KOI-1054 , the SIMBAD biblio

KOI-1054 , the SIMBAD biblio (30 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST18:48:01

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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
2011ApJ...736...19B viz 15       D               1 1507 867 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 15       D               1 997 230 On the low false positive probabilities of Kepler planet candidates. MORTON T.D. and JOHNSON J.A.
2011ApJS..197....2F viz 15       D               1 980 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.
2011ApJ...742L..19M viz 15       D               1 185 37 Compositions of hot super-Earth atmospheres: exploring Kepler candidates. MIGUEL Y., KALTENEGGER L., FEGLEY B., et al.
2012ApJ...752...53L 15       D               1 320 18 Debris disks in Kepler exoplanet systems. LAWLER S.M. and GLADMAN B.
2013ApJ...767..127H viz 16       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....146....9A 16       D               2 29 57 Adaptive optics images. II. 12 Kepler objects of interest and 15 confirmed transiting planets. ADAMS E.R., DUPREE A.K., KULESA C., et al.
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.
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.
2014PASP..126...34P 118           X         3 26 36 Investigation of Kepler Objects of Interest stellar parameters from observed transit durations. PLAVCHAN P., BILINSKI C. and CURRIE T.
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.
2015ApJS..217...16R viz 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...809....8B viz 16       D               1 112329 282 Terrestrial planet occurrence rates for the Kepler GK dwarf sample. BURKE C.J., CHRISTIANSEN J.L., MULLALLY F., et al.
2016AJ....152....8K viz 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.
2016MNRAS.460.3179W viz 16       D               1 77460 19 Distance and extinction determination for APOGEE stars with Bayesian method. WANG J., SHI J., PAN K., 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....154..107P viz 57       D     X         2 1306 226 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 16       D               1 3237 137 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.
2018ApJ...852...49H viz 16       D               1 1325 118 Disentangling the Galactic halo with APOGEE. I. Chemical and kinematical investigation of distinct metal-poor populations. HAYES C.R., MAJEWSKI S.R., SHETRONE M., et al.
2018AJ....155...68W viz 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...855..115B viz 16       D               1 1305 5 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 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.
2018ApJS..237...38B viz 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.
2019ApJ...872..137S viz 17       D               1 26099 39 Constraining metallicity-dependent mixing and extra mixing using [C/N] in alpha-rich field giants. SHETRONE M., TAYAR J., JOHNSON J.A., et al.
2019ApJ...875...29M viz 17       D               1 2918 72 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.
2019ApJ...879...69T viz 17       D               1 222609 141 The Payne: self-consistent ab initio fitting of stellar spectra. TING Y.-S., CONROY C., RIX H.-W., et al.
2020AJ....160..120J viz 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.
2020ApJ...900....4S viz 17       D               1 121537 14 The age distribution of stars in the Milky Way bulge. SIT T. and NESS M.K.
2020ApJS..251...15Z viz 17       D               1 20896 38 Phase II of the LAMOST-Kepler/K2 survey. I. Time series of medium-resolution Spectroscopic observations. ZONG W., FU J.-N., DE CAT P., et al.
2023A&A...671A..53M 159       D     X C       3 16 1 Red horizontal branch stars: An asteroseismic perspective. MATTEUZZI M., MONTALBAN J., MIGLIO A., et al.

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