TYC 3145-1523-1 , the SIMBAD biblio

TYC 3145-1523-1 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST01:39:20


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Title First 3 Authors
2014ApJS..215...19P viz 15       D               1 2388 259 The APOKASC catalog: an asteroseismic and spectroscopic joint survey of targets in the Kepler fields. PINSONNEAULT M.H., ELSWORTH Y., EPSTEIN C., et al.
2014A&A...572L...5M viz 15       D               1 1210 165 Mixed modes in red giants: a window on stellar evolution. MOSSER B., BENOMAR O., BELKACEM K., et al.
2015A&A...578A..76C 94       D       C       1 19 7 High-precision acoustic helium signatures in 18 low-mass low-luminosity red giants. Analysis from more than four years of Kepler observations. CORSARO E., DE RIDDER J. and GARCIA R.A.
2015A&A...579A..83C 368       D     X C       9 19 57 Bayesian peak bagging analysis of 19 low-mass low-luminosity red giants observed with Kepler. CORSARO E., DE RIDDER J. and GARCIA R.A.
2016AJ....152....6W viz 16       D               1 3060 13 Calibration of LAMOST stellar surface gravities using the Kepler asteroseismic data. WANG L., WANG W., WU Y., et al.
2016A&A...591A..99P 16       D               4 19 10 Asteroseismology of 19 low-luminosity red giant stars from Kepler. PEREZ HERNANDEZ F., GARCIA R.A., CORSARO E., et al.
2016A&A...594A..39F viz 16       D               2 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.
2017A&A...602A..62T 95       D       C       3 15 15 Internal rotation of 13 low-mass low-luminosity red giants in the Kepler field. TRIANA S.A., CORSARO E., DE RIDDER J., et al.
2018A&A...610A..80H 161           X C       3 22 10 Gravity mode offset and properties of the evanescent zone in red-giant stars. HEKKER S., ELSWORTH Y. and ANGELOU G.C.
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.476.1470G 96       D         F     5 19 7 Automated asteroseismic peak detections. GARCIA SARAVIA ORTIZ DE MONTELLANO A., HEKKER S. and THEMESSL N.
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.
2017NatAs...1...64C 16       D               1 96 ~ Spin alignment of stars in old open clusters. CORSARO E., LEE Y.-N., GARCIA R.A., et al.
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.
2018A&A...616A..24G viz 16       D               1 1140 108 Core rotation braking on the red giant branch for various mass ranges. GEHAN C., MOSSER B., MICHEL E., et al.
2020A&A...639A..63G viz 16       D               1 4575 22 Active red giants: Close binaries versus single rapid rotators. GAULME P., JACKIEWICZ J., SPADA F., et al.
2021A&A...645A.124G viz 268       D     X C F     5 1202 13 Automated approach to measure stellar inclinations: validation through large-scale measurements on the red giant branch. GEHAN C., MOSSER B., MICHEL E., et al.
2021AJ....161..170S viz 17       D               1 16187 ~ The Swan: data-driven inference of stellar surface gravities for cool stars from photometric light curves. SAYEED M., HUBER D., WHEELER A., et al.
2022ApJ...927..167L viz 17       D               1 3663 12 Asteroseismology of 3642 Kepler Red Giants: Correcting the Scaling Relations Based on Detailed Modeling. LI T., LI Y., BI S., et al.
2023ApJ...954..152K viz 17       D               1 1077 ~ Mixed-mode Ensemble Asteroseismology of Low-luminosity Kepler Red Giants. KUSZLEWICZ J.S., HON M. and HUBER D.
2024A&A...686A..93G viz 18       D               1 4574 ~ Magnetic activity of red giants: Correlation between the amplitude of solar-like oscillations and chromospheric indicators. GEHAN C., GODOY-RIVERA D. and GAULME P.

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