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Fig. 11.

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VLA radio spectral energy distributions of SN 2020qmp at four different epochs. The lines are fitted models as discussed in Sect. 5.1, with shaded confidence regions of 1σ drawn from the posterior distributions. A two-power-law model, as presented in Eq. (4) in Chevalier (1998), was fitted to the spectrum 57 days after the explosion. An optically thin power-law model was fitted to the spectra 51, 104, and 136 days after the explosion.

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