The effect of quasar redshift errors on Lyman-α forest correlation functions. Issue 1 (29th July 2022)

• Record Type: Journal Article
• Authors: Youles, Samantha; Bautista, Julian E; Font-Ribera, Andreu; Bacon, David; Rich, James; Brooks, David; Davis, Tamara M; Dawson, Kyle; de la Macorra, Axel; Dhungana, Govinda; Doel, Peter; Fanning, Kevin; Gaztañaga, Enrique; Gontcho A Gontcho, Satya; Gonzalez-Morales, Alma X; Guy, Julien; Honscheid, Klaus; Iršič, Vid; Kehoe, Robert; Kirkby, David; Kisner, Theodore; Landriau, Martin; Le Guillou, Laurent; Levi, Michael E; Martini, Paul; Muñoz-Gutiérrez, Andrea; Palanque-Delabrouille, Nathalie; Pérez-Ràfols, Ignasi; Poppett, Claire; Ramírez-Pérez, César; Schubnell, Michael; Tarlé, Gregory; Walther, Michael;
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 516:Issue 1(2022)
• Page Start: 421
• Page End: 433
• Publication Date: 2022-07-29
• Subjects: large-scale structure of Universe -- cosmology: theory; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stac2102
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: Using synthetic Lyman-α forests from the Dark Energy Spectroscopic Instrument (DESI) survey, we present a study of the impact of errors in the estimation of quasar redshift on the Lyman-α correlation functions. Estimates of quasar redshift have large uncertainties of a few hundred km s −1 due to the broadness of the emission lines and the intrinsic shifts from other emission lines. We inject Gaussian random redshift errors into the mock quasar catalogues, and measure the auto-correlation and the Lyman-α-quasar cross-correlation functions. We find a smearing of the BAO feature in the radial direction, but changes in the peak position are negligible. However, we see a significant unphysical correlation for small separations transverse to the line of sight which increases with the amplitude of the redshift errors. We interpret this contamination as a result of the broadening of emission lines in the measured mean continuum, caused by quasar redshift errors, combined with the unrealistically strong clustering of the simulated quasars on small scales.