What can we learn from constraining Extreme-Emission Line Galaxies models with large samples of local analogs?
Extreme Emission Line Galaxies (EELGs) are characterized by their compact sizes and very high equivalent widths of certain optical emission lines (e.g. EW([OIII]) $>$ 500Å), indicative of very high specific star formation rates, similar to those detected in the reionization epoch galaxies. Many of them also present certain high-excitation emission
Pérez-Montero, Enrique et al.
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2023