The giant radio array for neutrino detection (GRAND): Science and design
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 …
observatory of ultra-high-energy (UHE) cosmic particles, with energies exceeding 10 8 GeV …
Gravitational waves: Sources, detectors and searches
Gravitational wave science should transform in this decade from a study of what has not
been seen to a full-fledged field of astronomy in which detected signals reveal the nature of …
been seen to a full-fledged field of astronomy in which detected signals reveal the nature of …
The international pulsar timing array: first data release
The highly stable spin of neutron stars can be exploited for a variety of (astro) physical
investigations. In particular, arrays of pulsars with rotational periods of the order of …
investigations. In particular, arrays of pulsars with rotational periods of the order of …
LOFAR detection of 110–188 MHz emission and frequency-dependent activity from FRB 20180916B
The object FRB 20180916B is a well-studied repeating fast radio burst source. Its proximity
(∼ 150 Mpc), along with detailed studies of the bursts, has revealed many clues about its …
(∼ 150 Mpc), along with detailed studies of the bursts, has revealed many clues about its …
LOFAR: The low-frequency array
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 …
the north of the Netherlands and across europe. Utilizing a novel phased-array design …
Chromatic periodic activity down to 120 megahertz in a fast radio burst
Fast radio bursts (FRBs) are extragalactic astrophysical transients whose brightness
requires emitters that are highly energetic yet compact enough to produce the short …
requires emitters that are highly energetic yet compact enough to produce the short …
The green bank northern celestial cap pulsar survey. I. Survey description, data analysis, and initial results
We describe an ongoing search for pulsars and dispersed pulses of radio emission, such as
those from rotating radio transients (RRATs) and fast radio bursts, at 350 MHz using the …
those from rotating radio transients (RRATs) and fast radio bursts, at 350 MHz using the …
Gravitational wave astronomy with the SKA
On a time scale of years to decades, gravitational wave (GW) astronomy will become a
reality. Low frequency (nanoHz) GWs are detectable through long-term timing observations …
reality. Low frequency (nanoHz) GWs are detectable through long-term timing observations …
LOFAR Discovery of a 23.5 s Radio Pulsar
CM Tan, CG Bassa, S Cooper, TJ Dijkema… - The Astrophysical …, 2018 - iopscience.iop.org
We present the discovery of PSR J0250+ 5854, a radio pulsar with a spin period of 23.5 s.
This is the slowest-spinning radio pulsar known. PSR J0250+ 5854 was discovered by the …
This is the slowest-spinning radio pulsar known. PSR J0250+ 5854 was discovered by the …
Detection of repeating FRB 180916. J0158+ 65 down to frequencies of 300 MHz
We report on the detection of seven bursts from the periodically active, repeating fast radio
burst (FRB) source FRB 180916. J0158+ 65 in the 300–400 MHz frequency range with the …
burst (FRB) source FRB 180916. J0158+ 65 in the 300–400 MHz frequency range with the …