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Context. High-precision cosmology requires the analysis of large-scale surveys in 3D spherical coordinates, i.e. spherical Fourier-Bessel decomposition. Current methods are insufficient for future data-sets from wide-field cosmology surveys.
Jean-Paul Richard Kneib, Daniel Felipe Forero Sanchez, Andrei Variu
Frédéric Courbin, Georges Meylan, Austin Chandler Peel
Frédéric Courbin, Georges Meylan