activity
20142026
most citedChromatic periodic activity down to 120 MHz in a Fast Radio Burst

131 citations · 458 across the 18 of their papers we have counts for

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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…

astro-ph.HE2020★ 19 cited

The Nonstandard Properties of a "Standard" PWN: Unveiling the Mysteries of PWN G21.5-0.9 Using its IR and X-ray emission

Soichiro Hattori, Samayra M. Straal, Emily Zhang +3

The evolution of a pulsar wind nebula (PWN) depends on properties of the progenitor star, supernova, and surrounding environment. As some of these quantities are difficult to measu…

astro-ph.HE2020★ 17 cited

X-ray Spectroscopy of the Highly Magnetized Pulsar PSR J1846-0258, its Wind Nebula and Hosting Supernova Remnant Kes 75

E. V. Gotthelf, S. Safi-Harb, S. M. Straal +1

We present broad-band X-ray spectroscopy of the energetic components that make up the supernova remnant (SNR) Kesteven 75 using concurrent 2017 Aug 17-20 XMM-Newton and NuSTAR obse…

astro-ph.HE2020★ 48 cited

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★ 66 cited

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…

astro-ph.HE2020★ 7 cited

A dispersion excess from pulsar wind nebulae and supernova remnants: Implications for pulsars and FRBs

Samayra M. Straal, Liam Connor, Joeri van Leeuwen

Young pulsars and the pulsar wind nebulae (PWNe) or supernova remnants (SNRs) that surround them are some of the most dynamic and high-powered environments in our Universe. With th…