Abstract The Canadian Hydrogen Intensity Mapping Experiment (CHIME) is a drift scan
radio telescope operating across the 400–800 MHz band. CHIME is located at the Dominion …

We review the properties and nature of luminous high-redshift radio galaxies (HzRGs, z> 2)
and the environments in which they are located. HzRGs have several distinct constituents …

The LOFAR Two-metre Sky Survey (LoTSS) is a deep 120–168 MHz imaging survey that will
eventually cover the entire northern sky. Each of the 3170 pointings will be observed for 8 h …

We present the first full release of a survey of the 150 MHz radio sky, observed with the Giant
Metrewave Radio Telescope (GMRT) between April 2010 and March 2012 as part of the …

Astronomical wide-field imaging of interferometric radio data is computationally expensive,
especially for the large data volumes created by modern non-coplanar many-element …

GLEAM, the GaLactic and Extragalactic All-sky MWA survey, is a survey of the entire radio
sky south of declination+ 25° at frequencies between 72 and 231 MHz, made with the MWA …

LOFAR, the LOw-Frequency ARray, is a new-generation radio interferometer constructed in
the north of the Netherlands and across europe. Utilizing a novel phased-array design …

We present the first wide area (19 deg2), deep (≈ 120–150 μJy beam− 1), high-resolution
(5.6× 7.4 arcsec) LOFAR High Band Antenna image of the Boötes field made at 130–169 …

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 …

We use the largest complete sample of 64 galaxy clusters (HIghest X-ray FLUx Galaxy
Cluster Sample) with available high-quality X-ray data from Chandra, and apply 16 cool …