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Kepler-109 , the SIMBAD biblio

Kepler-109 , the SIMBAD biblio (65 results) C.D.S. - SIMBAD4 rel 1.7 - 2021.03.11CET08:28:51

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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
2019A&A...622A.130B 18       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.
2019AJ....157...52B viz 18       D               1 88 ~ An excess of Jupiter analogs in super-Earth systems. BRYAN M.L., KNUTSON H.A., LEE E.J., et al.
2019ApJ...875...29M 18       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.
2019MNRAS.482.4146D 251     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.
2018AJ....156..292T viz 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.
2018ApJ...855..115B viz 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.
2018ApJ...861..149F viz 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.
2018ApJ...866...99B viz 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.
2018ApJS..237...38B viz 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.
2017A&A...603A..30S viz 17       D               4 2500 14 Observational evidence for two distinct giant planet populations. SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al.
2017AJ....153...71F viz 17       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.
2017AJ....154..107P viz 17       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 viz 17       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.
2017ApJ...844..102H viz 17       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.
2017MNRAS.465.2634A viz 17       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.
2017MNRAS.467..971B 17       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.
2017RAA....17....5W 17       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.
2016A&A...591A.118S viz 17       D               1 31388 40 The PASTEL catalogue: 2016 version. SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., et al.
2016A&A...594A..39F viz 17       D               2 51408 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....6W viz 17       D               4 3060 13 Calibration of LAMOST stellar surface gravities using the Kepler asteroseismic data. WANG L., WANG W., WU Y., et al.
2016AJ....152..187M viz 17       D               2 471 33 A super-solar metallicity for stars with hot rocky exoplanets. MULDERS G.D., PASCUCCI I., APAI D., et al.
2016ApJ...822...86M viz 17       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.
2016ApJ...830...31B 17       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.
2016ApJS..225....9H viz 17       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 viz 17       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.
2016MNRAS.456.2183D 18       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.
2016PASP..128i4502E 17       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.
2015ApJ...801....3M viz 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.
2015ApJ...807..170H viz 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 82           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 viz 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 viz 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 viz 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.
2015ApJS..217...16R viz 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 viz 83           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.
2015MNRAS.452.2127S viz 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.
2014AJ....147..119C viz 16       D               1 8005 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.
2014AJ....148...78D 81             C       1 111 35 Adaptive optics images. III. 87 Kepler objects of interest. DRESSING C.D., ADAMS E.R., DUPREE A.K., et al.
2014ApJ...783....4W viz 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 viz 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.
2014ApJ...788L...9B viz 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.
2014ApJS..210...19B viz 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 viz 627       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.
2014MNRAS.444.2525C 17       D               1 95 172 Improving PARSEC models for very low mass stars. CHEN Y., GIRARDI L., BRESSAN A., et al.
2013ApJ...763...41C viz 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 viz 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 viz 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 viz 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 viz 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 viz 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.
2012A&A...547A..36A viz 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.
2012AJ....144...42A viz 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...752...53L 16       D               1 320 18 Debris disks in Kepler exoplanet systems. LAWLER S.M. and GLADMAN B.
2012ApJ...756..185F viz 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 viz 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.
2012ApJS..199...24T viz 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.
2012MNRAS.420L..23V viz 16       D               1 94 22 Identifying non-resonant Kepler planetary systems. VERAS D. and FORD E.B.
2012Natur.486..375B viz 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.
2011ApJ...736...19B viz 16       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 viz 16       D               2 997 198 On the low false positive probabilities of Kepler planet candidates. MORTON T.D. and JOHNSON J.A.
2011ApJ...742L..19M viz 16       D               1 185 37 Compositions of hot super-Earth atmospheres: exploring Kepler candidates. MIGUEL Y., KALTENEGGER L., FEGLEY B., et al.
2011ApJS..197....2F viz 16       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 viz 17       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.

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2021.03.11-08:28:52

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