Method
NumCosmoXcorSSCSijset_mask_cl
Declaration [src]
void
nc_xcor_ssc_sij_set_mask_cl (
NcXcorSSCSij* ssc_sij,
NcmVector* mask_cl
)
Description [src]
Sets the angular power spectrum of the survey footprint, $C^{\rm
mask}\ell$ for $\ell$ in $[0, \ell{\rm max}]$, so mask_cl has length
$\ell_{\rm max} + 1$ and its truncation sets how many multipoles are summed.
NcmSphereMap computes it from a HEALPix map; it does not depend on
cosmology, so it is set once and reused for every cosmology afterwards.
Passing NULL restores the full-sky spectrum, see nc_xcor_ssc_sij_mask_cl_fullsky().
| Sets property | NumCosmo.XcorSSCSij:mask-cl |
Parameters
mask_cl-
Type:
NcmVectorThe mask angular power spectrum, or
NULLfor the full sky.The argument can be NULL.The data is owned by the caller of the method.