collaborators

5 papers

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.GA2025

Galaxy-halo internal alignments across cosmic time

Agustina V. Marsengo-Colazo, Facundo Rodriguez, Manuel Merchán

Investigations of intrinsic alignments suggest a link between the alignment of a central galaxy's major axis with the galaxy distribution and its internal galaxy-halo shape alignme…

astro-ph.CO2025

The invariance of group occupation across the cosmic web

Vicente Izzo Dominguez, Facundo Rodriguez, Antonio D. Montero-Dorta

Recent efforts to identify secondary variations in the Halo Occupation Distribution (HOD) have primarily focused on simulations examining the role of large-scale cosmic environment…

astro-ph.GA2025

The evolution of the halo occupation distribution in cosmic voids

Ignacio G. Alfaro, Facundo Rodriguez, Andrés N. Ruiz

The halo occupation distribution is a cornerstone in understanding galaxy formation within the large-scale structure.On the other hand, in the context of the large-scale structure…

astro-ph.CO2025

The galaxy bias profile of cosmic voids

Antonio D. Montero-Dorta, Andrés Balaguera-Antolínez, Ignacio G. Alfaro +7

Cosmic voids are underdense regions within the large-scale structure of the Universe, spanning a wide range of physical scales - from a few megaparsecs (Mpc) to the largest observa…