A novel optimal transport-based approach for interpolating spectral time series - Paving the way for photometric classification of supernovae

Open Access

Fig. 5

Same as Fig. 3, but in this case Eq. (5) has been used to compute the flux of the spectra. We note that in this figure a given Δ_ph refers to the largest phase interval of the interpolated spectral pairs that enter in the weighted mean.

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