Nearly all the sky is covered by Lyman-alpha emission around high redshift galaxies
L. Wisotzki, R. Bacon, J. Brinchmann, S. Cantalupo, P. Richter, J., Schaye, K. B. Schmidt, T. Urrutia, P. M. Weilbacher, M. Akhlaghi, N. Bouche,, T. Contini, B. Guiderdoni, E. C. Herenz, H. Inami, J. Kerutt, F. Leclercq, R., A. Marino, M. Maseda, A. Monreal-Ibero, T. Nanayakkara

TL;DR
This study reveals that nearly the entire sky around high-redshift galaxies is covered by faint Lyman-alpha emission, indicating widespread circumgalactic hydrogen that matches absorption measurements from quasar spectra.
Contribution
It demonstrates that low surface brightness Lyman-alpha emission from faint galaxies at redshifts 3-6 covers almost 100% of the sky, revealing the extent of circumgalactic hydrogen.
Findings
Sky coverage of Lyman-alpha emission is nearly 100%.
Incidence rate of Lyman-alpha emitters exceeds unity.
Emission detection aligns with absorption measurements of hydrogen.
Abstract
Galaxies are surrounded by large reservoirs of gas, mostly hydrogen, fed by inflows from the intergalactic medium and by outflows due to galactic winds. Absorption-line measurements along the sightlines to bright and rare background quasars indicate that this circumgalactic medium pervades far beyond the extent of starlight in galaxies, but very little is known about the spatial distribution of this gas. A new window into circumgalactic environments was recently opened with the discovery of ubiquitous extended Lyman-alpha emission from hydrogen around high-redshift galaxies, facilitated by the extraordinary sensitivity of the MUSE instrument at the ESO Very Large Telescope. Due to the faintness of this emission, such measurements were previously limited to especially favourable systems or to massive statistical averaging. Here we demonstrate that low surface brightness Lyman-alpha…
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