Line Intensity Mapping Prediction from the Cosmic Dawn (CoDa). III. Simulation for H<i>α</i> from Galaxies and the Intergalactic Medium During the Epoch of Reionization

Abstract The evolution of large-scale structure, galaxies and the intergalactic medium (IGM) during the Epoch of Reionization can be probed by upcoming Line Intensity Mapping (LIM) experiments, which sample in redshift and direction without needing to resolve individual galaxies. We predict the intensity and sources of hydrogen H α emission, dominated by radiative recombination following ionization by UV from the same massive stars that caused reionization, down to redshift 4.6, using the largest fully coupled, radiation-hydro simulation of galaxy formation and reionization to date, Cosmic Dawn (CoDa) III. We compute the mean intensity and VID versus redshift, including the relative contributions of galaxies and IGM. This will provide mock data to guide and interpret LIM experiments such as NASA’s SPHEREx and proposed CoDa Intensity Mapper.

Authors

Institutions

Publication Details

Journal
Research Notes of the AAS
Published
2025-04-23
DOI
https://doi.org/10.3847/2515-5172/adcea7
Citations
1
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
1.15

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Line Intensity Mapping Prediction from the Cosmic Dawn (CoDa). III. Simulation for Hα from Galaxies and the Intergalactic Medium During the Epoch of Reionization

Ilian T. Iliev, Dominique Aubert, Gustavo Yepes, Kyungjin Ahn et al.
1 citations
Research Notes of the AAS
Galaxies: Formation, Evolution, Phenomena
1.15
article

Line Intensity Mapping Prediction from the Cosmic Dawn (CoDa). III. Simulation for Hα from Galaxies and the Intergalactic Medium During the Epoch of Reionization

Ilian T. Iliev, Dominique Aubert, Gustavo Yepes, Kyungjin Ahn, Paul R. Shapiro, Stefan Gottlöber, Eugene Hyeonmin Lee, Luke Conaboy, Jenny G. Sorce, Pierre Ocvirk, Joohyun Lee, Joseph S. W. Lewis, Hyunbae Park, Romain Teyssier, Yohan Dubois, Taha Dawoodbhoy
article en
1 citations

Abstract

Abstract The evolution of large-scale structure, galaxies and the intergalactic medium (IGM) during the Epoch of Reionization can be probed by upcoming Line Intensity Mapping (LIM) experiments, which sample in redshift and direction without needing to resolve individual galaxies. We predict the intensity and sources of hydrogen H α emission, dominated by radiative recombination following ionization by UV from the same massive stars that caused reionization, down to redshift 4.6, using the largest fully coupled, radiation-hydro simulation of galaxy formation and reionization to date, Cosmic Dawn (CoDa) III. We compute the mean intensity and VID versus redshift, including the relative contributions of galaxies and IGM. This will provide mock data to guide and interpret LIM experiments such as NASA’s SPHEREx and proposed CoDa Intensity Mapper.

Research Notes of the AASVol. 9(4)
Centre National de la Recherche Scientifique (FR), University of Nottingham (GB), University of Tsukuba (JP), California Polytechnic State University (US), Chosun University (KR), University of Sussex (GB), Princeton University (US), Université de Lille (FR), Leibniz Institute for Astrophysics Potsdam (DE), Institut d'Astrophysique de Paris (FR), Observatoire astronomique de Strasbourg (FR), Sorbonne Université (FR), Universidad Autónoma de Madrid (ES), Université de Strasbourg (FR), École Centrale de Lille (FR), The University of Texas at Austin (US)
National Science Foundation, U.S. Department of Energy, National Aeronautics and Space Administration, Nuclear Safety and Security Commission
Openalex Percentile: Top 20%
Galaxies: Formation, Evolution, Phenomena
1.15
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.