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First scientific VLBI observations using New Zealand 30 meter radio telescope WARK30M

Citation

Petrov, L and Natusch, T and Weston, S and McCallum, J and Ellingsen, S and Gulyaev, S, First scientific VLBI observations using New Zealand 30 meter radio telescope WARK30M, Publications of the Astronomical Society of The Pacific, 127, (952) pp. 516-522. ISSN 0004-6280 (2015) [Refereed Article]

Copyright Statement

Copyright 2015 The Astronomical Society of the Pacific

DOI: doi:10.1086/681965

Abstract

We report the results of a successful 24 hr 6.7 GHz VLBI experiment using the 30-m radio telescope WARK30M near Warkworth, New Zealand, recently converted from a radio telecommunications antenna, and two radio telescopes located in Australia: Hobart 26-m and Ceduna 30-m. The geocentric position of wark30m is determined with a 100 mm uncertainty for the vertical component and 10 mm for the horizontal components. We report correlated flux densities at 6.7 GHz of 175 radio sources associated with Fermi γ-ray sources. A parsec-scale emission from the radio source 1031-837 is detected, and its association with the γ-ray object 2FGL J1032.9-8401 is established with a high likelihood ratio. We conclude that the new Pacific area radio telescope WARK30M is ready to operate for scientific projects.

Item Details

Item Type:Refereed Article
Keywords:astronomy: instrumentation
Research Division:Physical Sciences
Research Group:Astronomical and Space Sciences
Research Field:Astronomical and Space Instrumentation
Objective Division:Expanding Knowledge
Objective Group:Expanding Knowledge
Objective Field:Expanding Knowledge in the Physical Sciences
Author:McCallum, J (Dr Jamie McCallum)
Author:Ellingsen, S (Professor Simon Ellingsen)
ID Code:101356
Year Published:2015
Deposited By:Mathematics and Physics
Deposited On:2015-06-19
Last Modified:2016-06-01
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