2011
DOI: 10.3726/978-3-0353-0022-2
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Cited by 3 publications
(2 citation statements)
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“…The quoted value of σ 8 = 0.813 ± 0.013 is given at a characteristic mass of 2.5 × 10 14 h −1 M . In addition, we illustrate constraints from galaxy clustering calibrated with weak lensing mass estimates of brightest cluster galaxies (BCG) (Tinker et al 2011), quoted as σ 8 = 0.826 ± 0.02. In this case, we compute the characteristic mass M c (and hence k c ) from the inverse variance weighted average mass of the halos (from Table 2 in Tinker et al (2011)) as M c = 4.7 × 10 13 h −1 M .…”
Section: Reconstructed P (K)mentioning
confidence: 99%
See 1 more Smart Citation
“…The quoted value of σ 8 = 0.813 ± 0.013 is given at a characteristic mass of 2.5 × 10 14 h −1 M . In addition, we illustrate constraints from galaxy clustering calibrated with weak lensing mass estimates of brightest cluster galaxies (BCG) (Tinker et al 2011), quoted as σ 8 = 0.826 ± 0.02. In this case, we compute the characteristic mass M c (and hence k c ) from the inverse variance weighted average mass of the halos (from Table 2 in Tinker et al (2011)) as M c = 4.7 × 10 13 h −1 M .…”
Section: Reconstructed P (K)mentioning
confidence: 99%
“…In addition, we illustrate constraints from galaxy clustering calibrated with weak lensing mass estimates of brightest cluster galaxies (BCG) (Tinker et al 2011), quoted as σ 8 = 0.826 ± 0.02. In this case, we compute the characteristic mass M c (and hence k c ) from the inverse variance weighted average mass of the halos (from Table 2 in Tinker et al (2011)) as M c = 4.7 × 10 13 h −1 M . To remove the dependence on cosmology, the CCCP and BCG mass measurements are multiplied by a factor of h −1 (where h = 0.738 is taken from the recent Riess et al (2011) result).…”
Section: Reconstructed P (K)mentioning
confidence: 99%