TYC 3139-826-1 , the SIMBAD biblio

TYC 3139-826-1 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST00:00:42


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Title First 3 Authors
2011A&A...534A.125U viz 15       D   O           2 764 297 The Kepler characterization of the variability among A- and F-type stars. I. General overview. UYTTERHOEVEN K., MOYA A., GRIGAHCENE A., 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 15       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.
2016ApJ...829...23D viz 16       D               1 4045 212 The Kepler catalog of stellar flares. DAVENPORT J.R.A.
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.
2017MNRAS.471.2491M viz 16       D               1 226 2 Semi-empirical seismic relations of A-F stars from COROT and Kepler legacy data. MOYA A., SUAREZ J.C., GARCIA HERNANDEZ A., 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.
2018MNRAS.479..183B viz 16       D               1 2598 17 Gaia luminosities of pulsating A-F stars in the Kepler field. BALONA L.A.
2019MNRAS.485.2380M viz 16       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.
2019MNRAS.486.2129D 650 T K A D     X C F     14 1 ~ Spectroscopic confirmation of the binary nature of the hybrid pulsator
KIC 5709664 found with the frequency modulation method.
DEREKAS A., MURPHY S.J., DALYA G., et al.
2019ApJ...879...69T viz 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.
2019MNRAS.490.2112B viz 16       D               1 2864 ~ Evidence for spots on hot stars suggests major revision of stellar physics. BALONA L.A.
2020A&A...638A..57S 41           X         1 7 ~ KIC 8975515: A fast-rotating (γ Dor - δ Sct) hybrid star with Rossby modes and a slower δ Sct companion in a long-period orbit. SAMADI-GHADIM A., LAMPENS P., JASSUR D.M., et al.
2020A&A...638A..59B viz 16       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.
2020AJ....160..120J viz 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.
2020A&A...642A..91L 16       D               1 61 10 Asteroseismology of two Kepler detached eclipsing binaries. LIAKOS A.
2022AJ....163..152S viz 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 viz 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.
2022ApJ...930....7A viz 17       D               1 4216 14 Rotation Distributions around the Kraft Break with TESS and Kepler: The Influences of Age, Metallicity, and Binarity. AVALLONE E.A., TAYAR J.N., VAN SADERS J.L., et al.

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