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This paper offers a new point of view on component separation, based on amodel of additive components which enjoys a much greater flexibility than moretraditional linear component models. This flexibility is needed to process thecomplex full-sky observations of the CMB expected from the Planck spacemission, for which it was developed, but it may also be useful in any contextwhere accurate component separation is needed.

Component separation with flexible models. Application to the separation of astrophysical emissions