activity
20202022
most citedFirst release of Apertif imaging survey data

42 citations · 111 across the 7 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE2022

A fast radio burst with sub-millisecond quasi-periodic structure

Inés Pastor-Marazuela, Joeri van Leeuwen, Anna Bilous +31

Fast radio bursts (FRBs) are extragalactic radio transients of extraordinary luminosity. Studying the diverse temporal and spectral behaviour recently observed in a number of FRBs…

astro-ph.HE2021

Dual-frequency single-pulse study of PSR B0950+08

A. V. Bilous, J. M. Griessmeier, T. Pennucci +33

PSR B0950+08 is a bright non-recycled pulsar whose single-pulse fluence variability is reportedly large. Based on observations at two widely separated frequencies, 55 MHz (NenuFAR)…

astro-ph.HE2021

A search for radio emission from double-neutron star merger GW190425 using Apertif

Olivér Boersma, Joeri van Leeuwen, Elizabeth A. K. Adams +26

Detection of the electromagnetic emission from coalescing binary neutron stars (BNS) is important for understanding the merger and afterglow. We present a search for a radio counte…

astro-ph.HE2020

Chromatic periodic activity down to 120 MHz in a Fast Radio Burst

Inés Pastor-Marazuela, Liam Connor, Joeri van Leeuwen +34

Fast radio bursts (FRBs) are extragalactic astrophysical transients whose brightness requires emitters that are highly energetic, yet compact enough to produce the short, milliseco…

astro-ph.HE2020

A bright, high rotation-measure FRB that skewers the M33 halo

Liam Connor, Joeri van Leeuwen, L. C. Oostrum +37

We report the detection of a bright fast radio burst, FRB\,191108, with Apertif on the Westerbork Synthesis Radio Telescope (WSRT). The interferometer allows us to localise the FRB…

astro-ph.HE2020

Repeating fast radio bursts with WSRT/Apertif

L. C. Oostrum, Y. Maan, J. van Leeuwen +40

Repeating fast radio bursts (FRBs) present excellent opportunities to identify FRB progenitors and host environments, as well as decipher the underlying emission mechanism. Detaile…