3 papers found
Refreshing results…
The Lyα and UV luminosity-dependent clustering of typical Lyα emitters up to z ~ 6
LoTSS/HETDEX: Optical quasars I. Low-frequency radio properties of optically selected quasars
The clustering of typical Ly$α$ emitters from $z ∼ 2.5 - 6$: host halo masses depend on Ly$α$ and UV luminosities
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