activity
20102023
most citedCoincidence of a high-fluence blazar outburst with a PeV-energy neutrino event

248 citations · 507 across the 23 of their papers we have counts for

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Showing astro-ph.GAShow all

7 papers · 1 filter

astro-ph.GA2022★ 9 cited

Inverse MultiView II: Microarcsecond Trigonometric Parallaxes for Southern Hemisphere 6.7~GHz Methanol Masers G232.62+00.99 and G323.7400.26

Lucas J. Hyland, Mark J. Reid, Gabor Orosz +11

We present the first results from the Southern Hemisphere Parallax Interferometric Radio Astrometry Legacy Survey (\spirals): as-accurate parallaxes and proper motions for two…

astro-ph.GA2022★ 17 cited

Unprecedented change in the position of four radio sources

Oleg Titov, Sándor Frey, Sébastien Lambert +7

Astrometric positions of radio-emitting active galactic nuclei (AGNs) can be determined with sub-milliarcsec accuracy using very long baseline interferometry (VLBI). The usually sm…

astro-ph.GA2020★ 24 cited

The GLEAM 4-Jy (G4Jy) Sample: I. Definition and the catalogue

Sarah V. White, Thomas M. O. Franzen, Chris J. Riseley +21

The Murchison Widefield Array (MWA) has observed the entire southern sky (Declination, 30 deg) at low radio-frequencies, over the range 72-231 MHz. These observations constitu…

astro-ph.GA2020★ 25 cited

The GLEAM 4-Jy (G4Jy) Sample: II. Host-galaxy identification for individual sources

Sarah V. White, Thomas M. O. Franzen, Chris J. Riseley +20

The entire southern sky (Declination, 30 deg) has been observed using the Murchison Widefield Array (MWA), which provides radio imaging of 2-arcmin resolution at low fre…

astro-ph.GA2019★ 12 cited

Spica and the annual cycle of PKS B1322-110 scintillations

Hayley Bignall, Cormac Reynolds, Jamie Stevens +9

PKS B1322-110 is a radio quasar that is located only 8.5' in angular separation from the bright B star Spica. It exhibits intra-day variability in its flux density at GHz frequenci…

astro-ph.GA2018★ 2 cited

The MWA GLEAM 4-Jy (G4Jy) Sample

Sarah V. White, Thomas M. O. Franzen, O. Ivy Wong +15

Powerful radio-galaxies feature heavily in our understanding of galaxy evolution. However, when it comes to studying their properties as a function of redshift and/or environment,…