Searching for Clusters with SUMSS
(2003)
Follow-up of the 9C survey: Initial results
(2003)
Searching for Clusters with SUMSS
New Astronomy Reviews 47:4-5 (2003) 329-332
Abstract:
Statistical overdensities of radio sources in the Sydney University Molonglo Sky Survey (SUMSS) are used as signposts to identify high-redshift clusters of galaxies. These potential clusters have been observed at 20 and 13 cm at the Australia Telescope Compact Array (ATCA) to obtain better positional accuracy for the sources. A subsample have been imaged in V, R and I at the 2.3-m telescope at Siding Spring and in J and K at the Anglo Australian Telescope (AAT) and the New Technology Telescope (NTT) at La Silla, Chile. The colours obtained from these observations will be used to estimate redshifts for the potential cluster members. 漏 2003 Elsevier B.V. All rights reserved.Follow-up of the 9C survey: initial results
NEW ASTRONOMY REVIEWS 47:4-5 (2003) 367-371
Ground-Based Mid Infra-Red Observations of Nearby Starburst and AGN Galaxies
Chapter in The Evolution of Galaxies, Springer Nature (2003) 279-282