TYC 3148-2032-1 , the SIMBAD biblio

TYC 3148-2032-1 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST17:09:44


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Title First 3 Authors
2016AJ....151...68K viz 16       D               1 2915 316 Kepler eclipsing binary stars. VII. The catalog of eclipsing binaries found in the entire Kepler data set. KIRK B., CONROY K., PRSA A., et al.
2017AJ....154..105K viz 16       D               1 532 5 Orbital parameters of the eclipsing detached Kepler binaries with eccentric orbits. KJURKCHIEVA D., VASILEVA D. and ATANASOVA T.
2017MNRAS.469.4578H viz 16       D               1 8666 48 Deep learning classification in asteroseismology. HON M., STELLO D. and YU J.
2017AJ....154..250L viz 16       D               1 2281 72 Tidal synchronization and differential rotation of Kepler eclipsing binaries. LURIE J.C., VYHMEISTER K., HAWLEY S.L., et al.
2018MNRAS.475.3633W viz 16       D               1 3727 38 Mass and age of red giant branch stars observed with LAMOST and Kepler. WU Y., XIANG M., BI S., et al.
2018MNRAS.476.3233H viz 16       D               1 15009 17 Deep learning classification in asteroseismology using an improved neural network: results on 15 000 Kepler red giants and applications to K2 and TESS data. HON M., STELLO D. and YU J.
2018ApJS..236...42Y viz 16       D               1 16097 158 Asteroseismology of 16,000 Kepler red giants: global oscillation parameters, masses, and radii. YU J., HUBER D., BEDDING T.R., et al.
2019MNRAS.487.2455O 301       D     X C F     6 98 ~ Solving eclipsing binaries with a solar-like pulsator via Kepler data. OU J.-W., YANG M., LIU H.-G., et al.
2019A&A...630A.106G viz 16       D               1 308 39 Systematic search for stellar pulsators in the eclipsing binaries observed by Kepler. GAULME P. and GUZIK J.A.
2019ApJS..244...43Z viz 16       D               1 1328 22 Unbiased distribution of binary parameters from LAMOST and Kepler observations. ZHANG J., QIAN S.-B., WU Y., 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.
2021A&A...648A.113B viz 394       D     X   F     9 19 20 Spectroscopic and seismic analysis of red giants in eclipsing binaries discovered by Kepler. BENBAKOURA M., GAULME P., McKEEVER J., et al.
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.
2022A&A...667A..31B 17       D               1 196 4 99 oscillating red-giant stars in binary systems with NASA TESS and NASA Kepler identified from the SB9-Catalogue. BECK P.G., MATHUR S., HAMBLETON K., et al.
2023ApJS..264...17Z viz 17       D               1 31380 1 Stellar Parameters and Spectroscopic Properties of TESS Objects Observed in the LAMOST Low- and Medium-resolution Spectral Survey. ZHANG L.-Y., SU T., MISRA P., et al.
2023A&A...674A..34G viz 17       D               1 307215 85 Gaia Data Release 3 Stellar multiplicity, a teaser for the hidden treasure. GAIA COLLABORATION, ARENOU F., BABUSIAUX C., et al.
2023A&A...678A.158A viz 17       D               1 171655 ~ Spectroscopic age estimates for APOGEE red-giant stars: Precise spatial and kinematic trends with age in the Galactic disc. ANDERS F., GISPERT P., RATCLIFFE B., et al.
2024A&A...682A...7B viz 18       D               2 2137 ~ Constraining stellar and orbital co-evolution through ensemble seismology of solar-like oscillators in binary systems A census of oscillating red giants and dwarf stars in Gaia DR3 binaries. BECK P.G., GROSSMANN D.H., STEINWENDER L., et al.
2024A&A...685A..62I viz 18       D               1 2906 ~ Automated eccentricity measurement from raw eclipsing binary light curves with intrinsic variability. IJSPEERT L.W., TKACHENKO A., JOHNSTON C., et al.

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