activity
20042024
most citedA Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34

609 citations · 5.8k across the 89 of their papers we have counts for

collaborators
Showing 2022Show all

11 papers · 1 filter

astro-ph.GA2022

Kiloparsec-scale imaging of the CO(1-0)-traced cold molecular gas reservoir in a z~3.4 submillimeter galaxy

Marta Frias Castillo, Matus Rybak, Jacqueline Hodge +9

We present a high-resolution study of the cold molecular gas as traced by CO(1-0) in the unlensed z3.4 submillimeter galaxy SMM J13120+4242, using multi-configuration observa…

astro-ph.GA20222 cited

The Nature of 500 Micron Risers II: Sub-mm Faint Dusty Star Forming Galaxies

J. Cairns, D. L. Clements, J. Greenslade +6

We present SCUBA-2 and SMA follow-up observations of four candidate high redshift Dusty Star-Forming Galaxies, selected as sources with rising SEDs in the 250, 350 and 500m Hers…

astro-ph.GA2022

Dense Gas History of the Universe: from ASPECS to the ngVLA

C. L. Carilli, F. Walter, R. Decarli +7

We review the evolution of the cosmic average molecular gas density to large look-back times, using observations of rotational transitions of CO. Molecular gas is the fuel for star…

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.GA202210 cited

Tomography of the environment of the COSMOS/AzTEC-3 submillimeter galaxy at z=5.3 revealed by Lyalpha and MUSE observations

L. Guaita, M. Aravena, S. Gurung-Lopez +8

We study the members of the protocluster around AzTEC3 submillimeter galaxy at z=5.3. We analyzed the data from the MUSE instrument in an area of 1.4x1.4 arcmin^2 around AzTEC3 and…