Constructing the Universe with Clusters of Galaxies

By Michael Drinkwater, Steve Phillipps, Gregg, J. B. Jones. 2000

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Citations in the corpus

Weak-Lensing Mass Reconstruction of the Interacting Cluster 1E 0657–558: Direct Evidence for the Existence of Dark Matter (2003, unknown): “…lower than those produced by galaxy groups (Hoekstra et al. 2001), which are an order of magnitude lower than those produced by poor clusters (Wittman et al. 2000), which are in turn significantly lower than those produced by rich clusters (Dahle et al. 2002; Clowe et al. 2000; Clowe &…”
The nature and space density of fossil groups of galaxies (2003, methodology): “spectroscopic identification of the full WARPS sample, using methods described in Jones et al. (1998) and Perlman et al. (2002), has since been used to confirm and update the”
Quintessence without scalar fields (2003, result): “1 [38] consistent to the estimates obtained by different approaches.”
Discovery of Ghost Cavities in the X-Ray Atmosphere of Abell 2597 (2001, background): “This implies that feedback between radio heating and radiative cooling may be operating there (Tucker & David 1997; Soker et al. 2001).”
The Cluster-Scale AGN Outburst in Hydra A (2004, background): “The northern part of this edge was noted previously by Forman et al. (2000) and by Markevitch et al. (2002).”
Galaxy Clusters in Hubble Volume Simulations: Cosmological Constraints from Sky Survey Populations (2001, methodology): “We refer the reader to J01, White (2001), and Lacey & Cole (1994) for discussion and intercomparisons of common approaches.”
Determining the Cosmic Distance Scale from Interferometric Measurements of the Sunyaev-Zeldovich Effect (2002, background): “…observations at centimeter wavelengths are now routinely producing high quality images of the SZE (Jones et al. 1993; Grainge et al. 1993; Carlstrom et al. 1996; Carlstrom et al. 1998; Saunders et al. 1999; Grainge et al. 2002b; Reese et al. 2000; Grego et al. 2000; Carlstrom et al.…”
On the efficiency and reliability of cluster mass estimates based on member galaxies (2006, methodology): “A similar conclusion was reached observationally by Biviano et al. (1997), who suggested to exclude emission-line galaxies from the sample of objects to be used in a cluster virial mass determination (see also Sanchis et al.”
Measuring Ωm with the ROSAT Deep Cluster Survey (2001, background): “…for several serendipitous, flux-limited searches for high– redshift clusters (RDCS by Rosati et al. 1995, 1998; 160 deg2 Survey by Vikhlinin et al. 1998; SHARC by Romer et al. 2000; WARPS by Jones et al. 1998; NEP by Gioia et al. 2001; see also Rosati et al. 2000 and Gioia 2000 for recent reviews).”