New fully empirical calibrations of strong-line metallicity indicators in star forming galaxies

By M. Curti, G. Cresci, F. Mannucci, A. Marconi, R. Maiolino, S. Esposito. 2016

173 citations recorded by the source corpus.

MC acknowledges financial support from INAF for his PhD fellowship. RM acknowledges support from the ERC Advanced Grant 695671 "QUENCH'' and support from the Science and Technology Facilities Council (STFC). Funding for the SDSS and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the U.S. Department of Energy, the National Aeronautics and Space Administration, the Japanese Monbukagakusho, the Max Planck Society and the Higher Education Funding Council for England. The SDSS Web Site is http://www.sdss.org/.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/aed58599944f26e1a100ff5ac6ac5350eec34ef2

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In Astronomy and Astrophysics

Citations in the corpus

SDSS IV MaNGA – metallicity and nitrogen abundance gradients in local galaxies (2017, background): “Despite recent advances (Dopita et al. 2013; Perez-Montero 2014; Blanc et al. 2015; Asari et al. 2016; Curti et al. 2017), reliably measuring the gas metallicity from strong emission lines ratios remains a difficult problem in observational astrophysics.”
The mass–metallicity and the fundamental metallicity relation revisited on a fully Te-based abundance scale for galaxies (2019, methodology): “…consideration that we want to stress here is that the main results presented throughout the paper are robust against the choice of different combinations of line ratios, as proven also by the good internal consistency of the proposed calibrations (see Figure 10 and 11 of Curti et al. 2017).”