activity
20202022
most citedChromatic periodic activity down to 120 MHz in a Fast Radio Burst

131 citations · 367 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.IM2022★ 42 cited

First release of Apertif imaging survey data

Elizabeth A. K. Adams, B. Adebahr, W. J. G. de Blok +56

(Abridged) Apertif is a phased-array feed system for WSRT, providing forty instantaneous beams over 300 MHz of bandwidth. A dedicated survey program started on 1 July 2019, with th…

astro-ph.IM2022★ 6 cited

Characterising the Apertif primary beam response

H. Dénes, K. M. Hess, E. A. K. Adams +27

Context. Phased Array Feeds (PAFs) are multi element receivers in the focal plane of a telescope that make it possible to form simultaneously multiple beams on the sky by combining…

astro-ph.GA2022★ 12 cited

The Apertif science verification campaign - Characteristics of polarised radio sources

B. Adebahr, A. Berger, E. A. K. Adams +24

We analyse five early science datasets from the APERture Tile in Focus (Apertif) phased array feed system to verify the polarisation capabilities of Apertif in view of future large…

astro-ph.HE2021★ 28 cited

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★ 25 cited

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★ 131 cited

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…