collaborators

5 papers

astro-ph.GA2026

Assembly bias from nuisance to probe I: the relation between galactic conformity and the linear matter clustering

Nelson Padilla, Ivan Lacerna, Dante Paz

Two-halo galactic conformity is commonly interpreted as a manifestation of galaxy assembly bias, but its statistical structure and physical origin remain unclear. We aim to write t…

astro-ph.CO2026

CNN+FoF: application of deep learning to the identification of dark matter haloes

Soumadeep Maiti, Carlos M. Correa, Andrea Fiorilli +4

We present a deep-learning-based approach for identifying dark matter haloes in cosmological N-body simulations. Our framework consists of a volumetric Convolutional Neural Network…

astro-ph.CO2026

The Galaxy Bias Profile of Cosmic Voids:A Comparison of Void Finders

Ignacio G. Alfaro, Antonio D. Montero-Dorta, Jorge F. Bustillos +6

Cosmic voids, the largest underdense regions in the Universe, provide unique laboratories for studying galaxy formation and constitute powerful probes of cosmology. Recent work has…

astro-ph.CO2025

The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

Eleonora Di Valentino, Jackson Levi Said, Adam Riess +533

The standard model of cosmology has provided a good phenomenological description of a wide range of observations both at astrophysical and cosmological scales for several decades.…

astro-ph.GA2025

Traces of the evolution of cosmic void galaxies: An Integral Field Spectroscopy based analysis

Agustín M. Rodríguez-Medrano, Dante J. Paz, Damián Mast +2

Galaxies in the most underdense regions of the Universe, known as cosmic voids, exhibit astrophysical properties that suggest a distinct evolutionary path compared to galaxies in d…