activity
20042026
most citedA radio ridge connecting two galaxy clusters in a filament of the cosmic web

163 citations · 3.2k across the 56 of their papers we have counts for

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10 papers · 1 filter

astro-ph.CO2026

The giant radio source 0917+75: Origin and properties

G. Giovannini, N. Biava, M. Girardi +11

Context. Several author have studied the giant radio source GRS0917 + 75 , but its origin remains unclear. Aims. This source is unusual, because of its large size and its location…

astro-ph.CO2022★ 16 cited

The thermal and non-thermal components within and between galaxy clusters Abell 399 and Abell 401

Federico Radiconi, Valentina Vacca, Elia Battistelli +28

We measure the local correlation between radio emission and Compton- signal across two galaxy clusters, Abell~399 and Abell~401, using maps from the Low-Frequency Array (LOFAR)…

astro-ph.CO2022★ 5 cited

Spectral study of the diffuse synchrotron source in the galaxy cluster Abell 523

Valentina Vacca, Timothy Shimwell, Richard A. Perley +26

The galaxy cluster Abell 523 (A523) hosts an extended diffuse synchrotron source historically classified as a radio halo. Its radio power at 1.4 GHz makes it one of the most signif…

astro-ph.CO2018★ 51 cited

Observations of a nearby filament of galaxy clusters with the Sardinia Radio Telescope

V. Vacca, M. Murgia, F. Govoni +29

We report the detection of diffuse radio emission which might be connected to a large-scale filament of the cosmic web covering a 8deg x 8deg area in the sky, likely associated wit…

astro-ph.CO2017★ 31 cited

Observations of the galaxy cluster CIZA J2242.8+5301 with the Sardinia Radio Telescope

F. Loi, M. Murgia, F. Govoni +25

We observed the galaxy cluster CIZA J2242.8+5301 with the Sardinia Radio Telescope to provide new constraints on its spectral properties at high frequency. We conducted observation…

astro-ph.CO2013★ 17 cited

The brightness and spatial distributions of terrestrial radio sources

A. R. Offringa, A. G. de Bruyn, S. Zaroubi +75

Faint undetected sources of radio-frequency interference (RFI) might become visible in long radio observations when they are consistently present over time. Thereby, they might obs…

astro-ph.CO2011★ 17 cited

LOFAR: Recent imaging results & future prospects

George Heald, Michael R. Bell, Andreas Horneffer +27

The Low Frequency Array (LOFAR) is under construction in the Netherlands and in several surrounding European countries. In this contribution, we describe the layout and design of t…

astro-ph.CO2011★ 6 cited

LOFAR: Early imaging results from commissioning for Cygnus A

John McKean, Louise Ker, Reinout J. van Weeren +19

The Low Frequency Array (LOFAR) will operate between 10 and 250 MHz, and will observe the low frequency Universe to an unprecedented sensitivity and angular resolution. The constru…

astro-ph.CO2010★ 33 cited

Low-frequency study of two giant radio galaxies: 3C35 and 3C223

E. Orrù, M. Murgia, L. Feretti +5

Radio galaxies with a projected linear size > 1 Mpc are classified as giant radio sources. According to the current interpretation these are old sources which have evolved in a low…

astro-ph.CO2009★ 14 cited

Radio spectral index images of the spiral galaxies NGC 0628, NGC 3627, and NGC 7331

R. Paladino, M. Murgia, E. Orrù

In order to understand the cosmic ray propagation mechanism in galaxies, and its correlation with the sites of star formation, we compare the spatially resolved radio spectral inde…