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  • ...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
  • ...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
  • #Nozawa1998 bibtex=@ARTICLE{1998ApJ...508...17N,
    173 KB (25,381 words) - 15:29, 4 June 2014
  • |Nozawa1998=[http://iopscience.iop.org/0004-637X/508/1/17/pdf/0004-637X_508_1_17.pdf ''
    128 KB (20,140 words) - 08:49, 15 May 2018