UCL Discovery Stage
UCL home » Library Services » Electronic resources » UCL Discovery Stage

Planting a Lyman alpha forest on AbacusSummit

Hadzhiyska, B; Font-Ribera, A; Cuceu, A; Chabanier, S; Aguilar, J; Brooks, D; De La Macorra, A; ... Zhou, Z; + view all (2023) Planting a Lyman alpha forest on AbacusSummit. Monthly Notices of the Royal Astronomical Society , 524 (1) pp. 1008-1024. 10.1093/mnras/stad1920. Green open access

[thumbnail of stad1920.pdf]
Preview
Text
stad1920.pdf - Published Version

Download (2MB) | Preview

Abstract

The full-shape correlations of the Lyman alpha (Ly α) forest contain a wealth of cosmological information through the Alcock-Paczyński effect. However, these measurements are challenging to model without robustly testing and verifying the theoretical framework used for analysing them. Here, we leverage the accuracy and volume of the N-body simulation suite AbacusSummit to generate high-resolution Ly α skewers and quasi-stellar object (QSO) catalogues. One of the main goals of our mocks is to aid in the full-shape Ly α analysis planned by the Dark Energy Spectroscopic Instrument (DESI) team. We provide optical depth skewers for six of the fiducial cosmology base-resolution simulations (, N = 69123) at z = 2.5. We adopt a simple recipe based on the Fluctuating Gunn-Peterson Approximation (FGPA) for constructing these skewers from the matter density in an N-body simulation and calibrate it against the 1D and 3D Ly α power spectra extracted from the hydrodynamical simulation IllustrisTNG (TNG;, N = 25003). As an important application, we study the non-linear broadening of the baryon acoustic oscillation (BAO) peak and show the cross-correlation between DESI-like QSOs and our Ly α forest skewers. We find differences on small scales between the Kaiser approximation prediction and our mock measurements of the Ly α × QSO cross-correlation, which would be important to account for in upcoming analyses. The AbacusSummit Ly α forest mocks open up the possibility for improved modelling of cross-correlations between Ly α and cosmic microwave background (CMB) lensing and Ly α and QSOs, and for forecasts of the 3-point Ly α correlation function. Our catalogues and skewers are publicly available on Globus via the National Energy Research Scientific Computing Center (NERSC) (full link under the section 'Data Availability').

Type: Article
Title: Planting a Lyman alpha forest on AbacusSummit
Open access status: An open access version is available from UCL Discovery
DOI: 10.1093/mnras/stad1920
Publisher version: https://doi.org/10.1093/mnras/stad1920
Language: English
Additional information: This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: methods: numerical – quasars: absorption lines – cosmology: theory
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery-pp.ucl.ac.uk/id/eprint/10175391
Downloads since deposit
400Downloads
Download activity - last month
Download activity - last 12 months
Downloads by country - last 12 months

Archive Staff Only

View Item View Item