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Table A.2.

Apparent light curve parameters of SN 2022ngb.

Filter System tpeak trise mpeak γ0 − 15 γ15 − 100
[MJD] [days] [mag] [mag (100 days)−1] [mag (100 days)−1]
B Vega 59772.96 ± 0.07 23.06 ± 0.50 17.66 ± 0.01 10.01 ± 0.40 0.77 ± 0.06
g ab 59773.92 ± 0.04 24.01 ± 0.50 17.22 ± 0.01 8.06 ± 0.08 0.98 ± 0.04
c ab - - - 5.97 ± 0.30 1.43 ± 0.11
V Vega 59774.22 ± 0.06 24.32 ± 0.50 16.74 ± 0.01 6.82 ± 0.24 1.25 ± 0.03
r ab 59778.17 ± 0.02 28.27 ± 0.50 16.53 ± 0.01 4.12 ± 0.18 1.55 ± 0.02
o ab 59778.63 ± 0.05 28.73 ± 0.50 16.44 ± 0.01 3.67 ± 0.14 1.64 ± 0.05
i ab 59779.88 ± 0.03 29.97 ± 0.50 16.35 ± 0.01 3.23 ± 0.16 1.89 ± 0.03
z ab 59780.18 ± 0.05 30.27 ± 0.50 16.33 ± 0.01 - 1.94 ± 0.03
J* Vega - - - - 1.95 ± 0.11
H* Vega - - - - 1.58 ± 0.21
K* Vega - - - - 1.83 ± 0.18

Notes. †: The ATLAS c-band data do not cover the maximum of SN 2022ngb, and therefore the fitting could not be performed. The corresponding decline rate is thus not reliable, as the late-phase data are of limited quality. *: The NIR (JHK) bands lack early phase and pre-maximum coverage, and the post-maximum data are also incomplete. Consequently, the fitting results should be treated with caution and considered less reliable.

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