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 d d d d d d d d d d d d d d d e d d d d g d d  Z e d d d d  d d! d	 d" d d# d d$ d d% d d& d d' d d d d d e d d d d g d d(  Z	 e d d) d d* d d+ d	 d, d d- d d. d d/ d d0 d d1 d d2 d d3 d d d e d d4  Z
 e d d5 d d6 d d7 d	 d8 d d9 d d: d d; d d< d d= d d2 d d3 d d d e d d>  Z e d d? d d@ d dA d	 dB d dC d dD d dE d dF d dG d d2 d d3 d d d e d dH  Z dI dJ dK dL dM g Z dN S(O   u   This module contains dictionaries with sets of parameters for a
given cosmology.

Each cosmology has the following parameters defined:

    ==========  =====================================
    Oc0         Omega cold dark matter at z=0
    Ob0         Omega baryon at z=0
    Om0         Omega matter at z=0
    flat        Is this assumed flat?  If not, Ode0 must be specified
    Ode0        Omega dark energy at z=0 if flat is False
    H0          Hubble parameter at z=0 in km/s/Mpc
    n           Density perturbation spectral index
    Tcmb0       Current temperature of the CMB
    Neff        Effective number of neutrino species
    sigma8      Density perturbation amplitude
    tau         Ionisation optical depth
    z_reion     Redshift of hydrogen reionisation
    t0          Age of the universe in Gyr
    reference   Reference for the parameters
    ==========  =====================================

The list of cosmologies available are given by the tuple
`available`. Current cosmologies available:

Planck 2015 (Planck15) parameters from Planck Collaboration 2016, A&A, 594, A13
 (Paper XIII), Table 4 (TT, TE, EE + lowP + lensing + ext)

Planck 2013 (Planck13) parameters from Planck Collaboration 2014, A&A, 571, A16
 (Paper XVI), Table 5 (Planck + WP + highL + BAO)

WMAP 9 year (WMAP9) parameters from Hinshaw et al. 2013, ApJS, 208, 19,
doi: 10.1088/0067-0049/208/2/19. Table 4 (WMAP9 + eCMB + BAO + H0)

WMAP 7 year (WMAP7) parameters from Komatsu et al. 2011, ApJS, 192, 18,
doi: 10.1088/0067-0049/192/2/18. Table 1 (WMAP + BAO + H0 ML).

WMAP 5 year (WMAP5) parameters from Komatsu et al. 2009, ApJS, 180, 330,
doi: 10.1088/0067-0049/180/2/330. Table 1 (WMAP + BAO + SN ML).

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'@g+Η+@uY   Planck Collaboration 2014, A&A, 571, A16 (Paper XVI), Table 5 (Planck + WP + highL + BAO)g?߾?gR?gtV?gGzTQ@g?߾?g=
ףp=?g#~j?g333333$@g%C+@g@gRQ@us   Hinshaw et al. 2013, ApJS, 208, 19, doi: 10.1088/0067-0049/208/2/19. Table 4 (WMAP9 + eCMB + BAO + H0, last column)g!rh?gK?g rh?gQ@gl?gQ?g(\µ?g$@gQ+@ub   Komatsu et al. 2011, ApJS, 192, 18, doi: 10.1088/0067-0049/192/2/18. Table 1 (WMAP + BAO + H0 ML).g rh?g9m4?g|?5^?ǧQ@gbX9?g/$?gI+?g&@gq=
ףp+@ud   Komatsu et al. 2009, ApJS, 180, 330, doi: 10.1088/0067-0049/180/2/330. Table 1 (WMAP + BAO + SN ML).u   Planck15u   Planck13u   WMAP9u   WMAP7u   WMAP5N(   t   __doc__t
   __future__R    R   R   R   t   dictt   Truet   Planck15t   Planck13t   WMAP9t   WMAP7t   WMAP5t	   available(    (    (    s;   lib/python2.7/site-packages/astropy/cosmology/parameters.pyt   <module>*   s   "						