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Accurate radio positions with the Tidbinbilla interferometerThe Tidbinbilla interferometer (Batty et al., 1977) is designed specifically to provide accurate radio position measurements of compact radio sources in the Southern Hemisphere with high sensitivity. The interferometer uses the 26-m and 64-m antennas of the Deep Space Network at Tidbinbilla, near Canberra. The two antennas are separated by 200 m on a north-south baseline. By utilizing the existing antennas and the low-noise traveling-wave masers at 2.29 GHz, it has been possible to produce a high-sensitivity instrument with a minimum of capital expenditure. The north-south baseline ensures that a good range of UV coverage is obtained, so that sources lying in the declination range between about -80 and +30 deg may be observed with nearly orthogonal projected baselines of no less than about 1000 lambda. The instrument also provides high-accuracy flux density measurements for compact radio sources.
Document ID
19800051366
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Batty, M. J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Gulkis, S.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Jauncey, D. L.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Rayner, P. T.
(Commonwealth Scientific and Industrial Research Organization Div. of Radiophysics, Sydney, Australia)
Date Acquired
August 10, 2013
Publication Date
January 1, 1979
Publication Information
Publication: Astronomical Society of Australia
Subject Category
Astronomy
Accession Number
80A35536
Funding Number(s)
CONTRACT_GRANT: NAS7-100
Distribution Limits
Public
Copyright
Other

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