TYC 3550-1536-1 , the SIMBAD biblio

TYC 3550-1536-1 , the SIMBAD biblio (30 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST07:09:26

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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
2014MNRAS.445.2758R viz 15       D               1 1992 127 Bayesian distances and extinctions for giants observed by Kepler and APOGEE. RODRIGUES T.S., GIRARDI L., MIGLIO A., et al.
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.
2015ApJ...807...82T viz 16       D               4 40 52 Rapid rotation of low-mass red giants using APOKASC: a measure of interaction rates on the post-main-sequence. TAYAR J., CEILLIER T., GARCIA-HERNANDEZ D.A., et al.
2016MNRAS.456.3655M viz 16       D               1 1476 181 Red giant masses and ages derived from carbon and nitrogen abundances. MARTIG M., FOUESNEAU M., RIX H.-W., et al.
2016ApJ...823..114N viz 16       D               1 72935 173 Spectroscopic determination of masses (and implied ages) for red giants. NESS M., HOGG D.W., RIX H.-W., et al.
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.
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.
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.
2016A&A...594A..43H viz 16       D               1 2093 93 An accurate and self-consistent chemical abundance catalogue for the APOGEE/Kepler sample. HAWKINS K., MASSERON T., JOFRE P., et al.
2017MNRAS.469.4578H viz 16       D               1 8666 48 Deep learning classification in asteroseismology. HON M., STELLO D. and YU J.
2017A&A...605A.111C viz 16       D               1 531 81 Surface rotation of Kepler red giant stars. CEILLIER T., TAYAR J., MATHUR S., et al.
2018MNRAS.475.5487S viz 16       D               1 1201 147 Confirming chemical clocks: asteroseismic age dissection of the Milky Way disc(s). SILVA AGUIRRE V., BOJSEN-HANSEN M., SLUMSTRUP D., 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.
2019ApJ...872..137S viz 16       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...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.
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.
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.
2020ApJ...900....4S viz 16       D               1 121537 14 The age distribution of stars in the Milky Way bulge. SIT T. and NESS M.K.
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.
2021ApJ...913L...4S 17       D               1 22 16 Tracking the evolution of lithium in giants using asteroseismology: super-Li-rich stars are almost exclusively young red-clump stars. SINGH R., REDDY B.E., CAMPBELL S.W., 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...664A..78F viz 17       D               1 7452 7 Characterization of Kepler targets based on medium-resolution LAMOST spectra analyzed with ROTFIT,. FRASCA A., MOLENDA-ZAKOWICZ J., ALONSO-SANTIAGO J., et al.
2023ApJ...944L...5M viz 17       D               1 1240 3 Lithium Abundances in Giants as a Function of Stellar Mass: Evidence for He Flash as the Source of Li Enhancement in Low-mass Giants. MALLICK A., SINGH R. and REDDY B.E.
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...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.
2024ApJ...977..138H 18       D               1 209 ~ Revisiting the Activity-Rotation Relation for Evolved Stars. HAN H., WANG S., LI X., et al.
2025ApJ...980..265M 19       D               1 84 ~ High Lithium Abundance Connection with the Chromospheric Helium in Red Giants: Spectroscopic and Asteroseismic Analyses. MALLICK A., SNEDEN C., REDDY B.E., et al.
2025ApJ...990L..12S 19       D               1 17 ~ Li Enrichment in Red Clump Giants: Clues for Past Binary Interaction or Merger Events. SINGH R., REDDY B.E., MALLICK A., et al.

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