How much can we trust high-resolution spectroscopic stellar chemical abundances?

S. Blanco-Cuaresma; T. Nordlander; U. Heiter; P. Jofré; T. Masseron; L. Casamiquela; H. M. Tabernero; S. S. Bhat; A. R. Casey; J. Meléndez; I. Ramírez

How much can we trust high-resolution spectroscopic stellar chemical abundances?

S. Blanco-Cuaresma, T. Nordlander, U. Heiter, P. Jofré, T. Masseron, L. Casamiquela, H. M. Tabernero, S. S. Bhat, A. R. Casey, J. Meléndez, I. Ramírez

Research output: Chapter in Book/Report/Conference proceeding › Conference Paper › Research

Abstract

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?

Original language	English
Title of host publication	Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society
Subtitle of host publication	Highlights of Spanish Astrophysics IX, SEA 2016
Editors	S. Arribas, A. Alonso-Herrero, F. Figueras, C. Hernandez-Monteagudo, A. Sanchez-Lavega, S. Perez-Hoyos
Place of Publication	Spain
Publisher	Spanish Astronomical Society (SEA)
Pages	334-337
Number of pages	4
ISBN (Electronic)	9788461789313
Publication status	Published - 1 Jan 2016
Externally published	Yes
Event	Scientific Meeting of the Spanish Astronomical Society: Highlights of Spanish Astrophysics IX - Bilbao, Spain Duration: 18 Jul 2016 → 22 Jul 2016 Conference number: 12th

Conference

Conference	Scientific Meeting of the Spanish Astronomical Society
Abbreviated title	SEA 2016
Country	Spain
City	Bilbao
Period	18/07/16 → 22/07/16

Access to Document

318989110-oaFinal published version, 154 KBLicence: CC BY

Cite this

Blanco-Cuaresma, S., Nordlander, T., Heiter, U., Jofré, P., Masseron, T., Casamiquela, L., Tabernero, H. M., Bhat, S. S., Casey, A. R., Meléndez, J., & Ramírez, I. (2016). How much can we trust high-resolution spectroscopic stellar chemical abundances? In S. Arribas, A. Alonso-Herrero, F. Figueras, C. Hernandez-Monteagudo, A. Sanchez-Lavega, & S. Perez-Hoyos (Eds.), Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society: Highlights of Spanish Astrophysics IX, SEA 2016 (pp. 334-337). Spanish Astronomical Society (SEA).

Blanco-Cuaresma, S. ; Nordlander, T. ; Heiter, U. ; Jofré, P. ; Masseron, T. ; Casamiquela, L. ; Tabernero, H. M. ; Bhat, S. S. ; Casey, A. R. ; Meléndez, J. ; Ramírez, I. / How much can we trust high-resolution spectroscopic stellar chemical abundances?. Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society: Highlights of Spanish Astrophysics IX, SEA 2016. editor / S. Arribas ; A. Alonso-Herrero ; F. Figueras ; C. Hernandez-Monteagudo ; A. Sanchez-Lavega ; S. Perez-Hoyos. Spain : Spanish Astronomical Society (SEA), 2016. pp. 334-337

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title = "How much can we trust high-resolution spectroscopic stellar chemical abundances?",

abstract = "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?",

author = "S. Blanco-Cuaresma and T. Nordlander and U. Heiter and P. Jofr{\'e} and T. Masseron and L. Casamiquela and Tabernero, {H. M.} and Bhat, {S. S.} and Casey, {A. R.} and J. Mel{\'e}ndez and I. Ram{\'i}rez",

year = "2016",

month = jan,

day = "1",

language = "English",

pages = "334--337",

editor = "S. Arribas and A. Alonso-Herrero and F. Figueras and C. Hernandez-Monteagudo and A. Sanchez-Lavega and S. Perez-Hoyos",

booktitle = "Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society",

publisher = "Spanish Astronomical Society (SEA)",

note = "Scientific Meeting of the Spanish Astronomical Society : Highlights of Spanish Astrophysics IX, SEA 2016 ; Conference date: 18-07-2016 Through 22-07-2016",

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Blanco-Cuaresma, S, Nordlander, T, Heiter, U, Jofré, P, Masseron, T, Casamiquela, L, Tabernero, HM, Bhat, SS, Casey, AR, Meléndez, J & Ramírez, I 2016, How much can we trust high-resolution spectroscopic stellar chemical abundances? in S Arribas, A Alonso-Herrero, F Figueras, C Hernandez-Monteagudo, A Sanchez-Lavega & S Perez-Hoyos (eds), Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society: Highlights of Spanish Astrophysics IX, SEA 2016. Spanish Astronomical Society (SEA), Spain, pp. 334-337, Scientific Meeting of the Spanish Astronomical Society, Bilbao, Spain, 18/07/16.

How much can we trust high-resolution spectroscopic stellar chemical abundances? / Blanco-Cuaresma, S.; Nordlander, T.; Heiter, U.; Jofré, P.; Masseron, T.; Casamiquela, L.; Tabernero, H. M.; Bhat, S. S.; Casey, A. R.; Meléndez, J.; Ramírez, I.

Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society: Highlights of Spanish Astrophysics IX, SEA 2016. ed. / S. Arribas; A. Alonso-Herrero; F. Figueras; C. Hernandez-Monteagudo; A. Sanchez-Lavega; S. Perez-Hoyos. Spain : Spanish Astronomical Society (SEA), 2016. p. 334-337.

Research output: Chapter in Book/Report/Conference proceeding › Conference Paper › Research