Nelson Padilla

activity

20232026

α

Emitter Selection Techniques for

z

= 2.4, 3.1, and 4.5

15 citations · 32 across the 13 of their papers we have counts for

collaborators

Showing 2026Show all

2 papers · 1 filter

astro-ph.CO2026

Pinpointing the cosmic web between massive galaxy clusters I. The incidence of HI and OVI as WHIM tracers

Karen Martínez-Acosta, Nicolas Tejos, Ismael Pessa +6

At redshift z<1, the $Λ$ CDM paradigm predicts that $\sim$ 40-50\% of baryons reside in the warm-hot intergalactic medium (WHIM) within cosmic web filaments. Characterizing the physi…

astro-ph.GA2026★ 1 cited

ODIN: Clustering Properties of Ly $α$ Blobs at $z$ $\sim$ 2.4 and 3.1

Byeongha Moon, Yujin Yang, Eric Gawiser +18

Spatially extended Ly $α$ nebulae, known as Ly $α$ blobs (LABs), are a rare population at $z > 2$ that are thought to trace proto-groups or the progenitors of massive galaxies in the…

Pinpointing the cosmic web between massive galaxy clusters I. The incidence of HI and OVI as WHIM tracers

ODIN: Clustering Properties of Lyα Blobs at z ∼ 2.4 and 3.1

ODIN: Clustering Properties of Ly $α$ Blobs at $z$ $\sim$ 2.4 and 3.1