218 citations · 2.8k across the 98 of their papers we have counts for
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The LOFAR Two Metre Sky Survey: Deep Fields Data Release 1 -- III. Host-galaxy identifications and value added catalogues
R. Kondapally, P. N. Best, M. J. Hardcastle +40
We present the source associations, cross-identifications, and multi-wavelength properties of the faint radio source population detected in the deep tier of the LOFAR Two Metre Sky…
Constraints on the [CII] luminosity of a proto-globular cluster at z~6 obtained with ALMA
F. Calura, E. Vanzella, S. Carniani +11
We report on ALMA observations of D1, a system at z~6.15 with stellar mass M_* ~ 10^7 M_sun containing globular cluster (GC) precursors, strongly magnified by the galaxy cluster MA…
The AGN fuelling/feedback cycle in nearby radio galaxies III. 3D relative orientations of radio jets and CO discs and their interaction
I. Ruffa, R. A. Laing, I. Prandoni +4
This is the third paper of a series exploring the multi-frequency properties of a sample of eleven nearby low-excitation radio galaxies (LERGs) in the southern sky. We are conducti…
Spectro-polarimetric observations of the CIZA J2242.8+5301 northern radio relic: no evidence of high-frequency steepening
Francesca Loi, Matteo Murgia, Valentina Vacca +16
Observations of radio relics at very high frequency (>10 GHz) can help to understand how particles age and are (re-)accelerated in galaxy cluster outskirts and how magnetic fields…
The molecular gas in the central region of NGC 7213
Francesco Salvestrini, Carlotta Gruppioni, Francesca Pozzi +4
We present a multi-wavelength study (from X-ray to millimetre) of the nearby low-luminosity active galactic nucleus (LLAGN) NGC 7213. We combine the information from the different…
The high molecular gas content, and the efficient conversion of neutral into molecular gas, in jellyfish galaxies
A. Moretti, R. Paladino, B. M. Poggianti +11
In the disks of four jellyfish galaxies from the GASP sample at redshift we detect molecular gas masses systematically higher than in field galaxies. These galaxies are…