3.5k citations
- R. Manchester219 · h 92
- B. Koribalski2 profiles180 · h 34
- S. Johnston2 profiles175 · h 62
- M. Bailes153 · h 86
- F. Camilo146 · h 82
- L. Staveley-Smith140 · h 73
- G. Hobbs2 profiles130 · h 65
- R. Shannon3 profiles124 · h 53
- A. Possenti120 · h 81
- A. Lyne2 profiles119 · h 90
- M. Kerr3 profiles101 · h 86
- B. Stappers93 · h 88
- Commonwealth Scientific and Industrial Research OrganisationAU1.7k papers
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- Australian National UniversityAU219 papers
89 papers · 1 filter
The Australian experience with the PC-EVN recorder
R. Dodson, S. Tingay, C. West +4
We report on our experiences using the Metsahovi Radio Observatory's (MRO) VLBI Standard Interface (VSI, Whitney 2002) recorder in a number of astronomical applications. The PC-EVN…
The ATNF Pulsar Catalogue
R N Manchester, G B Hobbs, A Teoh +1
We have compiled a new and complete catalog of the main properties of the 1509 pulsars for which published information currently exists. The catalog includes all spin-powered pulsa…
COSMIC : Microarcsecond resolution with a 30 metre radio telescope
P. M. McCulloch, S. P. Ellingsen, D. L. Jauncey +4
Interstellar scintillation has been conclusively demonstrated to be the principal cause of the intraday variability (IDV) observed in the centimetre-wavelength emission of many AGN…
What do loose groups tell us about galaxy formation?
D. J. Pisano, David Barnes, Brad Gibson +3
We present the results of a Parkes Multibeam HI survey of six loose groups of galaxies analogous to the Local Group. This survey was sensitive to HI-rich objects in these groups to…
Pulsars and Gravitational Wave Detection
George Hobbs
The number of known millisecond pulsars has dramatically increased in the last few years. Regular observations of these pulsars may allow gravitational waves with frequencies ~10^-…
PSR J1022+1001: Profile Stability & Precision Timing
A. W. Hotan, M. Bailes, S. M. Ord
We present an investigation of the morphology and arrival times of integrated radio pulses from the binary millisecond pulsar PSR J1022+1001. This pulsar is renowned for its poor t…