COMET: Clustering Observables Modelled by Emulated perturbation Theory
Alexander Eggemeier, Benjamin Camacho-Quevedo, Andrea Pezzotta, Martin, Crocce, Rom\'an Scoccimarro, Ariel G. S\'anchez

TL;DR
COMET is a fast, accurate Gaussian process emulator for galaxy power spectrum multipoles in redshift-space, enabling efficient cosmological parameter inference with minimal loss of precision.
Contribution
It introduces COMET, a novel emulator based on perturbation theory, capable of predicting power spectrum multipoles across various cosmologies and redshifts with high accuracy and speed.
Findings
Achieves 0.1% accuracy for monopole and quadrupole
Speeds up predictions by at least two orders of magnitude
Suitable for Euclid survey precision requirements
Abstract
In this paper we present COMET, a Gaussian process emulator of the galaxy power spectrum multipoles in redshift-space. The model predictions are based on one-loop perturbation theory and we consider two alternative descriptions of redshift-space distortions: one that performs a full expansion of the real- to redshift-space mapping, as in recent effective field theory models, and another that preserves the non-perturbative impact of small-scale velocities by means of an effective damping function. The outputs of COMET can be obtained at arbitrary redshifts (up to ), for arbitrary fiducial background cosmologies, and for a large parameter space that covers the shape parameters , , and , as well as the evolution parameters , , , , and . This flexibility does not impair COMET's accuracy, since we exploit an exact degeneracy…
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