Evaluating Lya Emission as a Tracer of the Largest Cosmic Structure at z~2.47

TL;DR

This study uses Lya emitters to trace and analyze the structure of a proto-supercluster at z~2.47, revealing its composition, galaxy distribution, and AGN prevalence, demonstrating LAEs as effective large-scale structure markers.

Contribution

It provides the first detailed mapping of Hyperion using LAEs, linking galaxy distribution to large-scale structure and environmental effects at high redshift.

Findings

LAE overdensity delta_g~40 indicating a massive proto-supercluster

LAE distribution traces protocluster cores and filaments

AGN are 12 times more abundant in the Hyperion region

Abstract

The discovery and spectroscopic confirmation of Hyperion, a proto-supercluster at z~2.47, provides an unprecedented opportunity to study distant galaxies in the context of their large-scale environment. We carry out deep narrow-band imaging of a ~1*1 deg^2 region around Hyperion and select 157 Lya emitters (LAEs). The inferred LAE overdensity is delta_g~40 within an effective volume of 30*20*15 cMpc^3, consistent with the fact that Hyperion is composed of multiple protoclusters and will evolve into a super-cluster with a total mass of M_tot ~1.4*10^15 M_sun at z=0. The distribution of LAEs closely mirrors that of known spectroscopic members, tracing the protocluster cores and extended filamentary arms connected to them, suggesting that they trace the same large-scale structure. By cross-correlating the LAE positions with HI tomography data, we find weak evidence that LAEs may be less abundant in the highest HI regions, perhaps because Lya is suppressed in such regions. The Hyperion region hosts a large population of active galactic nuclei (AGN), ~12 times more abundant than that in the field. The prevalence of AGN in protocluster regions hints at the possibility that they may be triggered by physical processes that occur more frequently in dense environments, such as galaxy mergers. Our study demonstrates LAEs as reliable markers of the largest cosmic structures. When combined with ongoing and upcoming imaging and spectroscopic surveys, wide-field narrow-band imaging has the potential to advance our knowledge in the formation and evolution of cosmic structures and of their galaxy inhabitants.