Fig. 2 from Deep ATLAS Radio Observations of the Chandra Deep Field–South/Spitzer Wide‐Area Infrared Extragalactic Field

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Deep ATLAS Radio Observations of the Chandra Deep Field–South/Spitzer Wide‐Area Infrared Extragalactic Field

Authors: Ray P. Norris, José Afonso, Phil N. Appleton, Brian J. Boyle, Paolo Ciliegi, Scott M. Croom, Minh T. Huynh, Carole A. Jackson, Anton M. Koekemoer, Carol J. Lonsdale, Enno Middelberg, Bahram Mobasher, Seb J. Oliver, Mari Polletta, Brian D. Siana, Ian Smail, and Maxim A. Voronkov

Norris et al. 2006 The Astronomical Journal 132 2409.

Provider: AAS Journals

Caption: Fig. 2.

Left: Representative sample of the radio image used for component identification in this paper, showing a classical triple radio galaxy (C616, C619, and C622) together with other single‐component galaxies. This image has a beam size of ﹩11^{\prime \prime }\times 5^{\prime \prime }﹩ and a local rms noise of 25 μJy. Right: Same image, but made with natural weighting. It has a higher sensitivity (17 μJy rms) but a larger beam size (﹩28^{\prime \prime }\times 16^{\prime \prime }﹩).

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