Evidence for a low Lyman Continuum Escape fraction in three Massive, UV-bright galaxies at z > 7
Callum Witten, Nicolas Laporte, Harley Katz

TL;DR
This study investigates the Lyman Continuum escape fraction in three massive, UV-bright galaxies at z > 7, finding it to be less than 10%, which challenges the idea that such galaxies significantly contributed to reionization.
Contribution
The paper provides the first direct constraints on the LyC escape fraction in massive, UV-bright galaxies at z > 7 using deep spectroscopic stacking analysis.
Findings
Lyman alpha profiles show a dominant red peak with no blue peak.
Estimated escape fraction of LyC photons is less than 10%.
Massive, UV-bright galaxies at z > 7 are unlikely to be the main reionization sources.
Abstract
Although low-mass star-forming galaxies are the leading candidates of the reionisation process, we cannot conclusively rule out high-mass star-forming galaxies as candidates. While most simulations indicate the former is the best candidate some models suggest that at z > 6 massive, UV-bright galaxies - "oligarchs" - account for at least 80% of the ionising budget. To test this hypothesis we target massive (log10 (M*[Msol]) > 10), UV-bright (MUV ~ -22) Lya emitters at z > 7 in archival data, observed with similar resolution spectrographs (VLT/X-shooter and Keck/MOSFIRE). To increase the reliability of our conclusions we stack all spectra and obtain a deep-stacked spectrum of 24.75 hrs. The stacked Lya profile displays a clear asymmetric red peak and an absence of a blue peak. We additionally estimate the intrinsic stacked Lya profile of our targets by correcting for IGM transmission…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Galaxies: Formation, Evolution, Phenomena · Spectroscopy and Laser Applications
