2MASS J13481626-0049214 , the SIMBAD biblio

2MASS J13481626-0049214 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST11:22:22


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Title First 3 Authors
2015RAA....15.1671S viz 16       D               1 176 4 Identifying Carbon stars from the LAMOST pilot survey with the efficient manifold ranking algorithm. SI J.-M., LI Y.-B., LUO A.-L., 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.
2016ApJS..226....1J viz 16       D               1 894 4 Carbon stars from LAMOST DR2 data. JI W., CUI W., LIU C., et al.
2018ApJ...852...49H viz 16       D               1 1325 118 Disentangling the Galactic halo with APOGEE. I. Chemical and kinematical investigation of distinct metal-poor populations. HAYES C.R., MAJEWSKI S.R., SHETRONE M., et al.
2018AJ....156...18P viz 16       D               1 51824 872 Binary companions of evolved stars in APOGEE DR14: search method and catalog of ∼5000 companions. PRICE-WHELAN A.M., HOGG D.W., RIX H.-W., et al.
2019ApJ...872..137S viz 17       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 17       D               1 222609 141 The Payne: self-consistent ab initio fitting of stellar spectra. TING Y.-S., CONROY C., RIX H.-W., et al.
2019AJ....158..147H viz 17       D               1 44781 43 Spectrophotometric parallaxes with linear models: accurate distances for luminous red-giant stars. HOGG D.W., EILERS A.-C. and RIX H.-W.
2020AJ....160..120J viz 17       D               1 365761 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 17       D               1 121537 14 The age distribution of stars in the Milky Way bulge. SIT T. and NESS M.K.

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