output
20072026
most citedSearch for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array

1.2k citations

Showing astro-ph.GAShow all

6 papers · 1 filter

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.GA2022★ 1 cited

Absorption spectra of electrified hydrogen molecules

Mark A. Walker

Molecular hydrogen normally has only weak, quadrupole transitions between its rovibrational states, but in a static electric field it acquires a dipole moment and a set of allowed…

astro-ph.GA2021★ 20 cited

ASKAP observations of multiple rapid scintillators reveal a degrees-long plasma filament

Yuanming Wang, Artem Tuntsov, Tara Murphy +5

We present the results from an Australian Square Kilometre Array Pathfinder search for radio variables on timescales of hours. We conducted an untargeted search over a 30 deg f…

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…

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…