A fast radio burst source at a complex magnetized site in a barred galaxy
Fast radio bursts (FRBs) are highly dispersed, millisecond-duration radio bursts 1, 2, 3.
Recent observations of a Galactic FRB 4, 5, 6, 7, 8 suggest that at least some FRBs originate …
Recent observations of a Galactic FRB 4, 5, 6, 7, 8 suggest that at least some FRBs originate …
Frequency-dependent polarization of repeating fast radio bursts—implications for their origin
The polarization of fast radio bursts (FRBs), which are bright astronomical transient
phenomena, contains information about their environments. Using wide-band observations …
phenomena, contains information about their environments. Using wide-band observations …
Diverse polarization angle swings from a repeating fast radio burst source
Fast radio bursts (FRBs) are millisecond-duration radio transients, of unknown origin. Two
possible mechanisms that could generate extremely coherent emission from FRBs invoke …
possible mechanisms that could generate extremely coherent emission from FRBs invoke …
LOFAR detection of 110–188 MHz emission and frequency-dependent activity from FRB 20180916B
Z Pleunis, D Michilli, CG Bassa… - The Astrophysical …, 2021 - iopscience.iop.org
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 …
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 …
GLEAM: The galactic and extragalactic all-sky MWA survey
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 …
sky south of declination+ 25° at frequencies between 72 and 231 MHz, made with the MWA …
LOFAR: The low-frequency array
MP van Haarlem, MW Wise, AW Gunst, G Heald… - Astronomy & …, 2013 - aanda.org
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 …
The magnetic field and turbulence of the cosmic web measured using a brilliant fast radio burst
Fast radio bursts (FRBs) are millisecond-duration events thought to originate beyond the
Milky Way galaxy. Uncertainty surrounding the burst sources, and their propagation through …
Milky Way galaxy. Uncertainty surrounding the burst sources, and their propagation through …
The MeerTime Pulsar Timing Array: A census of emission properties and timing potential
MeerTime is a five-year Large Survey Project to time pulsars with MeerKAT, the 64-dish
South African precursor to the Square Kilometre Array. The science goals for the programme …
South African precursor to the Square Kilometre Array. The science goals for the programme …
Magnetic field strength in cosmic web filaments
E Carretti, V Vacca, SP O'Sullivan… - Monthly Notices of …, 2022 - academic.oup.com
We used the rotation measure (RM) catalogue derived from the LOFAR Two-metre Sky
Survey Data Release 2 (LoTSS DR2) at 144 MHz to measure the evolution with redshift of …
Survey Data Release 2 (LoTSS DR2) at 144 MHz to measure the evolution with redshift of …