activity
20092023
most citedSearch for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array

1.2k citations · 10.8k across the 126 of their papers we have counts for

collaborators
Showing 2019Show all

11 papers · 1 filter

astro-ph.HE2019

Detection of a Glitch in PSR J09084913 by UTMOST

Marcus E. Lower, Matthew Bailes, Ryan M. Shannon +20

We report the first detection of a glitch in the radio pulsar PSR J09084913 (PSR B090649) during regular timing observations by the Molonglo Observatory Synthesis Telescope (…

astro-ph.HE2019★ 38 cited

Which bright fast radio bursts repeat?

C. W. James, S. Oslowski, C. Flynn +13

A handful of fast radio bursts (FRBs) are now known to repeat. However, the question remains --- do they all? We report on an extensive observational campaign with the Australian S…

astro-ph.HE2019★ 2 cited

Probing the emission states of PSR J1107-5907

Jingbo Wang, George Hobbs, Matthew Kerr +14

The emission from PSR J1107-5907 is erratic. Sometimes the radio pulse is undetectable, at other times the pulsed emission is weak, and for short durations the emission can be very…

astro-ph.IM2019★ 229 cited

An ultra-wide bandwidth (704 to 4032 MHz) receiver for the Parkes radio telescope

G. Hobbs, R. N. Manchester, A. Dunning +69

We describe an ultra-wide-bandwidth, low-frequency receiver ("UWL") recently installed on the Parkes radio telescope. The receiver system provides continuous frequency coverage fro…

astro-ph.HE2019★ 24 cited

A fast radio burst in the direction of the Virgo cluster

Devansh Agarwal, Duncan R. Lorimer, Anastasia Fialkov +19

The rate of fast radio bursts (FRBs) in the direction of nearby galaxy clusters is expected to be higher than the mean cosmological rate if intrinsically faint FRBs are numerous. I…

astro-ph.HE2019★ 19 cited

The emission and scintillation properties of RRAT J2325-0530 at 154 MHz and 1.4 GHz

B. W. Meyers, S. E. Tremblay, N. D. R. Bhat +6

Rotating Radio Transients (RRATs) represent a relatively new class of pulsar, primarily characterised by their sporadic bursting emission of single pulses on time scales of minutes…