activity
20202022
most citedThe REBELS ALMA Survey: cosmic dust temperature evolution out to z 7

131 citations · 554 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.GA202244 cited

A new look at the infrared properties of z 5 galaxies

L. Sommovigo, A. Ferrara, S. Carniani +6

Recent ALMA large surveys unveiled the presence of significant dust continuum emission in star-forming galaxies at . Unfortunately, such large programs -- i.e. ALPINE ($z\sim…

astro-ph.GA2022124 cited

The ALMA REBELS Survey: the dust content of Lyman Break Galaxies

P. Dayal, A. Ferrara, L. Sommovigo +22

We include a fully coupled treatment of metal and dust enrichment into the Delphi semi-analytic model of galaxy formation to explain the dust content of 13 Lyman Break Galaxies (LB…

astro-ph.GA2022104 cited

The ALMA REBELS Survey. Epoch of Reionization giants: properties of dusty galaxies at

A. Ferrara, L. Sommovigo, P. Dayal +27

We analyse FIR dust continuum measurements for 14 galaxies () in the ALMA REBELS LP to derive their physical properties. Our model uses three input data: (a) the UV spe…

astro-ph.GA2022131 cited

The REBELS ALMA Survey: cosmic dust temperature evolution out to z 7

L. Sommovigo, A. Ferrara, A. Pallottini +27

ALMA observations have revealed the presence of dust in the first generations of galaxies in the Universe. However, the dust temperature remains mostly unconstrained due to t…

astro-ph.GA202180 cited

Accurate dust temperature determination in a galaxy

Tom J. L. C. Bakx, Laura Sommovigo, Stefano Carniani +8

We report ALMA Band 9 continuum observations of the normal, dusty star-forming galaxy A1689-zD1 at , resulting in a 4.6 detection at GHz. For the first tim…

astro-ph.GA202171 cited

Dust temperature in ALMA $\hbox{[C $\scriptstyle\rm II $]}$-detected high- galaxies

L. Sommovigo, A. Ferrara, S. Carniani +4

At redshift the far-infrared (FIR) continuum spectra of main-sequence galaxies are sparsely sampled, often with a single data point. The dust temperature thu…