The Southern SHARC Survey: the z = 0.3 - 0.7 Cluster XLF

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dc.creatorBurke, D. J.
dc.creatorCollins, C. A.
dc.creatorSharples, R. M.
dc.creatorRomer, A. K.
dc.creatorHolden, B. P.
dc.creatorNichol, R. C.
dc.date1997-08-15
dc.date.accessioned2026-07-07T02:24:00Z
dc.date.available2026-07-07T02:24:00Z
dc.descriptionWe present the z = 0.3 - 0.7 cluster X-ray luminosity function (XLF) determined from the Southern SHARC (Serendipitous High-redshift Archival ROSAT Cluster) survey. Over the luminosity range L ~ (0.3 - 3) x 10^44 erg/s (0.5 - 2.0 keV) the XLF is in close agreement with that of the low redshift X-ray cluster population. This result greatly strengthens our previous claim of no evolution of the cluster population, at these luminosities, at a median redshift of z =0.44.
dc.descriptionAccepted for publication in the ApJL, 6 pages, including 4 figures, LaTeX format, requires AASTEX v4.0 macros
dc.identifierhttps://arxiv.org/abs/astro-ph/9708145
dc.identifierhttp://arxiv.org/abs/astro-ph/9708145
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11469
dc.subjectAstrophysics
dc.titleThe Southern SHARC Survey: the z = 0.3 - 0.7 Cluster XLF
dc.typetext

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