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Fig. 5.

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Optical luminosity light curve of WD–NS mSNe. The left panel shows our fiducial model, assuming an ejecta mass of Mej = 0.3 M and a 56Ni mass of MNi = 0.01 M. The right panel presents the WD–NS mSNe model in which both the ejecta and 56Ni masses are reduced by an order of magnitude, adopting Mej = 0.03 M and MNi = 0.001 M. Different colors indicate different viewing angles at θview = 0°, 15°, 30°, 45°, 60°, and 90°. Solid and dashed lines correspond to the g- and r-band luminosities, respectively.

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