Fig. 5.

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Peak magnitudes of SLSN template. The limiting magnitudes of each visit by the EDS observations (25.5 mag for the IE band and 24.0 mag for the YE, JE, and HE bands in AB magnitudes) are shown with the dashed lines. The template magnitudes are randomly scattered by the standard deviation of 0.7 mag (both to brighter and fainter magnitudes) assuming the Gaussian probability distribution in the survey simulations to match the observed luminosity function as discussed in Sect. 3.
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