140 citations · 603 across the 10 of their papers we have counts for
12 papers · 1 filter
The VLA Frontier Fields Survey: Deep, High-resolution Radio Imaging of the MACS Lensing Clusters at 3 and 6 GHz
I. Heywood, E. J. Murphy, E. F. Jiménez-Andrade +9
The Frontier Fields project is an observational campaign targeting six galaxy clusters, with the intention of using the magnification provided by gravitational lensing to study gal…
Fast rotating and low-turbulence discs at : Dynamical evidence of their evolution into local early-type galaxies
F. Fraternali, A. Karim, B. Magnelli +3
Massive starburst galaxies in the early Universe are estimated to have depletion times of Myr and thus be able to convert their gas very quickly into stars, possibly lea…
Turbulent Gas in Lensed Planck-selected Starbursts at redshifts 1-3.5
Kevin C. Harrington, Axel Weiss, Min S. Yun +26
Dusty star-forming galaxies at high redshift (1 < z < 3) represent the most intense star-forming regions in the Universe. Key aspects to these processes are the gas heating and coo…
The VLA-COSMOS 3 GHz Large Project: Evolution of specific star formation rates out to
Sarah Leslie, Eva Schinnerer, Daizhong Liu +17
We provide a coherent, uniform measurement of the evolution of the logarithmic star formation rate (SFR) - stellar mass () relation, called the main sequence of star-forming g…
The redshift and star formation mode of AzTEC2: a pair of massive galaxies at
E. F. Jiménez-Andrade, J. A. Zavala, B. Magnelli +14
We combine observations from the Atacama Large Millimeter/submillimeter Array (ALMA) and the NOrthern Extended Millimeter Array (NOEMA) to assess the redshift and to study the star…
ACOSMOS: The Dust Attenuation of Star-Forming Galaxies at from the COSMOS-ALMA Archive
Yoshinobu Fudamoto, P. A. Oesch, B. Magnelli +7
We present an analysis of the dust attenuation of star forming galaxies at through the relationship between the UV spectral slope (), stellar mass () and t…