activity
19972026
most citedEvolution of asymptotic giant branch stars II. Optical to far-infrared isochrones with improved TP-AGB models

1.5k citations · 6.2k across the 58 of their papers we have counts for

collaborators

61 papers

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.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.GA2024★ 3 cited

Dust sub-millimetre emission in green valley galaxies

Massimiliano Parente, Cinthia Ragone-Figueroa, Gian Luigi Granato +5

Context. Green valley (GV) galaxies are objects defined on a colour-magnitude diagram, or a colour-mass diagram, as being associated with a transition from a star-forming to a quie…

astro-ph.GA2024★ 9 cited

GalaPy, the highly optimised C++/Python spectral modelling tool for galaxies -- I. Library presentation and photometric fitting

Tommaso Ronconi, Andrea Lapi, Martina Torsello +13

Fostered by upcoming data from new generation observational campaigns, we are about to enter a new era for the study of how galaxies form and evolve. The unprecedented quantity of…

astro-ph.GA2020★ 48 cited

Dust evolution in zoom-in cosmological simulations of galaxy formation

Gian Luigi Granato, Cinthia Ragone-Figueroa, Antonela Taverna +6

We present cosmological zoom-in hydro-dynamical simulations for the formation of disc galaxies, implementing dust evolution and dust promoted cooling of hot gas. We couple an impro…

astro-ph.GA2018★ 110 cited

Comprehensive comparison of models for spectral energy distributions from 0.1 micron to 1 mm of nearby star-forming galaxies

L. K. Hunt, I. De Looze, M. Boquien +26

We have fit the far-ultraviolet (FUV) to sub-millimeter (850 micron) spectral energy distributions (SEDs) of the 61 galaxies from the "Key Insights on Nearby Galaxies: A Far-Infrar…