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May 11, 2020 18:57
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from astropy.cosmology import FlatLambdaCDM | |
import astropy.units as u | |
planck18_cosmology = {'Oc0': 0.2607, | |
'Ob0': 0.04897, | |
'Om0': 0.3111, | |
'H0': 67.66, | |
'n': 0.9665, | |
'sigma8': 0.8102, | |
'tau': 0.0561, | |
'z_reion': 7.82, | |
't0': 13.787, | |
'Tcmb0': 2.7255, | |
'Neff': 3.046, | |
'm_nu': [0., 0., 0.06], | |
'z_recomb': 1089.80, | |
'reference': "Planck 2018 results. VI. Cosmological Parameters, " | |
"A&A, submitted, Table 2 (TT, TE, EE + lowE + lensing + BAO)" | |
} | |
Planck18 = FlatLambdaCDM(H0=planck18_cosmology['H0'], | |
Om0=planck18_cosmology['Om0'], | |
Tcmb0=planck18_cosmology['Tcmb0'], | |
Neff=planck18_cosmology['Neff'], | |
Ob0=planck18_cosmology['Ob0'], name="Planck18", | |
m_nu=u.Quantity(planck18_cosmology['m_nu'], u.eV)) |
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