Common tools used by the component sepration pipeline.
Compute covariance from alm.
A correction for beam and mask effect is performed is options are given.
Compute noise power spectra from alm.
A correction for beam and mask effect is performed is options are given.
Provide standard bins used for plots.
This is an arbitrary choice of bin size, only used for plots.
Return Planck 2015 empirical cmb power spectra.
Return Planck 2013 best fit cmb power spectra.
Make a common binary point source mask
Make a plot of the auto spectra of the covariance matrice. Noise is superimposed if provided.
Plot eigen value decomposition
Make a plot of detector weight as a function of the multipole.
Make a plot of the detector noise contribution as a function of the multipole.
Return smoothed power spectrum.
Power spectrum is averaged over window of size dloverl (in %)
Provide a set of covariance matrices which are smoothed over multipole range.
High ell regime is read from Rl_high starting from lilc multipole. Low ell regime can be forced to be constant from 0 to lcst. Matrices are supposed to be symmetric.