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dddddgddZedddddddddd
dddddgddZedddddd d!d"d#d$d%ddd&d'Zed(d)d*d+d,d-d.d/d0d$d%ddd1d'Zed2d3d4d5d6d7d8d9d:d$d%ddd;d'Zd<d=d>d?d@gZdAS )Ba   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).

g6;Nё?g+e?gGz?g(\P@ga4?gQ?gL7A`?g!@g++@g@g|?5^@Tg        gQ?zbPlanck Collaboration 2016, A&A, 594, A13 (Paper XIII), Table 4 (TT, TE, EE + lowP + lensing + ext))Oc0Ob0Om0H0nsigma8tauz_reiont0Tcmb0Neffflatm_nu	referenceg)?g&s|?g+ڧ?gzGP@goT?gݓ?gtF_?g
ףp=
'@g+Η+@zYPlanck 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$@g%C+@g@gRQ@zsHinshaw et al. 2013, ApJS, 208, 19, doi: 10.1088/0067-0049/208/2/19. Table 4 (WMAP9 + eCMB + BAO + H0, last column))r   r   r   r   r   r   r   r   r	   r
   r   r   r   r   g!rh?gK?g rh?gQ@gl?gQ?g(\µ?g$@gQ+@zbKomatsu 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+@zdKomatsu et al. 2009, ApJS, 180, 330, doi: 10.1088/0067-0049/180/2/330. Table 1 (WMAP + BAO + SN ML).Planck15Planck13WMAP9WMAP7WMAP5N)__doc__dictr   r   r   r   r   Z	available r   r   ;lib/python3.7/site-packages/astropy/cosmology/parameters.py<module>*   s   