Characterizing the ELG luminosity functions in the nearby Universe
Date Issued
2024-03
Author(s) USM
DOI
10.1051/0004-6361/202346443
Abstract
Context. Nebular emission lines are powerful diagnostics for the physical processes at play in galaxy formation and evolution. Moreover, emission-line galaxies (ELGs) are one of the main targets of current and forthcoming spectroscopic cosmological survey
