activity
20142026
most citedBaryons in the CosmicWeb of IllustrisTNG - I: Gas in Knots, Filaments, Sheets and Voids

201 citations · 1.9k across the 69 of their papers we have counts for

collaborators

70 papers

astro-ph.HE2026

Linking high-mass X-ray binaries to binary compact object mergers in Milky Way-like galaxies

Felipe Vivanco Cádiz, M. Celeste Artale, Nicola Masetti +5

High-mass X-ray binaries (HMXBs) constitute a potential intermediate phase connecting massive stellar binaries to the formation of coalescing binary compact objects (BCOs). Yet, th…

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 S-PLUS Fornax Project (S+FP): Fornax-like clusters in cosmological hydrodynamical simulations

L. J. Zenocratti, A. V. Smith Castelli, M. E. De Rossi +12

The Fornax galaxy cluster constitutes a suitable laboratory to explore the evolution of galaxies in a dense environment. Recently, the Southern Photometric Local Universe Survey (S…

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, bar…

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.GA2026

ODIN: Confirmation and 3D Reconstruction of Six Massive Protoclusters at Cosmic Noon

Ashley Ortiz, Vandana Ramakrishnan, Kyoung-Soo Lee +64

Protoclusters represent sites of accelerated galaxy formation and extreme astrophysical activity characteristic of dense environments. Identifying massive protoclusters and mapping…

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…

astro-ph.CO2026

Probing Cosmic Expansion and Early Universe with Einstein Telescope

Angelo Ricciardone, Mairi Sakellariadou, Archisman Ghosh +52

Over the next two decades, gravitational-wave (GW) observations are expected to evolve from a discovery-driven endeavour into a precision tool for astrophysics, cosmology, and fund…

astro-ph.HE2025

Uncovering the population of compact binary mergers and their formation pathways with gravitational waves through the Einstein Telescope

M. Arca-Sedda, I. Dvorkin, G. Franciolini +19

Ground-based gravitational-wave (GW) observatories have transformed our view of compact-object mergers, yet their reach still limits a comprehensive reconstruction of the processes…

astro-ph.GA2025★ 1 cited

ODIN: Using multiplicity of Lyman-Alpha Emitters to assess star formation activity in dark matter halos

M. Candela Cerdosino, Nelson Padilla, Ana Laura O'Mill +16

We investigate if systems of multiple Lyman-alpha emitters (LAEs) can serve as a proxy for dark matter halo mass, assess how their radiative properties relate to the underlying hal…

astro-ph.GA2025

ODIN: Characterizing the Three-dimensional Structure of Two Protocluster Complexes at

Vandana Ramakrishnan, Ashley Ortiz, Byeongha Moon +52

We present a detailed study of the 3D morphology of two extended associations of multiple protoclusters at . These protocluster 'complexes', designated COSMOS-z3.1-A and COS…

astro-ph.CO2025★ 1 cited

Modeling gravitational wave sources in the MillenniumTNG simulations

Federico Marinacci, Marco Baldi, Giuliano Iorio +5

(Edited) We introduce a flexible framework for building gravitational wave (GW) event catalogs in hydrodynamic simulations of galaxy formation. Our framework couples the state-of-t…

astro-ph.GA2025

Bar Evolution in Edge-on Galaxies: A Demographic Study of Boxy/Peanut Bulges

Atul A. Samanta, Ankit Kumar, Mousumi Das +1

Boxy/peanut and X-shaped (BP/X) bulges are prominent features in edge-on disk galaxies and are believed to be vertically thickened bars. Despite their relevance in bar evolution, a…

astro-ph.SR2025★ 6 cited

New insight into the variability of the Be star Aquarii: Determination of stellar and disk parameters

D. Concha, C. Arcos, D. Turis-Gallo +4

The Be star Aquarii shows peculiar Cas-type X-ray emission, likely caused by its outer disk interacting with a low-mass companion, probably a white dwarf. We study the long…

astro-ph.GA2025★ 1 cited

Massive Star Clusters in the Semi-Analytical Galaxy Formation Model L-Galaxies 2020

Nils Hoyer, Silvia Bonoli, Nate Bastian +7

It is established that there exists a direct link between the formation history of star cluster populations and their host galaxies. However, our lack of understanding of the assem…

astro-ph.GA2025★ 11 cited

ODIN: Clustering Analysis of 14,000 Lyα Emitting Galaxies at z=2.4, 3.1, and 4.5

Danisbel Herrera, Eric Gawiser, Barbara Benda +15

Lyman Alpha Emitters (LAEs) are star-forming galaxies that efficiently probe the spatial distribution of galaxies in the high redshift universe. The spatial clustering of LAEs refl…

astro-ph.GA2025★ 5 cited

Central galaxy alignments. Dependence on the mass and the large-scale environment

Facundo Rodriguez, Manuel Merchán, Daniela Galárraga-Espinosa +4

Observations indicate that central galaxies show a significant alignment of their main shape axes with other galaxies in their group, as well as with the large-scale structure of t…

gr-qc2025★ 97 cited

The Science of the Einstein Telescope

Adrian Abac, Raul Abramo, Simone Albanesi +485

Einstein Telescope (ET) is the European project for a gravitational-wave (GW) observatory of third-generation. In this paper we present a comprehensive discussion of its science ob…

astro-ph.GA2024

A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution

D. Stoppacher, A. D. Montero-Dorta, M. C. Artale +4

Investigating the assembly history of the most massive and passive galaxies will enhance our understanding of why galaxies exhibit such a remarkable diversity in structure and morp…

astro-ph.GA2024★ 4 cited

The VANDELS Survey: Star formation and quenching in two over-densities at 3 < z < 4

M. Espinoza Ortiz, L. Guaita, R. Demarco +11

Context: Understanding galaxy evolution in dense environments, particularly proto-clusters, is crucial for studying mechanisms driving star formation and quenching. Aims: This stud…

astro-ph.GA2024★ 5 cited

Quenching of Galaxies at Cosmic Noon: Understanding the Effect of Environment

Akriti Singh, Lucia Guaita, Pascale Hibon +16

The aim of this study is to identify quiescent galaxies in the 2-deg COSMOS field at and analyze their environment. Using data from the ODIN survey and COSMOS2020…

astro-ph.GA2024

ODIN: Strong Clustering of Protoclusters at Cosmic Noon

Vandana Ramakrishnan, Kyoung-Soo Lee, Nicole Firestone +15

The One-hundred-deg DECam Imaging in Narrowbands (ODIN) survey is carrying out a systematic search for protoclusters during Cosmic Noon, using Ly-emitting galaxies (LAEs) as…

astro-ph.CO2024★ 6 cited

Exploring the physical origins of halo assembly bias from early times

Antonio D. Montero-Dorta, Sergio Contreras, M. Celeste Artale +2

The large-scale linear halo bias encodes the relation between the clustering of dark-matter (DM) halos and that of the underlying matter density field. Although the primary depende…