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Context. Future cosmological surveys will provide 3D large scale structure maps with large sky coverage, for which a 3D spherical Fourier-Bessel (SFB) analysis in spherical coordinates is natural. Wavelets are particularly well-suited to the analysis and denoising of cosmological data, but a spherical 3D isotropic wavelet transform does not currently exist to analyse spherical 3D data.
Frédéric Courbin, Georges Meylan
Frédéric Courbin, Georges Meylan
Frédéric Courbin, Georges Meylan, Austin Chandler Peel