Despite their relative sparseness, during the recent years it has become more and more
clear that extragalactic radio sources (both AGN and star-forming galaxies) constitute an …

The Low Frequency Array (LOFAR) is an ideal instrument to conduct deep extragalactic
surveys. It has a large field of view and is sensitive to large-scale and compact emission. It …

Source classifications, stellar masses, and star-formation rates are presented for≈ 80 000
radio sources from the first data release of the Low Frequency Array Two-metre Sky Survey …

The second data release of the LOFAR Two-Metre Sky Survey (LoTSS) covers 27% of the
northern sky, with a total area of~ 5700 deg 1. The high angular resolution of LOFAR with …

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 …

The LOFAR Two-metre Sky Survey (LoTSS) will cover the full northern sky and, additionally,
aims to observe the LoTSS deep fields to a noise level of≲ 10 μJy beam− 1 over several …

In this paper, we present photometric redshift (photo-z) estimates for the Dark Energy
Spectroscopic Instrument (DESI) Legacy Imaging Surveys, currently the most sensitive …

In this paper, we investigate the relationship between 150 MHz luminosity and the star-
formation rate–the SFR-L 150 MHz relation–using 150 MHz measurements for a near …

Radio-loud active galaxies have two accretion modes [radiatively inefficient (RI) and
radiatively efficient (RE)], with distinct optical and infrared signatures, and two jet dynamical …

ABSTRACT WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility
for the William Herschel Telescope, saw first light in late 2022. WEAVE comprises a new 2 …