ODIN: Identifying Protoclusters and Cosmic Filaments Traced by Lyα-emitting Galaxies

Abstract To understand the formation and evolution of massive cosmic structures, studying them at high redshift, in the epoch when they formed the majority of their mass, is essential. The One-hundred-deg 2 DECam Imaging in Narrowbands (ODIN) survey is undertaking the widest-area narrowband program to date, to use Ly α -emitting galaxies (LAEs) to trace the large-scale structure (LSS) of the Universe on the scale of 10–100 cMpc at three cosmic epochs. In this work, we present results at z = 3.1 based on early ODIN data in the COSMOS field. We identify protoclusters and cosmic filaments using multiple methods and discuss their strengths and weaknesses. We then compare our observations against the IllustrisTNG suite of cosmological hydrodynamical simulations. The two are in excellent agreement, identifying a similar number and angular size of structures above a specified density threshold. We successfully recover the simulated protoclusters with log( M z =0 / M ⊙ ) ≳ 14.4 in ∼60% of the cases. With these objects, we show that the descendant masses of our observed protoclusters can be estimated purely based on our 2D measurements, finding a median z = 0 mass of ∼10 14.5 M ⊙ . The lack of information on the radial extent of each protocluster introduces a ∼0.4 dex uncertainty in its descendant mass. Finally, we show that the recovery of the cosmic web in the vicinity of protoclusters is both efficient and accurate. The similarity of our observations and the simulations implies that our structure selection is likewise robust and efficient, demonstrating that LAEs are reliable tracers of the LSS.

Authors

Publication Details

Journal
The Astrophysical Journal
Published
2024-12-01
DOI
https://doi.org/10.3847/1538-4357/ad83cb
Citations
12
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
3.98

Funders

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article

ODIN: Identifying Protoclusters and Cosmic Filaments Traced by Lyα-emitting Galaxies

Yi-Kuan Chiang, Seong-Kook Lee, Byeongha Moon, Robin Ciardullo et al.
12 citations
The Astrophysical Journal
Galaxies: Formation, Evolution, Phenomena
3.98
article

ODIN: Identifying Protoclusters and Cosmic Filaments Traced by Lyα-emitting Galaxies

Yi-Kuan Chiang, Seong-Kook Lee, Byeongha Moon, Robin Ciardullo, S.-L. Kim, P. Troncoso, L. Guaita, Yujin Yang, Vandana Ramakrishnan, F. Valdés, Ankit Kumar, Woong-Seob Jeong, Changbom Park, Nelson Padilla, Roxana Popescu, M. Celeste Artale, Ho Seong Hwang, Arjun T. Dey, Kyoung-Soo Lee, Sang Hyeok Im, Ann I. Zabludoff, Eric Gawiser, Alexandra Pope, C. Gronwall, Hyunmi Song, Jaehyun Lee, Akriti Singh
article en
12 citations

Abstract

Abstract To understand the formation and evolution of massive cosmic structures, studying them at high redshift, in the epoch when they formed the majority of their mass, is essential. The One-hundred-deg 2 DECam Imaging in Narrowbands (ODIN) survey is undertaking the widest-area narrowband program to date, to use Ly α -emitting galaxies (LAEs) to trace the large-scale structure (LSS) of the Universe on the scale of 10–100 cMpc at three cosmic epochs. In this work, we present results at z = 3.1 based on early ODIN data in the COSMOS field. We identify protoclusters and cosmic filaments using multiple methods and discuss their strengths and weaknesses. We then compare our observations against the IllustrisTNG suite of cosmological hydrodynamical simulations. The two are in excellent agreement, identifying a similar number and angular size of structures above a specified density threshold. We successfully recover the simulated protoclusters with log( M z =0 / M ⊙ ) ≳ 14.4 in ∼60% of the cases. With these objects, we show that the descendant masses of our observed protoclusters can be estimated purely based on our 2D measurements, finding a median z = 0 mass of ∼10 14.5 M ⊙ . The lack of information on the radial extent of each protocluster introduces a ∼0.4 dex uncertainty in its descendant mass. Finally, we show that the recovery of the cosmic web in the vicinity of protoclusters is both efficient and accurate. The similarity of our observations and the simulations implies that our structure selection is likewise robust and efficient, demonstrating that LAEs are reliable tracers of the LSS.

The Astrophysical JournalVol. 977(1)
National Science Foundation
Openalex Percentile: Top 6%
Galaxies: Formation, Evolution, Phenomena
3.98
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