TY - JOUR

T1 - (Re)Solving Reionization with Lyα

T2 - How Bright Lyα Emitters account for the z ≈ 2 − 8 Cosmic Ionizing Background

AU - Matthee, Jorryt

AU - Naidu, Rohan P

AU - Pezzulli, Gabriele

AU - Gronke, Max

AU - Sobral, David

AU - Oesch, Pascal A

AU - Hayes, Matthew

AU - Erb, Dawn

AU - Schaerer, Daniel

AU - Amorín, Ricardo

AU - Tacchella, Sandro

AU - Paulino-Afonso, Ana

AU - Llerena, Mario

AU - Calhau, João

AU - Röttgering, Huub

PY - 2022/6/30

Y1 - 2022/6/30

N2 - The cosmic ionizing emissivity from star-forming galaxies has long been anchored to UV luminosity functions. Here we introduce an emissivity framework based on Lyα emitters (LAEs), which naturally hones in on the subset of galaxies responsible for the ionizing background due to the intimate connection between production and escape of Lyα and LyC photons. Using constraints on the escape fractions of bright LAEs (LLyα > 0.2L*) at z ≈ 2 obtained from resolved Lyα profiles, and arguing for their redshift-invariance, we show that: (i) quasars and LAEs together reproduce the relatively flat emissivity at z ≈ 2 − 6, which is non-trivial given the strong evolution in both the star-formation density and quasar number density at these epochs and (ii) LAEs produce late and rapid reionization between z ≈ 6 − 9 under plausible assumptions. Within this framework, the >10 × rise in the UV population-averaged fesc between z ≈ 3 − 7 naturally arises due to the same phenomena that drive the growing Lyα emitter fraction with redshift. Generally, a LAE dominated emissivity yields a peak in the distribution of the ionizing budget with UV luminosity as reported in latest simulations. Using our adopted parameters ($f_{\rm {esc}}=50\%$, ξion = 1025.9 Hz erg−1 for half the bright LAEs), a highly ionizing minority of galaxies with MUV < −17 accounts for the entire ionizing budget from star-forming galaxies. Rapid flashes of LyC from such rare galaxies produce a “disco” ionizing background. We conclude proposing tests to further develop our suggested Lyα-anchored formalism.

AB - The cosmic ionizing emissivity from star-forming galaxies has long been anchored to UV luminosity functions. Here we introduce an emissivity framework based on Lyα emitters (LAEs), which naturally hones in on the subset of galaxies responsible for the ionizing background due to the intimate connection between production and escape of Lyα and LyC photons. Using constraints on the escape fractions of bright LAEs (LLyα > 0.2L*) at z ≈ 2 obtained from resolved Lyα profiles, and arguing for their redshift-invariance, we show that: (i) quasars and LAEs together reproduce the relatively flat emissivity at z ≈ 2 − 6, which is non-trivial given the strong evolution in both the star-formation density and quasar number density at these epochs and (ii) LAEs produce late and rapid reionization between z ≈ 6 − 9 under plausible assumptions. Within this framework, the >10 × rise in the UV population-averaged fesc between z ≈ 3 − 7 naturally arises due to the same phenomena that drive the growing Lyα emitter fraction with redshift. Generally, a LAE dominated emissivity yields a peak in the distribution of the ionizing budget with UV luminosity as reported in latest simulations. Using our adopted parameters ($f_{\rm {esc}}=50\%$, ξion = 1025.9 Hz erg−1 for half the bright LAEs), a highly ionizing minority of galaxies with MUV < −17 accounts for the entire ionizing budget from star-forming galaxies. Rapid flashes of LyC from such rare galaxies produce a “disco” ionizing background. We conclude proposing tests to further develop our suggested Lyα-anchored formalism.

KW - Space and Planetary Science

KW - Astronomy and Astrophysics

U2 - 10.1093/mnras/stac801

DO - 10.1093/mnras/stac801

M3 - Journal article

VL - 512

SP - 5960

EP - 5977

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 4

ER -