How much can we trust high-resolution spectroscopic stellar chemical abundances?
- Title
 - How much can we trust high-resolution spectroscopic stellar chemical abundances?
 - Creator
 - Blanco-Cuaresma S.; Nordlander T.; Heiter U.; JofrP.; Masseron T.; Casamiquela L.; Tabernero H.M.; Bhat S.S.; Casey A.R.; Meldez J.; Ramez I.
 - Description
 - To study stellar populations, it is common to combine chemical abundances from different spectroscopic surveys/studies where different setups were used. These inhomogeneities can lead us to inaccurate scientific conclusions. In this work, we studied one aspect of the problem: When deriving chemical abundances from high-resolution stellar spectra, what differences originate from the use of different radiative transfer codes? 2016 Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016. All rights reserved.
 - Source
 - Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016, pp. 334-337.
 - Date
 - 2016-01-01
 - Publisher
 - SEA
 - Coverage
 - Blanco-Cuaresma S., Observatoire de Gene, Universitde Gene, Versoix, CH-1290, Switzerland; Nordlander T., Dept. of Physics and Astronomy, Uppsala University, Box 516, Uppsala, 75120, Sweden; Heiter U., Dept. of Physics and Astronomy, Uppsala University, Box 516, Uppsala, 75120, Sweden; JofrP., Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, United Kingdom; Masseron T., Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, United Kingdom; Casamiquela L., Dep. Fica Qutica i Astrofica, Universitat de Barcelona, ICCUB-IEEC, Spain; Tabernero H.M., Dpto. Astrofica, Facultad de CC. Ficas, Universidad Complutense de Madrid, Spain; Bhat S.S., Christ University, Hosur Road, Bangalore, 560029, India; Casey A.R., Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, United Kingdom; Meldez J., Dept. de Astronomia do IAG/USP, Universidade de Sao Paulo, Brazil; Ramez I., McDonald Observatory, Dept. of Astronomy, University of Texas, Austin, United States
 - Rights
 - Restricted Access
 - Relation
 - ISBN: 978-846178931-3
 - Format
 - Online
 - Language
 - English
 - Type
 - Conference paper
 
Collection
Citation
Blanco-Cuaresma S.; Nordlander T.; Heiter U.; JofrP.; Masseron T.; Casamiquela L.; Tabernero H.M.; Bhat S.S.; Casey A.R.; Meldez J.; Ramez I., “How much can we trust high-resolution spectroscopic stellar chemical abundances?,” CHRIST (Deemed To Be University) Institutional Repository, accessed November 4, 2025, https://archives.christuniversity.in/items/show/21010.
            