activity
20152023
most citedCASA, the Common Astronomy Software Applications for Radio Astronomy

1.1k citations · 4.4k across the 20 of their papers we have counts for

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Showing astro-ph.HEShow all

14 papers · 1 filter

astro-ph.HE2023

Milliarcsecond Localisation of the Hyperactive Repeating FRB 20220912A

Danté M. Hewitt, Shivani Bhandari, Benito Marcote +23

We present very-long-baseline interferometry (VLBI) observations of the hyperactive repeating FRB 20220912A using the European VLBI Network (EVN) with an EVN-Lite setup. We detecte…

astro-ph.HE2022★ 39 cited

FRB 121102: drastic changes in the burst polarization contrasts with the stability of the persistent emission

A. V. Plavin, Z. Paragi, B. Marcote +5

We study milliarcsecond-scale properties of the persistent radio counterpart to FRB 121102 and investigate the spectro-polarimetric properties of a bright burst. For the former, we…

astro-ph.HE2021★ 27 cited

Burst timescales and luminosities link young pulsars and fast radio bursts

K. Nimmo, J. W. T. Hessels, F. Kirsten +45

Fast radio bursts (FRBs) are extragalactic radio flashes of unknown physical origin. Their high luminosities and short durations require extreme energy densities, like those found…

astro-ph.HE2021★ 301 cited

A repeating fast radio burst source in a globular cluster

F. Kirsten, B. Marcote, K. Nimmo +63

Fast radio bursts (FRBs) are exceptionally luminous flashes of unknown physical origin, reaching us from other galaxies (Petroff et al. 2019). Most FRBs have only ever been seen on…

astro-ph.HE2020★ 180 cited

LOFAR Detection of 110-188 MHz Emission and Frequency-Dependent Activity from FRB 20180916B

Z. Pleunis, D. Michilli, C. G. Bassa +32

FRB 20180916B is a well-studied repeating fast radio burst source. Its proximity (~150 Mpc), along with detailed studies of the bursts, have revealed many clues about its nature --…

astro-ph.HE2020★ 94 cited

The 60 pc Environment of FRB 20180916B

Shriharsh P. Tendulkar, Armando Gil de Paz, Aida Yu. Kirichenko +18

Fast Radio Burst FRB 20180916B in its host galaxy SDSS J015800.28+654253.0 at 149 Mpc is by far the closest-known FRB with a robust host galaxy association. The source also exhibit…