A HARD IONIZING SPECTRUM IN z = 3–4 Ly α EMITTERS WITH INTENSE $[{\rm{O}}\,{\rm{III}}]$ EMISSION: ANALOGS OF GALAXIES IN THE REIONIZATION ERA?

• Published in: Astrophysical journal. Letters 2016-11, Vol.831 (1), p.L9
• Main Authors: Nakajima, Kimihiko, Ellis, Richard S., Iwata, Ikuru, Inoue, Akio K., Kusakabe, Haruka, Ouchi, Masami, Robertson, Brant E.
• Format: Article
• Language: English
• Subjects: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; DIAGRAMS; GALAXIES; LUMINOSITY; LYMAN LINES; METALLICITY; PHOTOIONIZATION; PHOTONS; RECOMBINATION; RED SHIFT; SPECTRA; ULTRAVIOLET RADIATION
• ISSN: 2041-8213; 2041-8205; 2041-8213
• DOI: 10.3847/2041-8205/831/1/L9

We present Keck/MOSFIRE spectra of the diagnostic nebular emission lines [O iii]λλ5007,4959, [O ii]λ3727, and Hβ for a sample of 15 redshift z≃3.1--3.7 Lyα emitters (LAEs) and Lyman break galaxies (LBGs). In conjunction with spectra from other surveys, we confirm earlier indications that LAEs have a much higher [O iii]/[O ii] line ratio than is seen in similar redshift LBGs. By comparing their distributions on a [O iii]/[O ii] versus R23 diagram, we demonstrate that this difference cannot arise solely because of their lower metallicities but most likely is due to a harder ionizing spectrum. Using measures of Hβ and recombination theory, we demonstrate, for a subset of our LAEs, that ξ{sub ion}—the number of Lyman continuum photons per UV luminosity—is indeed 0.2–0.5 dex larger than for typical LBGs at similar redshifts. Using photoionization models, we estimate the effect this would have on both [O iii]/[O ii] and R23 and conclude such a hard spectrum can only partially explain such intense line emission. The additional possibility is that such a large [O iii]/[O ii] ratio is in part due to density rather than ionization bound nebular regions, which would imply a high escape fraction of ionizing photons. We discuss how further observations could confirm this possibility. Clearly LAEs with intense [O iii] emission represent a promising analog of those z>7 sources with similarly strong lines that are thought to be an important contributor to cosmic reionization.