def cosmol_x(row):
     key = {'H0': H0, "Om0": Om, 'Ode0': Ol, 'Ok0': Ok}
     z = row['z']
     err = row['dis_Ftab_averr']
     model = float(l.lum_dis(z, **key) / u.Mpc)
     x = ((row['dis_mpc'] - model)**2) / (err**2)
     return x
def lumdis(z, key):
    return l.lum_dis(z, **cosmology[key])
示例#3
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 def cosmol_x(row, z, err):
     key = {'H0': H0, "Om0": Om, 'Ode0': Ol, 'Ok0': Ok}
     z = row[z]
     model = float(l.lum_dis(z, **key) / u.Mpc)
     x = ((row['dis_mpc'] - model)**2) / (row[err]**2)
     return x