THE CONNECTION between REDDENING, GAS COVERING FRACTION, and the ESCAPE of IONIZING RADIATION at HIGH REDSHIFT

Naveen A. Reddy, Charles C. Steidel, Max Pettini, Milan Bogosavljevic, Alice E. Shapley

Research output: Contribution to journalArticle

Abstract

Using a large sample of spectroscopically confirmed z ∼ 3 galaxies, we establish an empirical relationship between reddening (E (B - V)), neutral gas covering fraction ( fcov (H I)), and the escape of ionizing (Lyman continuum, LyC) photons. Our sample includes 933 galaxies at z ∼ 3, 121 of which have deep spectroscopic observations (≲7 hr) at 850 ≳ lrest ≳ 1300 A with the Low Resolution Imaging Spectrograph on Keck. The high covering fraction of outflowing optically thick H I indicated by the composite spectra of these galaxies implies that photoelectric absorption, rather than dust attenuation, dominates the depletion of LyC photons. By modeling the composite spectra as the combination of an unattenuated stellar spectrum including nebular continuum emission with one that is absorbed by H I and reddened by a line-of-sight extinction, we derive an empirical relationship between E (B - V) and fcov (H I). Galaxies with redder UV continua have larger covering fractions of H I characterized by higher line-of-sight extinctions. We develop a model which connects the ionizing escape fraction with E (B - V), and which may be used to estimate the ionizing escape fraction for an ensemble of galaxies. Alternatively, direct measurements of the escape fraction for our sample allow us to constrain the intrinsic LyC-to-UV flux density ratio to be 〈S (900 A) S (1500 A)〉 int ≲ 0.20, a value that favors stellar population models that include weaker stellar winds, a flatter initial mass function, and/or binary evolution. Last, we demonstrate how the framework discussed here may be used to assess the pathways by which ionizing radiation escapes from highredshift galaxies.

Original languageEnglish (US)
Article number108
JournalAstrophysical Journal
Volume828
Issue number2
DOIs
StatePublished - Sep 10 2016

Fingerprint

coverings
escape
galaxies
continuums
extinction
gases
gas
line of sight
dust
stellar spectra
composite materials
stellar winds
neutral gases
photons
ionizing radiation
modeling
spectrographs
depletion
flux density
attenuation

Keywords

  • dark ages, reionization, first stars
  • dust, extinction
  • galaxies: evolution
  • galaxies: formation
  • galaxies: high-redshift
  • galaxies: ISM

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

THE CONNECTION between REDDENING, GAS COVERING FRACTION, and the ESCAPE of IONIZING RADIATION at HIGH REDSHIFT. / Reddy, Naveen A.; Steidel, Charles C.; Pettini, Max; Bogosavljevic, Milan; Shapley, Alice E.

In: Astrophysical Journal, Vol. 828, No. 2, 108, 10.09.2016.

Research output: Contribution to journalArticle

Reddy, Naveen A. ; Steidel, Charles C. ; Pettini, Max ; Bogosavljevic, Milan ; Shapley, Alice E. / THE CONNECTION between REDDENING, GAS COVERING FRACTION, and the ESCAPE of IONIZING RADIATION at HIGH REDSHIFT. In: Astrophysical Journal. 2016 ; Vol. 828, No. 2.
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