems around lower-mass stars. | MULDERS G.D., PASCUCCI I. and APAI D. | ||
2015MNRAS.452.2127S ![]() |
19 | D | 3 | 35 | 134 | Ages and fundamental properties of Kepler exoplanet host stars from asteroseismology. | SILVA AGUIRRE V., DAVIES G.R., BASU S., et al. | ||
2016MNRAS.456.2183D | 17 | D | 3 | 35 | 45 | Oscillation frequencies for 35 Kepler solar-type planet-hosting stars using Bayesian techniques and machine learning. | DAVIES G.R., SILVA AGUIRRE V., BEDDING T.R., et al. | ||
2016ApJ...822...86M ![]() |
16 | D | 1 | 6129 | 192 | 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....6W ![]() |
16 | D | 4 | 3060 | 13 | Calibration of LAMOST stellar surface gravities using the Kepler asteroseismic data. | WANG L., WANG W., WU Y., et al. | ||
2016A&A...591A.118S ![]() |
16 | D | 1 | 31385 | 40 | The PASTEL catalogue: 2016 version. | SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., et al. | ||
2016ApJS..225....9H ![]() |
16 | D | 4 | 2132 | 33 | 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 | 68 | 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. | ||
2016ApJ...830...31B | 16 | D | 2 | 37 | 17 | Fundamental parameters of main-sequence stars in an instant with machine learning. | BELLINGER E.P., ANGELOU G.C., HEKKER S., et al. | ||
2016A&A...594A..39F ![]() |
16 | D | 2 | 51409 | 21 | 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 | 33 | A super-solar metallicity for stars with hot rocky exoplanets. | MULDERS G.D., PASCUCCI I., APAI D., et al. | ||
2017AJ....153...71F ![]() |
16 | D | 1 | 3575 | 46 | 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. | ||
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 | 9 | 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..128i4502E | 16 | D | 1 | 35 | 16 | Kea: a new tool to obtain stellar parameters from low to moderate signal-to-noise and high-resolution echelle spectra. | ENDL M. and COCHRAN W.D. | ||
2017MNRAS.467..971B | 16 | D | 1 | 56 | 21 | ZASPE: a code to measure stellar atmospheric parameters and their covariance from spectra. | BRAHM R., JORDAN A., HARTMAN J., et al. | ||
2017ApJ...844..102H ![]() |
16 | D | 1 | 2236 | 41 | Asteroseismology and Gaia: testing scaling relations using 2200 Kepler stars with TGAS parallaxes. | HUBER D., ZINN J., BOJSEN-HANSEN M., et al. | ||
2017AJ....154..107P ![]() |
16 | D | 1 | 1306 | 56 | 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 | 46 | 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. | ||
2017A&A...603A..30S ![]() |
16 | D | 4 | 2500 | 14 | Observational evidence for two distinct giant planet populations. | SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al. | ||
2018ApJ...855..115B ![]() |
17 | D | 1 | 1305 | 2 | 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 ![]() |
17 | D | 1 | 1073 | 17 | Inferring probabilistic stellar rotation periods using Gaussian processes. | ANGUS R., MORTON T., AIGRAIN S., et al. | ||
2018ApJ...861..149F ![]() |
17 | D | 1 | 2261 | ~ | 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 ![]() |
17 | D | 1 | 1111 | ~ | Spectral properties of cool stars: extended abundance analysis of Kepler Objects of Interest. | BREWER J.M. and FISCHER D.A. | ||
2018MNRAS.479..391K | 17 | D | 1 | 101 | 1 | Reliability of stellar inclination estimated from asteroseismology: analytical criteria, mock simulations, and Kepler data analysis. | KAMIAKA S., BENOMAR O. and SUTO Y. | ||
2018ApJ...866...99B ![]() |
17 | D | 1 | 7129 | 101 | 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 ![]() |
17 | D | 1 | 647 | ~ | The effects of stellar companions on the observed transiting exoplanet radius distribution. | TESKE J.K., CIARDI D.R., HOWELL S.B., et al. | ||
2019MNRAS.482.4146D | 238 | A | X C F | 4 | 19 | ~ | Hidden planetary friends: on the stability of two-planet systems in the presence of a distant, inclined companion. | DENHAM P., NAOZ S., HOANG B.-M., et al. | |
2019AJ....157...52B ![]() |
17 | D | 1 | 88 | ~ | An excess of Jupiter analogs in super-Earth systems. | BRYAN M.L., KNUTSON H.A., LEE E.J., et al. | ||
2019A&A...622A.130B | 17 | D | 2 | 97 | ~ | Stellar ages, masses, and radii from asteroseismic modeling are robust to systematic errors in spectroscopy. | BELLINGER E.P., HEKKER S., ANGELOU G.C., et al. | ||
2019ApJ...875...29M ![]() |
17 | D | 1 | 2918 | ~ | 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. | ||
2020ApJ...890...23L ![]() |
17 | D | 2 | 4935 | ~ | 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 | 2 | 6855 | ~ | 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. | ||
2021ApJ...909..115C ![]() |
18 | D | 1 | 2175 | ~ | 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. | ||
2021NatAs...5..707H ![]() |
18 | D | 1 | 95 | ~ | Weakened magnetic braking supported by asteroseismic rotation rates of Kepler dwarfs. | HALL O.J., DAVIES G.R., VAN SADERS J., et al. | ||
2021ApJ...919..138T | 18 | D | 1 | 531 | ~ | Further evidence for tidal spin-up of hot Jupiter host stars. | TEJADA AREVALO R.A., WINN J.N. and ANDERSON K.R. | ||
2022ApJ...941..175L | 345 | D | S X | 7 | 99 | ~ | Meta-analysis of Photometric and Asteroseismic Measurements of Stellar Rotation Periods: The Lomb-Scargle Periodogram, Autocorrelation Function, and Wavelet and Rotational Splitting Analysis for 92 Kepler Asteroseismic Targets. | LU Y., BENOMAR O., KAMIAKA S., et al. |
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