Simulations Applied to the Bright SHARC XCLF: Results and Implications

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dc.creatorUlmer, M. P.
dc.creatorAdami, C.
dc.creatorPildis, R.
dc.creatorRomer, A. K.
dc.creatorNichol, R. C.
dc.creatorHolden, B. P.
dc.date1999-10-06
dc.date.accessioned2026-07-07T02:33:43Z
dc.date.available2026-07-07T02:33:43Z
dc.descriptionWe have performed simulations of the effectiveness of the Serendipitous High-redshift Archival ROSAT Cluster (SHARC) survey for various model universes. We find, in agreement with work based on a preliminary set of simulations no statistically significant evolution of the luminosity function out to z = 0.8.
dc.description5 pages, 4 Postscript figures, IGRAP-Marseille conf. June 1999
dc.identifierhttps://arxiv.org/abs/astro-ph/9910117
dc.identifierhttp://arxiv.org/abs/astro-ph/9910117
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14959
dc.subjectAstrophysics
dc.titleSimulations Applied to the Bright SHARC XCLF: Results and Implications
dc.typetext

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