activity
20182022
most citedThe main sequence of star forming galaxies I. The local relation and its bending

124 citations · 355 across the 11 of their papers we have counts for

collaborators

21 papers

astro-ph.GA202219 cited

The ALPINE-ALMA [CII] Survey: the population of [CII]-undetected galaxies and their role in the -SFR relation

Michael Romano, L. Morselli, P. Cassata +22

The [CII] 158m emission line represents so far one of the most profitable tools for the investigation of the high-redshift galaxies in the early Universe. Being one of the brig…

astro-ph.GA202159 cited

The ALPINE-ALMA [CII] survey: The contribution of major mergers to the galaxy mass assembly at z~5

M. Romano, P. Cassata, L. Morselli +25

Galaxy mergers are thought to be one of the main mechanisms of the mass assembly of galaxies. Recently, many works have suggested a possible increase in the fraction of major merge…

astro-ph.GA2021

The ALPINE-ALMA [CII] Survey: Kinematic Diversity & Rotation in Massive Star Forming Galaxies at z~4.4-5.9

G. C. Jones, D. Vergani, M. Romano +21

While the kinematics of galaxies up to z~3 have been characterized in detail, only a handful of galaxies at high redshift (z>4) have been examined in such a way. The Atacama Large…

astro-ph.GA20219 cited

Redshift Evolution of the H2/HI Mass Ratio In Galaxies

Laura Morselli, Alvio Renzini, Andrea Enia +1

In this paper we present an attempt to estimate the redshift evolution of the molecular to neutral gas mass ratio within galaxies (at fixed stellar mass). For a sample of five near…

astro-ph.GA202010 cited

Identification of single spectral lines through supervised machine learning in a large HST survey (WISP): a pilot study for Euclid and WFIRST

I. Baronchelli, C. M. Scarlata, G. Rodighiero +13

Future surveys focusing on understanding the nature of dark energy (e.g., Euclid and WFIRST) will cover large fractions of the extragalactic sky in near-IR slitless spectroscopy. T…

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…