activity
20182020
most citedThe main sequence of star forming galaxies I. The local relation and its bending

124 citations · 248 across the 6 of their papers we have counts for

collaborators

8 papers

astro-ph.GA20206 cited

The dust and cold gas content of local star forming galaxies

P. Popesso, A. Concas, L. Morselli +3

We use dust masses () derived from far-infrared data and molecular gas masses () based on CO luminosity, to calibrate proxies based on a combination of the galax…

astro-ph.GA201948 cited

Towards a deeper understanding of the physics driving galaxy quenching -- inferring trends in the gas content via extinction

Joanna Piotrowska, Asa F. L. Bluck, Roberto Maiolino +2

In order to investigate the importance of different proposed quenching mechanisms, we use an indirect method to estimate gas masses for ~62,000 SDSS DR7 galaxies. We infer gas surf…

astro-ph.SR2019

Stellar population models based on the SDSS-IV MaStar library of stellar spectra. I. Intermediate-age/old models

C. Maraston, L. Hill, D. Thomas +14

We use the first release of the SDSS/MaStar stellar library comprising ~9000, high S/N spectra, to calculate integrated spectra of stellar population models. The models extend over…

astro-ph.GA2019

The main sequence of star forming galaxies II. A non evolving slope at the high mass end

P. Popesso, L. Morselli, A. Concas +11

By using the deepest available mid and far infrared surveys in the CANDELS, GOODS and COSMOS fields we study the evolution of the Main Sequence (MS) of star forming galaxies (SFGs)…

astro-ph.GA20197 cited

Inquiring into the nature of the Abell 2667 Brightest Cluster Galaxy: physical properties from MUSE

E. Iani, G. Rodighiero, J. Fritz +21

Based on HST and MUSE data, we probe the stellar and gas properties (i.e. kinematics, stellar mass, star formation rate) of the radio-loud brightest cluster galaxy (BCG) located at…

astro-ph.GA201924 cited

A new empirical method to estimate the molecular gas mass in galaxies

Alice Concas, Paola Popesso

We find a tight correlation between the dust extinction, traced by the Balmer Decrement (BDH/H), the CO(1-0) line luminosity (L) and total molecular gas mass (M$_{H…