The Impact of AXAF & XMM on Measurements of Omega_0 from Cluster Abundances

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dc.creatorRomer, A. Kathy
dc.date1998-09-15
dc.date.accessioned2026-07-07T02:27:57Z
dc.date.available2026-07-07T02:27:57Z
dc.descriptionTwo major X-ray satellites, AXAF & XMM, will be launched in 1998/1999. Both satellites have spectral and imaging capabilities, and are several times more sensitive than either ROSAT or ASCA. AXAF & XMM will yield significant scientific returns in many fields of astrophysics. We concentrate here on how AXAF & XMM will improve constraints on the density parameter, Omega_0, via measurements of the cluster abundance at high redshift.
dc.description4 pages, To appear in the proceedings of the 14th IAP meeting, "Wide Field Surveys in Cosmology", ed. Y. Mellier & S. Colombi
dc.identifierhttps://arxiv.org/abs/astro-ph/9809198
dc.identifierhttp://arxiv.org/abs/astro-ph/9809198
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12913
dc.subjectAstrophysics
dc.titleThe Impact of AXAF & XMM on Measurements of Omega_0 from Cluster Abundances
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