The [O III]λ5007 equivalent width distribution at z ∼ 2: the redshift evolution of the extreme emission line galaxies. Issue 3 (25th April 2022)

• Record Type: Journal Article
• Authors: Boyett, Kristan N K; Stark, Daniel P; Bunker, Andrew J; Tang, Mengtao; Maseda, Michael V
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 513:Issue 3(2022)
• Page Start: 4451
• Page End: 4463
• Publication Date: 2022-04-25
• Subjects: galaxies: evolution -- galaxies: high-redshift; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stac1109
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: We determine the [O III]λ5007 equivalent width (EW) distribution of $1.700\lt \rm {z}\lt 2.274$ rest-frame ultraviolet (UV)-selected (MUV < −19) star-forming galaxies in the GOODS North and South fields. We make use of deep HDUV broad-band photometry catalogues for selection and 3D- HST WFC3/IR grism spectra for measurement of line properties. The [O III]λ5007 EW distribution allows us to measure the abundance of extreme emission line galaxies (EELGs) within this population. We model a lognormal distribution to the [O III]λ5007 rest-frame EWs of galaxies in our sample, with location parameter μ = 4.24 ± 0.07 and variance parameter σ = 1.33 ± 0.06. This EW distribution has a mean [O III]λ5007 EW of 168 ± 1 Å. The fractions of $\rm {z}\sim 2$ rest-UV-selected galaxies with [O III]λ5007 EWs greater than 500, 750, and 1000 Å are measured to be $6.8^{+1.0}_{-0.9}{{\ \rm per\ cent}}$, $3.6^{+0.7}_{-0.6}{{\ \rm per\ cent}}$, and $2.2^{+0.5}_{-0.4}{{\ \rm per\ cent}}$, respectively. The EELG fractions do not vary strongly with UV luminosity in the range (−21.6 < M UV < −19.0) considered in this paper, consistent with findings at higher redshifts. We compare our results to $\rm {z}\sim 5$ and $\rm {z}\sim 7$ 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 ∼10 between $\rm {z}\sim 2$ and $\rm {z}\sim 7$ ). This evolution is consistent with an increased incidence of strong bursts in the galaxy population of the reionization era. While this population makes a sub-dominant contribution of the ionizing emissivity at $\rm {z}\simeq 2$, EELGs are likely to dominate the ionizing output in the reionization era.