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Table 2.
Comparison between photometry prior to the nova outburst (epoch 2012.838 from PanSTARRS PS1) and during the SPOB phase (2020.194 and 2020.208), used to build the SEDs of Fig. 3.
| B | g | V | r | R | i | I | z | Y | epoch |
|---|---|---|---|---|---|---|---|---|---|
| V392 Per | |||||||||
| 17.49 | 16.37 | 15.74 | 15.38 | 15.09 | 2012.838 | ||||
| 16.13 | 15.53 | 15.10 | 14.76 | 14.46 | 14.28 | 13.73 | 2020.194 | ||
| 14.99 | 14.64 | 14.17 | 13.66 | 13.89 | 13.75 | 2020.208 | |||
| Field star 8″ to the north (FS8) | |||||||||
| 15.43 | 14.79 | 14.50 | 14.35 | 14.24 | 2012.838 | ||||
| 16.06 | 15.46 | 15.08 | 14.82 | 14.57 | 14.53 | 14.03 | 2020.194 | ||
| 15.09 | 14.81 | 14.53 | 14.04 | 14.38 | 14.29 | 2020.208 | |||
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