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Fig. 7.
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Spectral evolution from the UV to the optical and from ∼0.5 until ∼7.2 d for model ms1/ms0p9/vrel10/b0p1 (modelset # 1). Fλ represents the spectral flux density or the flux per unit wavelength interval. Corresponding results for all models from the six sets are shown in Appendix B.
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