collaborators

12 papers

astro-ph.GA2026

The role of filaments in the large-scale conformity signal

Daniela Palma, Ivan Lacerna, Noelia Pérez +8

We investigate the large-scale conformity signal and its connection with the large-scale structure, focusing on low-mass central galaxies, after excluding galaxies that were satell…

astro-ph.GA2026

Cluster-green galaxy correlations: where do these galaxies live?

Selene Levis, Facundo Rodriguez, Héctor J. Martínez +2

Green valley (GV) galaxies are thought to represent a transitional population between star-forming and quiescent systems. However, their spatial distribution relative to galaxy sys…

astro-ph.CO2026

Halo Occupation Distribution estimation performance for LSST data

P. Cataldi, V. Cristiani, F. Rodriguez +4

Upcoming imaging surveys, such as the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST), will enable high signal-to-noise measurements of galaxy clustering. The halo…

astro-ph.CO2026

Evolution of submillimeter galaxies across cosmic-web environments

Ankit Kumar, M. Celeste Artale, Antonio D. Montero-Dorta +12

Submillimeter galaxies (SMGs) provide valuable insights into galaxy formation and evolution and are likely influenced by their cosmic environment. However, their rarity makes envir…

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

Connecting clustering and the cosmic web:Observational constraints on secondary halo bias

Facundo Rodriguez, Antonio D. Montero-Dorta

Cosmological simulations predict significant secondary dependencies of halo clustering on internal properties and environment. Detecting these subtle signals in observational data…