Five cosmological simulations predict that the faint ultraviolet excess seen by the Condor telescope at z≈2.5 is Lyman-alpha light from the cosmic web, with measurable detection thresholds for wide-field surveys.
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The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection
Five cosmological simulations predict that the faint ultraviolet excess seen by the Condor telescope at z≈2.5 is Lyman-alpha light from the cosmic web, with measurable detection thresholds for wide-field surveys.