activity
20182020
most citedSCUBA-2 observations of candidate starbursting protoclusters selected by Planck and Herschel-SPIRE

24 citations · 34 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2020

Primordial nucleosynthesis constraints on high-z energy releases

Gianfranco De Zotti, Matteo Bonato

The cosmic microwave background (CMB) spectrum provides tight constraints on the thermal history of the universe up to . At higher redshifts thermalization pro…

astro-ph.GA2020

New constraints on the 1.4 GHz source number counts and luminosity functions in the Lockman Hole field

Matteo Bonato, Isabella Prandoni, Gianfranco De Zotti +3

We present a study of the 1173 sources brighter than Jy detected over an area of in the Lockman Hole field. Exploiting the mu…

astro-ph.GA20206 cited

SCUBA-2 overdensities associated with candidate protoclusters selected from Planck data

T. Cheng, D. L. Clements, J. Greenslade +21

We measure the 850-m source densities of 46 candidate protoclusters selected from the Planck High-z catalogue (PHz) and the Planck Catalogue of Compact Sources (PCCS) that were…

astro-ph.GA20194 cited

The unusual ISM in Blue and Dusty Gas Rich Galaxies (BADGRS)

L. Dunne, Z. Zhang, P. de Vis +12

The Herschel-ATLAS unbiased survey of cold dust in the local Universe is dominated by a surprising population of very blue (FUV-K < 3.5), dust-rich galaxies with high gas fractions…

astro-ph.GA201924 cited

SCUBA-2 observations of candidate starbursting protoclusters selected by Planck and Herschel-SPIRE

T. Cheng, D. L. Clements, J. Greenslade +21

We present SCUBA-2 850-m observations of 13 candidate starbursting protoclusters selected using Planck and Herschel data. The cumulative number counts of the 850-m sources in…

astro-ph.GA2018

VALES V: A kinematic analysis of the molecular gas content in -ATLAS galaxies at using ALMA

J. Molina, Edo Ibar, V. Villanueva +19

We present Atacama Large Millimeter/submillimeter Array (ALMA) resolved observations of molecular gas in galaxies up to to characterise the role of global galactic dynamic…