activity
20022023
most citedCompact radio emission indicates a structured jet was produced by a binary neutron star merger

395 citations · 1.2k across the 50 of their papers we have counts for

collaborators

51 papers

astro-ph.GA2023★ 22 cited

RadioAstron Space VLBI Imaging of the jet in M87: I. Detection of high brightness temperature at 22 GHz

Jae-Young Kim, Tuomas Savolainen, Petr Voitsik +19

We present results from the first 22 GHz space very-long-baseline interferometric (VLBI) imaging observations of M87 by RadioAstron. As a part of the Nearby AGN Key Science Program…

astro-ph.GA2023★ 4 cited

Milliarcsecond Structures of Variable Peaked-Spectrum Sources

K. Ross, C. Reynolds, N. Seymour +3

Spectral variability offers a new technique to identify small scale structures from scintillation, as well as determining the absorption mechanism for peaked-spectrum (PS) radio so…

astro-ph.GA2022

The Annual Cycle in Scintillation Timescale of PMN J1726+0639

Hayley E. Bignall, Artem V. Tuntsov, Jamie Stevens +3

We discovered rapid intra-day variability in radio source PMN J1726+0639 at GHz frequencies, during a survey to search for such variability with the Australia Telescope Compact Arr…

astro-ph.HE2021★ 7 cited

The Highly Self-Absorbed Blazar, PKS\,1351018

Brian Punsly, Sandor Frey, Cormac Reynolds +5

PKS\,1351018 at a redshift of is one of the most luminous, steady synchrotron sources with a luminosity \,erg~s. The synchrotron luminosity does not s…

astro-ph.HE2021★ 14 cited

A parsec-scale faint jet in the nearby changing-look Seyfert galaxy Mrk 590

J. Yang, I. van Bemmel, Z. Paragi +9

Broad Balmer emission lines in active galactic nuclei (AGN) may display dramatic changes in amplitude, even disappearance and re-appearance in some sources. As a nearby galaxy at a…

astro-ph.GA2020★ 1 cited

Optical study of PKS B1322-110, the intra-hour variable radio source

Juan P. Madrid, Artem V. Tuntsov, Mischa Schirmer +7

Observations with the Australia Telescope Compact Array revealed intra-hour variations in the radio source PKS B1322-110 (Bignall et al. 2019). As part of an optical follow-up, we…