Search Results for author: Pablo Villanueva-Domingo

Found 9 papers, 6 papers with code

Robust field-level inference with dark matter halos

no code implementations14 Sep 2022 Helen Shao, Francisco Villaescusa-Navarro, Pablo Villanueva-Domingo, Romain Teyssier, Lehman H. Garrison, Marco Gatti, Derek Inman, Yueying Ni, Ulrich P. Steinwandel, Mihir Kulkarni, Eli Visbal, Greg L. Bryan, Daniel Angles-Alcazar, Tiago Castro, Elena Hernandez-Martinez, Klaus Dolag

More importantly, we find that our models are very robust: they can infer the value of $\Omega_{\rm m}$ and $\sigma_8$ when tested using halo catalogues from thousands of N-body simulations run with five different N-body codes: Abacus, CUBEP$^3$M, Enzo, PKDGrav3, and Ramses.

Learning cosmology and clustering with cosmic graphs

1 code implementation28 Apr 2022 Pablo Villanueva-Domingo, Francisco Villaescusa-Navarro

We train deep learning models on thousands of galaxy catalogues from the state-of-the-art hydrodynamic simulations of the CAMELS project to perform regression and inference.

Clustering

Inferring halo masses with Graph Neural Networks

1 code implementation16 Nov 2021 Pablo Villanueva-Domingo, Francisco Villaescusa-Navarro, Daniel Anglés-Alcázar, Shy Genel, Federico Marinacci, David N. Spergel, Lars Hernquist, Mark Vogelsberger, Romeel Dave, Desika Narayanan

Furthermore, a GNN trained on a suite of simulations is able to preserve part of its accuracy when tested on simulations run with a different code that utilizes a distinct subgrid physics model, showing the robustness of our method.

Graph Learning

Removing Astrophysics in 21 cm maps with Neural Networks

1 code implementation25 Jun 2020 Pablo Villanueva-Domingo, Francisco Villaescusa-Navarro

From these simulations we produce tens of thousands of 21 cm maps at redshifts $10\leq z\leq 20$.

Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies

On the maximum amplitude of the high-redshift 21-cm absorption feature

1 code implementation19 Dec 2019 Pablo Villanueva-Domingo, Olga Mena, Jordi Miralda-Escudé

We examine the maximum possible strength of the global 21-cm absorption dip on the Cosmic Background Radiation at high-redshift caused by the atomic intergalactic medium, when the Lyman-$\alpha$ coupling is maximum, assuming no exotic cooling mechanisms from interactions with dark matter.

Cosmology and Nongalactic Astrophysics

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