Searching for Clusters with SUMSS

Simple item page
dc.creatorButtery, H. J.
dc.creatorCotter, G.
dc.creatorHunstead, R. W.
dc.creatorSadler, E. M.
dc.date2003-02-19
dc.date.accessioned2026-07-07T10:26:51Z
dc.date.available2026-07-07T10:26:51Z
dc.descriptionStatistical overdensities of radiosources 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.
dc.descriptionLaTeX, 5 pages, 4 figures Elsevier Science format. To appear in "Radio galaxies: past, present & future". eds. M. Jarvis et al., Leiden, Nov 2002
dc.identifierhttps://arxiv.org/abs/astro-ph/0302390
dc.identifierhttp://arxiv.org/abs/astro-ph/0302390
dc.identifierNewAstron.Rev.47:329-332,2003
dc.identifierdoi:10.1016/S1387-6473(03)00051-4
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/176983
dc.subjectAstrophysics
dc.titleSearching for Clusters with SUMSS
dc.typetext

Files

Collections

arXiv