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Fig. 1.


Spectral energy distribution of the NGC 3278 (red points). The G RASIL and M AGPHYS models are shown as black solid and blue dotted lines, respectively. For comparison we show the models for the hosts of GRB 980425 (Michałowski et al. 2014b) and 111005A (Michałowski et al. 2018b), scaled to approximately match near-IR fluxes.

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