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A multiwavelength study of the Magellanic-type galaxy NGC 4449 โ I. Modelling the spectral energy distribution, the ionization structure and the star formation history
[Abridged] We present an integrated photometric spectral energy distribution (SED) of the Magellanic-type galaxy NGC 4449 from the far-ultraviolet (UV) to the submillimetre, including new observations acquired by the Herschel Space Observatory. We include integrated UV photometry from the Swift Ultraviolet and Optical Telescope using a measurement technique which is โฆ