Visualization of LAEs on cosmological scales: Observed intensity (blue) and star forming regions in galaxies (red).

Cosmological radiative transfer simulations of Lyman-alpha emission: the impact on the galaxy clustering

Abstract

Lyman-alpha emitters and their intensity map are powerful probes of the large-scale structure at optical and near-infrared wavelength as HETDEX plans. However, the fact that the Lyman-alpha photons are scattered due to the neutral hydrogen has non-negligible impact on the observed distribution of Lyman-alpha photons. To study this in detail, we run a suit of radiative transfer (RT) simulations on Illustris and quantify the impact of RT on the real space galaxy clustering (Behrens, CB et al. arXiv: 1710.06171).

Date
Jan 1, 2018 12:00 AM
Location
Aspen, United States
Chris Byrohl
Chris Byrohl
PhD Student

My research interests include Lyman-$\alpha$ radiation to study galaxies and the large-scale structure, supernovae type Ia and high-performance computing.