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Table 2.

Error estimates for the studied SNe.

ξ D1 t0 D2 E(B-V) D3 σtot
(Mpc) (MJD) (Mpc) (mag) (Mpc) (Mpc)
SN2020dpw

Hamuy et al. (2001) 19.74 ± 0.39 58904.0 26.34 ±0.34 0.32 26.66 ±0.52
Eastman et al. (1996) 20.14 ± 0.38 58905.0 25.76 ±0.34 0.38 25.76 ±0.34
Dessart & Hillier (2005) 25.76 ± 0.34 58906.0 25.18 ±0.34 0.44 23.87 ± 0.3

σsys,ξ= 3.5 σsys,t0= 0.58 σsys,ebv= 1.43 5.51

SN2021sjt

Dessart et al. (2015) 24.57 ± 1.27 59400.0 26.47 ± 1.12
1 (Takáts & Vinkó 2012) 21.9 ± 1.15 59401.0 24.57 ±1.30
49402.0 22.67 ±1.41

σsys,ξ= 1.34 σsys,t0= 1.90 σsys,ebv= 1.43 4.67

Notes. Three main factors were taken into account as the sources of systematic error: using different ξ values, the choice of the date of the explosion (t0), and the interstellar reddening (E(B − V)).

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