Modeling of the High Column Density systems in The Lyman-Alpha Forest
T. Tan, J. Rich, E. Chaussidon, J.M. Le Goff, C. Balland, E. Armengaud, J. Aguilar, S. Ahlen, D. Bianchi, D. Brooks, T. Claybaugh, A. Cuceu, A. de la Macorra, P. Doel, J. E. Forero-Romero, E. Gazta\~naga, S. Gontcho A Gontcho, G. Gutierrez, H. K. Herrera-Alcantar, K. Honscheid

TL;DR
This paper develops a physically motivated model to account for high-column-density systems in the Lyman-alpha forest, improving the accuracy of cosmological parameter extraction from quasar spectra.
Contribution
The authors introduce a model based on the distribution and profiles of HCDs that accurately describes their impact on the Lyman-alpha forest power spectrum.
Findings
Model matches the accuracy of existing ad-hoc models
Effectively describes the scale-dependent bias caused by HCDs
Applicable to mock data with known HCD content
Abstract
The Lyman- forests observed in the spectra of high-redshift quasars can be used as a tracer of the cosmological matter density to study baryon acoustic oscillations (BAO) and the Alcock-Paczynski effect. Extraction of cosmological information from these studies requires modeling of the forest correlations. While the models depend most importantly on the bias parameters of the intergalactic medium (IGM), they also depend on the numbers and characteristics of high-column-density systems (HCDs) ranging from Lyman-limit systems with column densities to damped Lyman- systems (DLAs) with . These HCDs introduce broad damped absorption characteristic of a Voigt profile. Consequently they imprint a component on the power spectrum whose modes in the radial…
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