Abstract The Giant Radio Array for Neutrino Detection (GRAND) is a planned large-scale
observatory of ultra-high-energy (UHE) cosmic particles, with energies exceeding 10 8 GeV …

Solar type III radio bursts are an important diagnostic tool in the understanding of solar
accelerated electron beams. They are a signature of propagating beams of nonthermal …

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 …

ABSTRACT The Large-aperture Experiment to Detect the Dark Age (LEDA) was designed to
detect the predicted O (100) mK sky-averaged absorption of the cosmic microwave …

We present the results of a recent re-reduction of the data from the Very Large Array (VLA)
Low-frequency Sky Survey (VLSS). We used the VLSS catalogue as a sky model to correct …

The recent detection of the" cosmic dawn" redshifted 21 cm signal at 78 MHz by the
Experiment to Detect the Global EoR Signatures (EDGES) differs significantly from …

We present first results from a LOFAR census of non-recycled pulsars. The census includes
almost all such pulsars known (194 sources) at declinations Dec> 8° and Galactic latitudes …

Amongst standard model parameters that are constrained by cosmic microwave background
(CMB) observations, the optical depth τ stands out as a nuisance parameter. While τ …

LWA1 is a new radio telescope operating in the frequency range 10-88 MHz, located in
central New Mexico. The telescope consists of 258 pairs of dipole-type antennas whose …

Cosmic dawn, the onset of star formation in the early universe, can in principle be studied
via the 21-cm transition of neutral hydrogen, for which a sky-averaged absorption signal …