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Anastasios Tzioumis

Researcher at Commonwealth Scientific and Industrial Research Organisation

Publications -  121
Citations -  5907

Anastasios Tzioumis is an academic researcher from Commonwealth Scientific and Industrial Research Organisation. The author has contributed to research in topics: Very-long-baseline interferometry & Supernova. The author has an hindex of 39, co-authored 121 publications receiving 5421 citations. Previous affiliations of Anastasios Tzioumis include Australia Telescope National Facility.

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Science with ASKAP: The Australian square-kilometre-array pathfinder

TL;DR: The Australian SKA Pathfinder (ASKAP) as mentioned in this paper is aimed squarely in this frequency range, and achieves instantaneous wide-area imaging through the development and deployment of phase-array feed systems on parabolic reflectors.
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Radio/X-ray correlation in the low/hard state of GX 339-4

TL;DR: In this article, the authors present the results of a long-term study of the black hole candidate GX 339 4 using simultaneous radio and X-ray observations performed between 1997 and 2000.
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A Warped Accretion Disk and Wide-Angle Outflow in the Inner Parsec of the Circinus Galaxy

TL;DR: In this paper, the first VLBI maps of H2O maser emission (λ 1.3 cm) in the nucleus of the Circinus galaxy, constructed from data obtained with the Australia Telescope Long Baseline Array, were presented.
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Science with the Australian Square Kilometre Array Pathfinder

TL;DR: The Australian SKA Pathfinder (ASKAP) is a technology demonstrator aimed in the mid-frequency range, and achieves instantaneous wide-area imaging through the development and deployment of phased-array feed systems on parabolic reflectors as mentioned in this paper.
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Radiatively efficient accreting black holes in the hard state: the case study of H1743-322

TL;DR: In this article, the radio and X-ray emission of H1743−322 were investigated and it was shown that the inner accretion flow is radiatively efficient during the hard state, in contrast to what is usually assumed for black hole Xray binaries in this spectral state.