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• Simulation data
  ...ed to first order following the expansion of Nozawa et al. (1998){{BibCite|Nozawa1998}}. To assign an SZ flux to each cluster, we use a mass bias of <math>M_{Xra ...naud2010}}. Relativistic corrections following Itoh et al. (1998){{BibCite|Nozawa1998}} are included to first order. The simulated kinetic SZ effect assumes no b
  114 KB (17,146 words) - 09:49, 21 February 2022
• HFI sims
  ...ed to first order following the expansion of Nozawa et al. (1998){{BibCite|Nozawa1998}}. To assign an SZ flux to each cluster, we use a mass bias of <math>M_{Xra
  29 KB (4,250 words) - 13:56, 2 July 2018
• References
  #Nozawa1998 bibtex=@ARTICLE{1998ApJ...508...17N,
  173 KB (25,381 words) - 15:29, 4 June 2014