The [OIII] equivalent width distribution at z : The redshift evolution of the extreme emission line galaxies
arXiv:2110.15858 · doi:10.1093/mnras/stac1109
Abstract
We determine the [OIII] equivalent width (EW) distribution of rest-frame UV-selected (M) star-forming galaxies in the GOODS North and South fields. We make use of deep HDUV broadband photometry catalogues for selection and 3D-HST WFC3/IR grism spectra for measurement of line properties. The [OIII] EW distribution allows us to measure the abundance of extreme emission line galaxies (EELGs) within this population. We model a log-normal distribution to the [OIII] rest-frame equivalent widths of galaxies in our sample, with location parameter and variance parameter . This EW distribution has a mean [OIII] EW of 168. The fractions of rest-UV-selected galaxies with [OIII] EWs greater than and are measured to be , , and respectively. The EELG fractions do not vary strongly with UV luminosity in the range () considered in this paper, consistent with findings at higher redshifts. We compare our results to and studies where candidate EELGs have been discovered through Spitzer/IRAC colours, and we identify rapid evolution with redshift in the fraction of star-forming galaxies observed in an extreme emission line phase (a rise by a factor between and ). This evolution is consistent with an increased incidence of strong bursts in the galaxy population of the reionisation era. While this population makes a sub-dominant contribution of the ionising emissivity at , EELGs are likely to dominate the ionising output in the reionisation era.
arXiv commentSubmitted to MNRAS. 13 pages, 6 figures
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