activity
20172021
most citedA repeating fast radio burst source in a globular cluster

301 citations · 412 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2021★ 9 cited

J2102+6015: a young radio source at z = 4.575

Yingkang Zhang, Tao An, Sándor Frey +7

Jets of high-redshift active galactic nuclei (AGNs) can be used to directly probe the activity of the black holes in the early Universe. Radio sources with jets misaligned with res…

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.SR2019

Exploring the Asymmetry of the Solar Corona Electron Density with Very Long Baseline Interferometry

Dan Aksim, Alexey Melnikov, Dmitry Pavlov +1

The Sun's corona has interested researchers for multiple reasons, including the search for solution for the famous coronal heating problem and a purely practical consideration of p…

astro-ph.GA2019★ 39 cited

Detection statistics of the RadioAstron AGN survey

Y. Y. Kovalev, N. S. Kardashev, K. V. Sokolovsky +57

The largest Key Science Program of the RadioAstron space VLBI mission is a survey of active galactic nuclei (AGN). The main goal of the survey is to measure and study the brightnes…

astro-ph.GA2018★ 12 cited

High-resolution radio imaging of two luminous quasars beyond redshift 4.5

S. Frey, O. Titov, A. E. Melnikov +2

Context. Radio-loud active galactic nuclei in the early Universe are rare. The quasars J0906+6930 at redshift z=5.47 and J2102+6015 at z=4.57 stand out from the known sample with t…