Results from the REFLEX Cluster Survey

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dc.creatorBöhringer, H.
dc.creatorGuzzo, L.
dc.creatorCollins, C. A.
dc.creatorNeumann, D. M.
dc.creatorSchindler, S.
dc.creatorSchuecker, P.
dc.creatorCruddace, R.
dc.creatorChincarini, G.
dc.creatorDe Grandi, S.
dc.creatorEdge, A. C.
dc.creatorMacGillivray, H. T.
dc.creatorShaver, P.
dc.creatorVettolani, G.
dc.creatorVoges, W.
dc.date1998-09-29
dc.date.accessioned2026-07-07T02:28:08Z
dc.date.available2026-07-07T02:28:08Z
dc.descriptionBased on the ROSAT All-Sky Survey we have conducted a large redshift survey as an ESO key programme to identify and secure redshifts for the X-ray brightest clusters found in the southern hemisphere. We present first results for a highly controlled sample for a flux limit of 3 10-12 erg/s/cm+2 comprising 475 clusters (87% with redshifts). The logN-logS function of the sample shows an almost perfect Euclidian slope and a preliminary X-ray luminosity function is presented.
dc.description4 pages, 3 figures, To appear in the proceedings of the 14th IAP meeting: "Wide Field Surveys in Cosmology", Y. Mellier & S. Colombi (eds.)
dc.identifierhttps://arxiv.org/abs/astro-ph/9809381
dc.identifierhttp://arxiv.org/abs/astro-ph/9809381
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12987
dc.subjectAstrophysics
dc.titleResults from the REFLEX Cluster Survey
dc.typetext

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