ODIN: Where Do Lyman-alpha Blobs Live? Contextualizing Blob Environments within the Large-Scale Structure
Vandana Ramakrishnan, Byeongha Moon, Sang Hyeok Im, Rameen Farooq,, Kyoung-Soo Lee, Eric Gawiser, Yujin Yang, Changbom Park, Ho Seong Hwang,, Francisco Valdes, Maria Celeste Artale, Robin Ciardullo, Arjun Dey, Caryl, Gronwall, Lucia Guaita, Woong-Seob Jeong, Nelson Padilla

TL;DR
This study uses a large survey to show that Lyman-alpha Blobs (LABs) are predominantly found in dense, filamentary regions of the early universe's large-scale structure, especially near protoclusters.
Contribution
It provides the first large-scale observational evidence linking LABs to specific cosmic web environments using extensive wide-field data.
Findings
LABs are located in higher-than-average density regions.
Approximately 70% of LABs are within 2.4 pMpc of a filament.
Protoclusters with LABs tend to have higher descendant masses.
Abstract
While many Lyman-alpha Blobs (LABs) are found in and around several well-known protoclusters at high redshift, how they trace the underlying large-scale structure is still poorly understood. In this work, we utilize 5,352 Lyman-alpha emitters (LAEs) and 129 LABs at z=3.1 identified over a 9.5 sq. degree area in early data from the ongoing One-hundred-deg DECam Imaging in Narrowbands (ODIN) survey to investigate this question. Using LAEs as tracers of the underlying matter distribution, we identify overdense structures as galaxy groups, protoclusters, and filaments of the cosmic web. We find that LABs preferentially reside in regions of higher-than-average density and are located in closer proximity to overdense structures, which represent the sites of protoclusters and their substructures. Moreover, protoclusters hosting one or more LABs tend to have a higher descendant mass…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Galaxies: Formation, Evolution, Phenomena
