activity
20242026
collaborators

16 papers

astro-ph.GA2026

The VariableTNG project: Unveiling the physical drivers of galaxy quenching

Ignacio G. Alfaro, Antonio D. Montero-Dorta, Hong Guo +4

Understanding the physical processes that regulate galaxy quenching is a key challenge in galaxy formation and evolution. The VariableTNG (VTNG) project provides a laboratory to in…

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

The Inner Dark-Matter Structure of Galaxies

Vicente Honorato, Antonio D. Montero-Dorta, M. Celeste Artale +1

In the framework of the CDM model, galaxies evolve within dark matter (DM) haloes, where baryonic processes modify the inner structure of the DM distribution. In particular, ba…

astro-ph.GA2026

The Evolution of the Spin Alignments of Dark Matter Halos in the Cosmic Web

David Tobar, Rory Smith, Antonio Montero-Dorta +2

We investigate the evolution of dark matter halo spin alignments with respect to cosmic filaments, exploring how halo mass, proximity to filaments, and major mergers influence thei…

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

Predicting galaxy bias using machine learning

Catalina Riveros-Jara, Antonio D. Montero-Dorta, Natália V. N. Rodrigues +6

Understanding how galaxies trace the underlying matter density field is essential for characterizing the influence of the large-scale structure on galaxy formation, being therefore…