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19962007
most citedRadio Observations of the Hubble Deep Field South Region III: The 2.5, 5.2 and 8.7 GHz Catalogues and Radio Source Properties

17 citations · 22 across the 6 of their papers we have counts for

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astro-ph20071 cited

Deep ATLAS Radio Observations of the ELAIS-S1/Spitzer Wide-Area Infrared Extragalctic field

Enno Middelberg, Ray P. Norris, Tim J. Cornwell +12

We have conducted sensitive (1 sigma<30 uJy) 1.4 GHz radio observations with the Australia Telescope Compact Array of a field largely coincident with infrared observations of the S…

astro-ph20072 cited

How to Make the Dream Come True: The Astronomers' Data Manifesto

Ray P Norris

Astronomy is one of the most data-intensive of the sciences. Data technology is accelerating the quality and effectiveness of its research, and the rate of astronomical discovery i…

astro-ph20072 cited

ATLAS: Deep Radio Observations of Six Square Degrees

Ray P. Norris, Enno Middelberg, Brian J. Boyle

We are using the Australia Telescope Compact Array to image about six square degrees surrounding the Chandra Deep Field South and European Large Area ISO Survey - South 1 regions,…

astro-ph200617 cited

Radio Observations of the Hubble Deep Field South Region III: The 2.5, 5.2 and 8.7 GHz Catalogues and Radio Source Properties

Minh T. Huynh, Carole A. Jackson, Ray P. Norris

Deep radio observations of a wide region centred on the Hubble Deep Field South have been performed, providing one of the most sensitive set of radio observations acquired on the A…

astro-ph2005

Can Astronomy Manage Its Data?

Ray P Norris

Astronomy has a distinguished tradition of using technology to accelerate the quality and effectiveness of science, and data-intensive initiatives such as the Virtual Observatory l…

astro-ph2002

A massive star-forming region in a very early stage of evolution

K. J. Brooks, G. Garay, D. Mardones +2

We present results from a study of two luminous IRAS sources thought to be young massive star-forming regions and which have no previously detected radio continuum emission: IRAS 1…