Figure 5 - available via license: Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International
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Mean performance metrics over more than 30 realizations as a function of observation parameters. The default values of the parameters are summarized in Section 2.3.2.
Source publication
Tackling unsupervised source separation jointly with an additional inverse problem such as deconvolution is central for the analysis of multi-wavelength data. This becomes highly challenging when applied to large data sampled on the sphere such as those provided by wide-field observations in astrophysics, whose analysis requires the design of dedic...