B d@s<dZeddddddddd d d d d dddgddZeddddddddd d d d d dddgddZeddddddddddd d d dddgddZeddddd d!d"d#d$d%d d d dddgd&dZedd'd(d)d*d+d,d-d.d/d0d1dd d2d3Zedd4d5d6d7d8d9d:d;dd?d@dAdBdCdDdEdFd0d1dd dGd3ZdHdIdJdKdLdMdNgZ dOS)PaThis 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 m_nu Assumed mass of neutrino species, in eV. 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 2018 (Planck18) parameters from Planck Collaboration 2020, A&A, 641, A6 (Paper VI), Table 2 (TT, TE, EE + lowE + lensing + BAO) Planck 2018 (Planck18_arXiv_v2) parameters from Planck Collaboration 2018, arXiv:1807.06209v2 (Paper VI), Table 2 (TT, TE, EE + lowE + lensing + BAO) 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). Z FlatLambdaCDMgM O?ga?goG8-x?g ףp=P@g!rh?g(?gw#?gHzG@gm+@g@g|?5^@TggQ?zfPlanck Collaboration 2018, 2020, A&A, 641, A6 (Paper VI), Table 2 (TT, TE, EE + lowE + lensing + BAO)) cosmologyOc0Ob0Om0H0nsigma8tauz_reiont0Tcmb0Neffflatm_nu referencezrDEPRECATED: Planck Collaboration 2018, arXiv:1807.06209 v2 (Paper VI), Table 2 (TT, TE, EE + lowE + lensing + BAO)g6;Nё?g+e?gGz?g(\P@ga4?gQ?gL7A`?g!@g ++@zbPlanck Collaboration 2016, A&A, 594, A13 (Paper XIII), Table 4 (TT, TE, EE + lowP + lensing + ext)g)?g&s|?g+ڧ?gzGP@goT?gݓ?gtF_?g ףp= '@g+Η+@zYPlanck Collaboration 2014, A&A, 571, A16 (Paper XVI), Table 5 (Planck + WP + highL + BAO)g?߾?gR?gtV?gGzTQ@g?߾?g= ףp=?g#~j?g333333$@g%C+@g@gRQ@zsHinshaw et al. 2013, ApJS, 208, 19, doi: 10.1088/0067-0049/208/2/19. Table 4 (WMAP9 + eCMB + BAO + H0, last column))rrrrrrrrr r r r rr rg!rh?gK?g rh?gQ@gl?gQ?g(\µ?g$@gQ+@zbKomatsu et al. 2011, ApJS, 192, 18, doi: 10.1088/0067-0049/192/2/18. Table 1 (WMAP + BAO + H0 ML).g rh?g9m4?g|?5^?ǧQ@gbX9?g/$?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).Planck18Planck18_arXiv_v2Planck15Planck13WMAP9WMAP7WMAP5N) __doc__dictrrrrrrr availablerri/work/yifan.wang/ringdown/master-ringdown-env/lib/python3.7/site-packages/astropy/cosmology/parameters.py1s