NumCosmoPlanckFICorTT

Adds all default priors above: - nc_planck_fi_cor_tt_add_default18_gal_priors() - nc_planck_fi_cor_tt_add_default18_calib_priors() - nc_planck_fi_cor_tt_add_default18_sz_prior().

Adds all default priors above: - nc_planck_fi_cor_tt_add_default_gal_priors() - nc_planck_fi_cor_tt_add_default_calib_priors() - nc_planck_fi_cor_tt_add_default_sz_prior().

Add the calibration Gaussian priors using mean and sigma as mean and standard deviation.

Add the calibration priors as described in [Planck 2018 results V (2019)][XPlanckCollaboration2019]. It uses the default values.

Add the galaxy dust priors as described in [Planck 2018 results V (2019)][XPlanckCollaboration2019]. It uses the default values.

Add the SZ prior as described in [Planck 2018 results V (2019)][XPlanckCollaboration2019].

Add the calibration priors as described in [Planck 2015 results XI (2015)][XPlanckCollaboration2015a]. It uses the default values.

Add the galaxy dust priors as described in [Planck 2015 results XI (2015)][XPlanckCollaboration2015a]. It uses the default values.

Add the SZ prior as described in [Planck 2015 results XI (2015)][XPlanckCollaboration2015a]. The prior is given by a $\chi^2$ factor in the form $$\frac{(A^{\mathrm{kSZ}} + f_\mathrm{tSZ} A^{\mathrm{tSZ}} - \mu)^2}{\sigma^2}.$$ It uses the default values.

Add the galaxy dust Gaussian priors using mean and sigma as mean and standard deviation.

Add the SZ prior as described in [Planck 2015 results XI (2015)][XPlanckCollaboration2015a], see also [Planck 2018 results V (2019)][XPlanckCollaboration2019] Eq. (23), The prior is given by a $\chi^2$ factor in the form $$\frac{(A^{\mathrm{kSZ}} + f_\mathrm{tSZ} A^{\mathrm{tSZ}} - \mu)^2}{\sigma^2}.$$.