23–29 oct. 2022
Fuseau horaire Europe/Paris

Modeling of High Column Density systems in the Ly-α Forests Correlation Function

27 oct. 2022, 17:30
30m
Cosmology Cosmology

Orateur

ting tan

Description

The Lyman-α forest is detected as the series of absorption lines in the quasar spectra, caused by the Lyman-α transitions of neutral hydrogen in the low-density, high-redshift intergalactic medium (IGM). It is a biased continuous tracer of the quasi-linear matter density field, and the auto (cross) correlation function of the forests (with quasars) has been used to detect the Baryon Acoustic Oscillations (BAO) signal. The Damped Lyman-α System (DLAs) is one of the most important systematics in the Lyman-α BAO analysis. DLAs are strong absorption regions in Lyman-alpha forests caused by neutral hydrogen along the sightline with extremely high column densities, usually log(NHI)>=20. We present an accurate model to characterize the impact of DLAs on the measurement of the Lyman-α correlation function, as well as the BAO fitting.

Auteur principal

Co-auteurs

Christophe Balland (LPNHE Paris - UPMC -ILP) James Rich (SPP) Jean-Marc Le Goff (CEA Saclay DRF/Irfu/DPhP)

Documents de présentation