341 citations
- Australia Telescope National FacilityAU11 papers
- Commonwealth Scientific and Industrial Research OrganisationAU11 papers
- Western Sydney UniversityAU10 papers
- International Centre for Radio Astronomy ResearchAU5 papers
- National Astronomical ObservatoriesCN5 papers
- Purple Mountain ObservatoryCN5 papers
- Swinburne University of TechnologyAU5 papers
- ARC Centre of Excellence for Gravitational Wave DiscoveryAU4 papers
- Chinese Academy of SciencesCN4 papers
- National Radio Astronomy ObservatoryUS4 papers
- University of ManchesterGB4 papers
- ASTRO-3DAU3 papers
5 papers · 1 filter
ASKAPEMU Discovery of "Raspberry": a new Galactic SNR Candidate G308.73+1.38
Sanja Lazarević, Miroslav D. Filipović, Bärbel S. Koribalski +8
We report the ASKAP discovery of a new Galactic supernova remnant (SNR) candidate G308.73+1.38, which we name Raspberry. This new SNR candidate has an angular size of 20.7 arcmin $…
Radio detection of an elusive millisecond pulsar in the Globular Cluster NGC 6397
Lei Zhang, Alessandro Ridolfi, Harsha Blumer +32
We report the discovery of a new 5.78 ms-period millisecond pulsar (MSP), PSR J1740-5340B (NGC 6397B), in an eclipsing binary system discovered with the Parkes radio telescope (now…
Systematic upper limits on the size of missing pulsar glitches in the first UTMOST open data release
L. Dunn, A. Melatos, S. Suvorova +7
A systematic, semi-automated search for pulsar glitches in the first UTMOST public data release is presented. The search is carried out using a hidden Markov model which incorporat…
81 New Candidate Fast Radio Bursts in Parkes Archive
X. Yang, S. -B. Zhang, J. -S. Wang +14
We have searched for weak fast radio burst (FRB) events using a database containing 568,736,756 transient events detected using the Parkes radio telescope between 1997 and 2001. In…
On the evidence for a common-spectrum process in the search for the nanohertz gravitational-wave background with the Parkes Pulsar Timing Array
Boris Goncharov, R. M. Shannon, D. J. Reardon +26
A nanohertz-frequency stochastic gravitational-wave background can potentially be detected through the precise timing of an array of millisecond pulsars. This background produces l…