UCAC4 475-048435 , the SIMBAD biblio

UCAC4 475-048435 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST20:40:38

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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
2015A&A...579A..19A viz 16       D               1 8375 75 K2 Variable Catalogue: Variable stars and eclipsing binaries in K2 campaigns 1 and 0. ARMSTRONG D.J., KIRK J., LAM K.W.F., 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.
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.
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...929...33H viz 17       D               1 114072 2 Quantifying Chemical and Kinematical Properties of Galactic Disks. HU G. and SHAO Z.
2022A&A...663A.126F viz 17       D               2 424 10 Galactic ArchaeoLogIcaL ExcavatiOns (GALILEO). I. An updated census of APOGEE N-rich giants across the Milky Way. FERNANDEZ-TRINCADO J.G., BEERS T.C., BARBUY B., et al.
2023ApJ...950..142H viz 17       D               1 26076 ~ Angular Momentum Variation of the Milky Way Thick Disk: The Dependence of Chemical Abundance and Evidence of the Inside-out Formation Scenario. HU G., SHAO Z. and LI L.

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