DOI
10.48550/arXiv.2507.16707
Abstract
We present an empirical yet physically motivated simulation of realistic Lyman-๐ผ emitters (LAEs) at ๐ง โผ 2 โ 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-๐ผ radiative transfer, calibrating only three free parameters to simultaneously reproduce the observed Lyman-๐ผ luminosity function and the angular clustering. Our LAE model is further supported by its consistency with other observables such as the Lyman-๐ผ equivalent width distribution, the Lyman-๐ผ 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 Ly๐ผ 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
Recommended Citation
Khoraminezhad, Hasti; Saito, Shun; Gronke, Max; and Byrohl, Chris, "SIMULATING REALISTIC LYMAN-๐ผ EMITTERS INCLUDING THE EFFECT OF RADIATIVE TRANSFER" (2025). Research Data. 14.
https://scholarsmine.mst.edu/research_data/14
The definitive version is available at https://doi.org/10.48550/arXiv.2507.16707
Department(s)
Physics
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

This work is licensed under a Creative Commons Attribution-Share Alike 4.0 License.
Publication Date
25 November 2025
LAE_mock_w_spectra.tar.gz (2960688 kB)

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