How well can we determine ages and chemical abundances from spectral fitting of integrated light spectra? (2020)
- Authors:
- USP affiliated authors: COELHO, PAULA RODRIGUES TEIXEIRA - IAG ; SANTOS JUNIOR, GERALDO GONÇALVES DOS - IAG
- Unidade: IAG
- DOI: 10.1093/mnras/staa3051
- Subjects: COSMOLOGIA; AGLOMERADOS DE GALÁXIAS; UNIVERSO PRIMORDIAL; FOTOMETRIA
- Agências de fomento:
- Language: Inglês
- Imprenta:
- Source:
- Título: Monthly Notices of the Royal Astronomical Society
- ISSN: 1365-2966
- Volume/Número/Paginação/Ano: v. 499, n. 2, p. 2327–2339, 2020
- Este artigo possui versão em acesso aberto
- URL de acesso aberto
- PDF de acesso aberto
- Versão do Documento: Versão submetida (Pré-print)
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Status: Artigo possui versão em acesso aberto em repositório (Green Open Access) -
ABNT
GONÇALVES, Geraldo et al. How well can we determine ages and chemical abundances from spectral fitting of integrated light spectra?. Monthly Notices of the Royal Astronomical Society, v. 499, n. 2, p. 2327–2339, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/staa3051. Acesso em: 15 mar. 2026. -
APA
Gonçalves, G., Coelho, P., Shiavon, R., & Usher, C. (2020). How well can we determine ages and chemical abundances from spectral fitting of integrated light spectra? Monthly Notices of the Royal Astronomical Society, 499( 2), 2327–2339. doi:10.1093/mnras/staa3051 -
NLM
Gonçalves G, Coelho P, Shiavon R, Usher C. How well can we determine ages and chemical abundances from spectral fitting of integrated light spectra? [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 499( 2): 2327–2339.[citado 2026 mar. 15 ] Available from: https://doi.org/10.1093/mnras/staa3051 -
Vancouver
Gonçalves G, Coelho P, Shiavon R, Usher C. How well can we determine ages and chemical abundances from spectral fitting of integrated light spectra? [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 499( 2): 2327–2339.[citado 2026 mar. 15 ] Available from: https://doi.org/10.1093/mnras/staa3051 - Surface brightness fluctuation spectrum: a new probe of evolved stars inunresolved stellar populations
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