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:
External datasets:
Cosmological models:
- ΛCDM -- flat Universe with cosmological constant
- fν -- with massive neutrinos (three massive species)
- fν(1) -- with one massive neutrino
- Neff -- with free effective number of neutrino species, > 3.046
- dn/dlnk -- with free running spectral index
- r -- with tensor modes
- YHe -- 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+fν(1), WMAP7+SPT+BAO+H0+CL
ΛCDM+fν(1)+Neff, WMAP7+SPT+BAO+H0+CL
ΛCDM+fν(1)+Neff, WMAP7+SPT+BAO+H0+SN+CL
ΛCDM+fν+Neff, WMAP7+SPT+BAO+H0+CL
ΛCDM+fν+Neff, WMAP7+SPT+BAO+H0+SN+CL
ΛCDM+fν, WMAP7+H0+CL
ΛCDM+fν, WMAP7+SPT+BAO+H0+CL
ΛCDM+fν, WMAP7+SPT+BAO+H0+SN+CL
ΛCDM+Neff, WMAP7+BAO+H0+CL
ΛCDM+Neff, WMAP7+SPT+BAO+H0+CL
ΛCDM+Neff, 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+YHe, WMAP7+BAO+H0+CL
ΛCDM+YHe, 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