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Fig. 1.

image

Zwicky Transient Facility (black) and REM (red) g-band photometric points of the 2019 outburst of V1118 Ori. The two dashed lines indicate the linear fits to the points of the rising and declining phases, with indicated the values of their slopes (mag day−1). Both have an uncertainty of 0.002 mag day−1. Two continuous segments indicate the dates of the spectroscopic observations.

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