activity
20112026
most citedThe LOFAR Two-metre Sky Survey - I. Survey Description and Preliminary Data Release

654 citations · 1.9k across the 17 of their papers we have counts for

collaborators

15 papers

astro-ph.GA2026★ 17 cited

The LOFAR Two-metre Sky Survey: VII. Third Data Release

T. W. Shimwell, M. J. Hardcastle, C. Tasse +99

We present the third data release of the LOFAR Two-metre Sky Survey (LoTSS-DR3). The survey images cover 88% of the northern sky and were created from 12,950 hrs of data (18.6 PB)…

astro-ph.GA2025

Spectral indices in active galactic nuclei as seen by Apertif and LOFAR

A. M. Kutkin, R. Morganti, T. A. Oosterloo +5

We present two new radio continuum images obtained with Apertif at 1.4 GHz. The images, produced with a direction-dependent calibration pipeline, cover 136 square degrees of the Lo…

astro-ph.HE2024★ 6 cited

Comprehensive analysis of the Apertif Fast Radio Burst sample: similarities with young, energetic neutron stars

Inés Pastor-Marazuela, Joeri van Leeuwen, Anna Bilous +9

Understanding the origin of fast radio bursts (FRBs) has become the main science driver of recent dedicated FRB surveys. Between July 2019 and February 2022, we carried out ALERT,…

astro-ph.CO2024★ 8 cited

Sardinia Radio Telescope observations of the Coma Cluster

M. Murgia, F. Govoni, V. Vacca +25

We present deep total intensity and polarization observations of the Coma cluster at 1.4 and 6.6 GHz performed with the Sardinia Radio Telescope. By combining the single-dish 1.4 G…

astro-ph.HE2020★ 9 cited

Reaching thermal noise at ultra-low radio frequencies: the Toothbrush radio relic downstream of the shock front

F. de Gasperin, G. Brunetti, M. Bruggen +14

Ultra-low frequency observations (<100 MHz) are particularly challenging because they are usually performed in a low signal-to-noise ratio regime due to the high sky temperature an…

astro-ph.HE2020★ 66 cited

Repeating fast radio bursts with WSRT/Apertif

L. C. Oostrum, Y. Maan, J. van Leeuwen +40

Repeating fast radio bursts (FRBs) present excellent opportunities to identify FRB progenitors and host environments, as well as decipher the underlying emission mechanism. Detaile…