Cosmological parameters constraints

дНЙСЛЕМР БГЪР ХГ ЙЩЬЮ ОНХЯЙНБНИ ЛЮЬХМШ. юДПЕЯ НПХЦХМЮКЭМНЦН ДНЙСЛЕМРЮ : http://hea-www.harvard.edu/x-ray-clusters/cosm/combined/en/
дЮРЮ ХГЛЕМЕМХЪ: Unknown
дЮРЮ ХМДЕЙЯХПНБЮМХЪ: Tue Oct 2 10:45:47 2012
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From galaxy clusters mass function measured in Chandra Cluster Cosmology Project (CCCP) (Vikhlinin at al., 2009a, 2009b), in combination with other cosmological data. For details, see also Burenin, Vikhlinin (2012).

Download:

CCCP likelihood grids (108Mb)
CosmoMC module to interpolate on these likelihood grids (readme).

External datasets:

WMAP7 -- 7 year WMAP data (Larson at al., 2011)
SPT -- CMB power spectrum from SPT (Keisler et al., 2011)
H0 -- Determination of Hubble constant (Riess et al., 2011)
BAO -- SDSS and 2dF baryon acoustic oscillations measurements (Percival et al., 2010)
SN -- UNION2 Type I-a supernovae dataset (Amanullah et al., 2010)
SNSYS -- UNION2 Type I-a supernovae data with systematical uncertainties

Cosmological models:

ΛCDM -- flat Universe with cosmological constant
f_ν -- with massive neutrinos (three massive species)
f_ν(1) -- with one massive neutrino
N_eff -- with free effective number of neutrino species, > 3.046
dn/dlnk -- with free running spectral index
r -- with tensor modes
Y_He -- with free primordial helium abundance
OΛCDM -- curved Universe
WCDM -- flat Universe with dark energy
OWCDM -- curved Universe with dark energy
WACDM -- flat Universe with dark energy, time-dependent equation of state

Cosmological parameters constraints

ΛCDM

ΛCDM + ...

OΛCDM

WCDM

OWCDM

WACDM