DOI

10.48550/arXiv.2507.16707

Abstract

We present an empirical yet physically motivated simulation of realistic Lyman-๐›ผ emitters (LAEs) at ๐‘ง โˆผ 2 โˆ’ 3, crucial for ongoing and forthcoming cosmological LAE surveys. We combine an empirical UniverseMachine galaxy-halo model with a simple spherical expanding shell model for the Lyman-๐›ผ radiative transfer, calibrating only three free parameters to simultaneously reproduce the observed Lyman-๐›ผ luminosity function and the angular clustering. Our LAE model is further supported by its consistency with other observables such as the Lyman-๐›ผ equivalent width distribution, the Lyman-๐›ผ escape fraction as a function of stellar mass and dust reddening, and the systemic velocity offsets. Our LAE model provides predictions for the halo occupation distributions for LAEs and relationship between Ly๐›ผ luminosity and halo mass, including the distribution of satellite LAEs. Our work provides a crucial first step towards creating a high-fidelity LAE synthetic catalog for the LAE cosmology surveys. Our LAE catalog and spectra are publicly available at https://scholarsmine.mst.edu/research_data/14.

Start Date

November 2025

Department(s)

Physics

Comments

Please see the first attached supplemental file for an example of viewing the attached data set.

Subject Headings

Large-scale structureโ€” Lyman-Alpha Emitters โ€” Lyman-Alpha Radiative Transfer

Document Type

Article - Journal

Document Version

Final Version

File Format

text

Language(s)

English

Rights

ยฉ 2025 The Authors, All rights reserved

Creative Commons Licensing

Creative Commons License
This work is licensed under a Creative Commons Attribution-Share Alike 4.0 License.

Publication Date

25 November 2025

Included in

Physics Commons

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