activity
20122022
most citedThe MUSE Hubble Ultra Deep Field Survey: I. Survey description, data reduction and source detection

348 citations · 2.1k across the 30 of their papers we have counts for

collaborators

66 papers

astro-ph.GA202237 cited

Investigating the Effect of Galaxy Interactions on Star Formation at 0.5<z<3.0

Ekta A. Shah, Jeyhan S. Kartaltepe, Christina T. Magagnoli +24

Observations and simulations of interacting galaxies and mergers in the local universe have shown that interactions can significantly enhance the star formation rates (SFR) and fue…

astro-ph.GA202241 cited

GOALS-JWST: Resolving the Circumnuclear Gas Dynamics in NGC 7469 in the Mid-Infrared

Vivian U, Thomas Lai, Marina Bianchin +35

The nearby, luminous infrared galaxy (LIRG) NGC 7469 hosts a Seyfert nucleus with a circumnuclear star-forming ring and is thus the ideal local laboratory for investigating the sta…

astro-ph.GA202216 cited

GOALS-JWST: Unveiling Dusty Compact Sources in the Merging Galaxy IIZw096

Hanae Inami, Jason Surace, Lee Armus +30

We have used the Mid-InfraRed Instrument (MIRI) on the James Webb Space Telescope (JWST) to obtain the first spatially resolved, mid-infrared (mid-IR) images of IIZw096, a merging…

astro-ph.GA202225 cited

Characterizing Compact 15-33 GHz Radio Continuum Sources in Local U/LIRGs

Y. Song, S. T. Linden, A. S. Evans +23

We present the analysis of pc-scale compact radio continuum sources detected in 63 local (Ultra) Luminous Infrared Galaxies (U/LIRGs; ), u…

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…