A Systematic X-Ray Search for Clusters of Galaxies behind the Milky Way
By H. Ebeling, C. Mullis, R. B. Tully. 2002
145 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/e57bec27f80951b665477a37964259c7b3b07958
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Citations in the corpus
- Streaming motions of galaxy clusters within 12 000 km s−1– V. The peculiar velocity field (2004, background): “The “Clusters Behind the Zone of Avoidance” (CIZA), an X-ray selected survey galaxy clusters, Ebeling et al. (2002) alsoindicates several massive clusters at low galactic latitudes.”
- RELICS: Reionization Lensing Cluster Survey (2019, background): “Alternate cluster names include one also identified in the Rosat Bright Survey (RBS; Kausch et al. 2010) and another in Clusters in the Zone of Avoidance (CIZA; Kocevski et al. 2007).”
- A Measurement of Large-Scale Peculiar Velocities of Clusters of Galaxies: Results and Cosmological Implications (2008, background): “…Limited X-ray catalog (REFLEX) (Böhringer et al. 2004) in the southern hemisphere, the extended Brightest Cluster Sample (eBCS) (Ebeling et al. 1998, 2000) in the north, and the Clusters in the Zone of Avoidance (CIZA) (Ebeling et al. 2002; Kocevski et al. 2007) sample along the Galactic plane.”
- The ROSAT-ESO Flux Limited X-ray (REFLEX) Galaxy cluster survey. V. The cluster catalogue (2004, unknown): “…statistical galaxy cluster samples (Pierre et al. 1994; Romer et al. 1994; Ebeling et al. 1996, 1998, 2000; Burns et al. 1996; De Grandi et al. 1999; Ledlow et al. 1999; Böhringer et al. 2000, 2001c; Henry et al. 2001; Cruddace et al. 2002, 2003; Ebeling et al. 2001, 2002; Gioia et al. 2003).”
- The MCXC: a meta-catalogue of x-ray detected clusters of galaxies (2010, methodology): “The CIZA (Clusters in the Zone of Avoidance, Ebeling et al. 2002 and Kocevski et al. 2007, respectivelyCIZAI and CIZAII ) catalogues are based on the ROSAT Bright Source 3 MACSJ0358.”
- The X-ray brightest clusters of galaxies from the Massive Cluster Survey (2010, background): “…Trümper 1983) data (Ebeling et al. 1996, 1998, 2000; De Grandi et al. 1999; Ebeling, Mullis & Tully 2002; Cruddace et al. 2002; Böhringer et al. 2004; Kocevski et al. 2007) has allowed greatly improved, unbiased measurements of the properties of clusters as an astronomical class of objects.”
- The UKIDSS galactic plane survey (2007, background): “Dressler et al.(1987); Kolatt et al.(1995); Kraan-Korteweg & Lahav 2000, Schröder et al.(2007); Kocevski et al.(2007), and the origin of the dipole in the Cosmic Microwave Background.”