Simulating intergalactic gas for DESI-like small scale Lyman{\alpha} forest observations
Michael Walther, Eric Armengaud, Corentin Ravoux, Nathalie, Palanque-Delabrouille, Christophe Y\`eche, Zarija Luki\'c

TL;DR
This paper evaluates the accuracy and robustness of hydrodynamical simulations for modeling the Lyman-alpha forest in preparation for DESI survey data, introducing methods to improve parameter inference.
Contribution
It compares grid-based and SPH-based simulation codes, performs convergence tests, and employs Gaussian process emulation for efficient parameter space exploration.
Findings
Nyx and Gadget codes produce consistent P1D predictions.
Resolution and box size significantly affect simulation accuracy.
Gaussian process emulation enables unbiased parameter constraints.
Abstract
Measurements of the Ly forest based on large numbers of quasar spectra from sky surveys such as SDSS/eBOSS accurately probe the distribution of matter on small scales and thus provide important constraints on several ingredients of the cosmological model. A main summary statistic derived from those measurements is the one-dimensional power spectrum, P1D, of the Ly absorption. However, model predictions for P1D rely on expensive hydrodynamical simulations of the intergalactic medium, which was the limiting factor in previous analyses. Datasets from upcoming surveys such as DESI will push observational accuracy near the 1%-level and probe even smaller scales. This observational push mandate seven more accurate simulations as well as more careful exploration of parameter space. In this work we evaluate the robustness and accuracy of simulations and the statistical framework…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
