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| NcDataXcor * | nc_data_xcor_new_full () |
| void | nc_data_xcor_set_2 () |
| void | nc_data_xcor_set_AB () |
| void | nc_data_xcor_set_3 () |
| void | nc_data_xcor_set_4 () |
| void | nc_data_xcor_set_5 () |
| void | nc_data_xcor_mean_func_ab () |
| void | nc_data_xcor_get_cl_obs () |
| void | nc_data_xcor_cov_func_abcd () |
This object implements the gaussian likelihood described in \cite{2017arXiv170604583D} for the joint analysis of an abitrary number of cosmic probes with their auto- and cross-angular pseudo power spectra. The covariance of the pseudo spectra implemented here is \begin{align} \mathrm{Cov}\left( \tilde{C}_{\ell}^{AB}, \tilde{C}_{\ell'}^{CD} \right) = & \sqrt{ D_{\ell}^{AD} D_{\ell'}^{AD} D_{\ell}^{BC} D_{\ell'}^{BC}} \mathbfss{X_1}_{\ell \ell'}^{ABCD}\nonumber \ &+ \sqrt{ D_{\ell}^{AC} D_{\ell'}^{AC} D_{\ell}^{BD} D_{\ell'}^{BD}} \mathbfss{X_2}_{\ell \ell'}^{ABCD} \end{align} with \begin{equation} D_{\ell}^{AB} = \left{ \begin{array}{ll} C_{\ell}^{AB} & \text{if } A \neq B \ C_{\ell}^{AA} + N_{\ell}^{A} & \text{if } A=B \ \end{array}\right. . \end{equation}
The matrices $X_{1/2}$ are fixed and describe the mixing between spectra due to the effect of the masks.
NcDataXcor * nc_data_xcor_new_full (const guint nobs,NcXcor *xc,gboolean use_norma);
FIXME
nobs |
a guint, the number of observables |
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xc |
a NcXcor to perform the computation of theoretical power spectra. |
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use_norma |
a gboolean, whether to normalize the likehood. |
void nc_data_xcor_set_2 (NcDataXcor *dxc,guint a,guint b,guint ell_th_cut_off,guint ell_lik_min,guint ell_lik_max,const gchar *clobs_filename,const gchar *mixing_filename,const guint mixing_filelength);
void nc_data_xcor_set_AB (NcDataXcor *dxc,NcXcorAB *xcab);
Links the data object to the object actually containing the data.
void
nc_data_xcor_set_3 (NcDataXcor *dxc);
To be used once all data storage objects have been set.
void nc_data_xcor_set_4 (NcDataXcor *dxc,guint a,guint b,guint c,guint d,const gchar *X1_filename,const gchar *X2_filename,guint X_filelength);
Sets the $X_1$ and $X_2$ matrices used in the covariance matrix for observables $A$, $B$ $C$ and $D$.
dxc |
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a |
a guint, the index of observable $A$ |
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b |
a guint, the index of observable $B$ |
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c |
a guint, the index of observable $C$ |
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d |
a guint, the index of observable $D$ |
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X1_filename |
a gchar, the name of the file where the matrix $X_1^{ABCD}$ is stored |
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X2_filename |
a gchar, the name of the file where the matrix $X_2^{ABCD}$ is stored |
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X_filelength |
a guint, the size of the actual matrices stored in theses files (in case it is larger than the maximum multipole used) |
void
nc_data_xcor_set_5 (NcDataXcor *dxc);
To be used once all $X_{1/2}$ matrices have been set.
void nc_data_xcor_mean_func_ab (NcDataXcor *dxc,NcmVector *vp,guint a,guint b);
FIXME
void nc_data_xcor_get_cl_obs (NcDataXcor *dxc,NcmVector *vp,guint a,guint b);
FIXME
void nc_data_xcor_cov_func_abcd (NcDataXcor *dxc,NcmMatrix *cov,guint a,guint b,guint c,guint d);
FIXME
“nobs” property “nobs” guint
Number of observables.
Owner: NcDataXcor
Flags: Read / Write / Construct
Allowed values: <= 5
Default value: 0
“xc” property“xc” NcXcor *
Xcor object to compute theoretical spectra.
Owner: NcDataXcor
Flags: Read / Write
“xcab-oa” property“xcab-oa” NcmObjArray *
NcXcorAB array.
Owner: NcDataXcor
Flags: Read / Write