Fig. 1.
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Example of a SNooPy fit of ZTF18aaqfkqh light curves. The three ZTF gri bands do not have observations before peak magnitude, making the determination of the time of maximum very uncertain. Including co ATLAS data allows for a combined fit that adequately constrain the time of maximum and the light-curve width. Note: the ATgr- and ATri-bands correspond to c- and o-ATLAS bands, respectively.
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