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http://hea-www.harvard.edu/x-ray-clusters/cosm/combined/en/
Дата изменения: Unknown
Дата индексирования: Tue Oct 2 10:45:47 2012
Кодировка:
Поисковые слова:
cygnus
Cosmological parameters constraints
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
ΛCDM
ΛCDM, WMAP7
+CL
ΛCDM, WMAP7+BAO+H0
+CL
ΛCDM, WMAP7+BAO+H0+SPT
+CL
ΛCDM, WMAP7+H0
+CL
ΛCDM + ...
ΛCDM+f
ν
(1), WMAP7+SPT+BAO+H0
+CL
ΛCDM+f
ν
(1)+N
eff
, WMAP7+SPT+BAO+H0
+CL
ΛCDM+f
ν
(1)+N
eff
, WMAP7+SPT+BAO+H0+SN
+CL
ΛCDM+f
ν
+N
eff
, WMAP7+SPT+BAO+H0
+CL
ΛCDM+f
ν
+N
eff
, WMAP7+SPT+BAO+H0+SN
+CL
ΛCDM+f
ν
, WMAP7+H0
+CL
ΛCDM+f
ν
, WMAP7+SPT+BAO+H0
+CL
ΛCDM+f
ν
, WMAP7+SPT+BAO+H0+SN
+CL
ΛCDM+N
eff
, WMAP7+BAO+H0
+CL
ΛCDM+N
eff
, WMAP7+SPT+BAO+H0
+CL
ΛCDM+N
eff
, WMAP7+SPT+BAO+H0+SN
+CL
ΛCDM+dn/dlnk, WMAP7+BAO+H0
+CL
ΛCDM+r, WMAP7+BAO+H0
+CL
ΛCDM+r, WMAP7+SPT+BAO+H0
+CL
ΛCDM+Y
He
, WMAP7+BAO+H0
+CL
ΛCDM+Y
He
, WMAP7+SPT+BAO+H0
+CL
OΛCDM
OΛCDM, WMAP7+BAO+H0
+CL
OΛCDM, WMAP7+SPT+BAO+H0
+CL
WCDM
WCDM, WMAP7+BAO+H0
+CL
WCDM, WMAP7+BAO+H0+SN
+CL
WCDM, WMAP7+BAO+H0+SNSYS
+CL
WCDM, WMAP7+SPT+BAO+H0
+CL
WCDM, WMAP7+SPT+BAO+H0+SN
+CL
WCDM, WMAP7+SPT+BAO+H0+SNSYS
+CL
OWCDM
OWCDM, WMAP7+BAO+H0
+CL
OWCDM, WMAP7+BAO+H0+SN
+CL
WACDM
WACDM, WMAP7+BAO+H0+SN
+CL