activity
19952026
most citedEvolution of asymptotic giant branch stars II. Optical to far-infrared isochrones with improved TP-AGB models

1.5k citations · 9.1k across the 141 of their papers we have counts for

collaborators

138 papers

astro-ph.IM2026

Toward the Italian Astronomical Community's Contribution to HWO: Science, Technology, and Instrument Concepts

A. Fontana, F. Annibali, N. Antonietti +101

This paper summarizes the interest of the Italian astronomical community in the possible participation in the development of the Habitable Worlds Observatory (HWO). It is largely b…

astro-ph.GA2026

The abundance and emission of PAHs from the local to early Universe

Massimiliano Parente, Desika Narayanan, Paul Torrey +8

We present the first large-volume cosmological simulation of galaxy evolution with a model for the abundance and luminous emission of Polycyclic Aromatic Hydrocarbons (PAHs) across…

astro-ph.IM2026

The OpenGadget3 Code for Cosmological Simulations

Klaus Dolag, Geray S. Karademir, Luca Tornatore +28

We present the public release of OpenGadget3 (OG3), a substantially extended and re-organised version of the widely used Gadget-2/3 family of cosmological simulation codes. Since G…

astro-ph.CO2026

Dianoga simulations of galaxy clusters and groups: Properties of the baryonic components

Stefano Borgani, Alice Damiano, Elena Rasia +12

We introduce the Dianoga set of cosmological simulations of galaxy clusters and groups, specifically aimed at studying the impact of the implementation of AGN feedback and star for…

astro-ph.GA2026

The Drivers of Cosmic Dust Temperature Evolution

Massimiliano Parente, Francesco Salvestrini, Gian Luigi Granato +7

Observations of the rest-frame far-infrared (far-IR) emission of galaxies suggest a mild increase of dust temperature with redshift, although constraining $T_{\rm du…

astro-ph.GA2025★ 2 cited

High [OI] emission lines: ColdSIM simulations and ALMA observations

Massimiliano Parente, Manuela Bischetti, Umberto Maio +8

Neutral-oxygen [OI] far-infrared emission lines at m and m are powerful probes of the physical conditions in the interstellar medium, although they have not been fully e…