KIC 8329014 , the SIMBAD biblio

KIC 8329014 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST19:21:08


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Title First 3 Authors
2010AstL...36..338F viz 15       D               1 1150 6 Proper motions and CCD photometry of stars in the region of the open cluster NGC 6866. FROLOV V.N., ANANJEVSKAJA Y.K., GORSHANOV D.L., et al.
2012ApJS..199...24T viz 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.
2013A&A...557L..10N viz 16       D               1 12151 189 Rotation periods of 12000 main-sequence Kepler stars: dependence on stellar spectral type and comparison with v sin i observations. NIELSEN M.B., GIZON L., SCHUNKER H., et al.
2016A&A...594A..39F viz 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.
2018MNRAS.474.4322M viz 16       D               2 390 89 Finding binaries from phase modulation of pulsating stars with Kepler: V. Orbital parameters, with eccentricity and mass-ratio distributions of 341 new binaries. MURPHY S.J., MOE M., KURTZ D.W., et al.
2018A&A...614A..46B viz 16       D               1 1063 5 The envelope of the power spectra of over a thousand δ Scuti stars. The Teff - νmax scaling relation. BARCELO FORTEZA S., ROCA CORTES T. and GARCIA R.A.
2019MNRAS.485.2380M viz 17       D               1 14330 108 Gaia-derived luminosities of Kepler A/F stars and the pulsator fraction across the δ Scuti instability strip. MURPHY S.J., HEY D., VAN REETH T., et al.
2020MNRAS.491.3586L viz 17       D               1 609 75 Gravity-mode period spacings and near-core rotation rates of 611 γ Doradus stars with Kepler. LI G., VAN REETH T., BEDDING T.R., et al.
2020A&A...638A..59B viz 17       D               1 2220 17 Unveiling the power spectra of δ Scuti stars with TESS. The temperature, gravity, and frequency scaling relation. BARCELO FORTEZA S., MOYA A., BARRADO D., et al.

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