activity
20162019
most citedGalaxy Evolution in the Radio Band: The Role of Starforming Galaxies and Active Galactic Nuclei

103 citations · 162 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.GA201932 cited

Cosmic evolution of star-forming galaxies to in the faint low-frequency radio source population

E. F. Ocran, A. R. Taylor, M. Vaccari +4

We study the properties of star-forming galaxies selected at 610 MHz with the GMRT in a survey covering 1.86 deg down to a noise of 7.1\,Jy / beam. These were id…

astro-ph.GA201725 cited

Angular Momentum of Early and Late Type Galaxies: Nature or Nurture?

Jingjing Shi, Andrea Lapi, Claudia Mancuso +2

We investigate the origin, the shape, the scatter, and the cosmic evolution in the observed relationship between specific angular momentum and the stellar mass

astro-ph.GA2017103 cited

Galaxy Evolution in the Radio Band: The Role of Starforming Galaxies and Active Galactic Nuclei

Claudia. Mancuso, A. Lapi, I. Prandoni +6

We investigate the astrophysics of radio-emitting star-forming galaxies and ac- tive galactic nuclei (AGNs), and elucidate their statistical properties in the radio band including…

astro-ph.GA2017

Does the evolution of the radio luminosity function of star-forming galaxies match that of the star-formation rate function?

Matteo Bonato, Mattia Negrello, Claudia Mancuso +9

The assessment of the relationship between radio continuum luminosity and star formation rate (SFR) is of crucial importance to make reliable predictions for the forthcoming ultra-…

astro-ph.GA20172 cited

Modelling the UV to radio SEDs of nearby star-forming galaxies: new Parsec SSP for Grasil

I. A. Obi, A. Bressan, F. Perrotta +9

By means of the updated PARSEC database of evolutionary tracks of massive stars, we compute the integrated stellar light, the ionizing photon budget and the supernova rates of youn…

astro-ph.GA2016

The Quest for Dusty Star-forming Galaxies at High Redshift z>4

C. Mancuso, A. Lapi, J. Shi +3

We exploit the continuity equation approach and the `main sequence' star-formation timescales to show that the observed high abundance of galaxies with stellar masses > a few 10^10…