activity
20142019
most citedThe dust production rate of AGB stars in the Magellanic Clouds

110 citations · 539 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR201930 cited

AGB dust and gas ejecta in extremely metal-poor environments

F. Dell'Agli, R. Valiante, D. Kamath +2

We present asymptotic giant branch (AGB) models of metallicity and , with the aim of understanding how the gas enrichment and the dust production cha…

astro-ph.GA201642 cited

Faint progenitors of luminous quasars: why don't we see them?

Edwige Pezzulli, Rosa Valiante, Maria C. Orofino +3

Observational searches for faint active nuclei at have been extremely elusive, with a few candidates whose high- nature is still to be confirmed. Interpreting this lack…

astro-ph.GA2016108 cited

Limits on Pop III star formation with the most iron-poor stars

M. de Bennassuti, S. Salvadori, R. Schneider +2

We study the impact of star-forming mini-haloes, and the Initial Mass Function (IMF) of Population III (Pop III) stars, on the Galactic halo Metallicity Distribution Function (MDF)…

astro-ph.GA201658 cited

Interpreting the evolution of galaxy colours from to

Mattia Mancini, Raffaella Schneider, Luca Graziani +4

We attempt to interpret existing data on the evolution of the UV luminosity function and UV colours, , of galaxies at , to improve our understanding of their du…

astro-ph.GA2014100 cited

Decoding the stellar fossils of the dusty Milky Way progenitors

Matteo de Bennassuti, Raffaella Schneider, Rosa Valiante +1

We investigate the metallicity distribution function (MDF) in the Galactic halo and the relative fraction of Carbon-normal and Carbon-rich stars. To this aim, we use an improved ve…

astro-ph.GA201491 cited

High-redshift quasars host galaxies: is there a stellar mass crisis?

Rosa Valiante, Raffaella Schneider, Stefania Salvadori +1

We investigate the evolutionary properties of a sample of quasars at 5<z<6.4 using the semi-analytical hierarchical model GAMETE/QSOdust. We find that the observed properties of th…