Cosmic web Ly alpha emission in a sample of overdense regions
astro-ph.GA, astro-ph.CO
Submitted: 2026-09-17
Updated: 2026-10-13
Comments: 18 pages, 12 Figures (+2 in appendix). Resubmitted to A&A following a referee report
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- The Stacked Lyman-Alpha Emission Profile from the Circum-Galactic Medium of z~2 Quasars
- The MUSE Hubble Ultra Deep Field Survey: I. Survey description, data reduction and source detection
- WST -- Widefield Spectroscopic Telescope: Motivation, science drivers and top-level requirements for a new dedicated facility
- MUSEQuBES: Unveiling Cosmic Web Filaments at $z\approx3.6$ through Dual Absorption and Emission Line Analysis
- The VLT LBG Redshift Survey - V. Characterising the z = 3.1 Lyman Alpha Emitter Population
- The cosmic web in Lyman-alpha emission
- Discovery of an Enormous Ly$\alpha$ nebula in a massive galaxy overdensity at $z=2.3$
- Ancient Light from Young Cosmic Cities: Physical and Observational Signatures of Galaxy Proto-Clusters
- An Analytic Model for the Evolution of the Stellar, Gas, and Metal Content of Galaxies
- Cold streams in early massive hot haloes as the main mode of galaxy formation
- Detecting the Cosmic Web: Ly{\alpha} Emission from Simulated Filaments at z=3
- Stacking the Cosmic Web in Fluorescent Lyman alpha Emission with MUSE
- QSO MUSEUM III: the circumgalactic medium in Ly$\alpha$ emission around 120 $z\sim3$ quasars covering the SDSS parameter space. Witnessing the instantaneous AGN feedback on halo scales
- Imaging the Lyman-alpha Forest
- Median Surface Brightness Profiles of Lyman-$\alpha$ Haloes in the MUSE Extremely Deep Field
- The Lyman-alpha Forest in the Cold Dark Matter Model
- QSO MUSEUM II: Search for extended Ly$\alpha$ emission around eight $z \sim 3$ quasar pairs
- Testing Lyman Alpha Emitters and Lyman-Break Galaxies as Tracers of Large-Scale Structures at High Redshifts
- Lyman-alpha Emission From Cosmic Structure I: Fluorescence
- Discovery of a Very Large Structure at Z=3.78
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