Table 1.
Open in new tab

Here are the parameter values of Model_ext for fitting the early flux excess of SNe Ia except for SN 2020hvf. The unit of parameters R1, R2, and R3 is 1014 cm, and that of |$\dot{M}_{\text{w}}(0)$| is 10−6 M⊙ yr−1. MCSM is the total mass of CSM integrated to the distance of R3.

SNeR1R2R3|$\dot{M}_{\text{w}}(0)$|MCSM/10−4 M⊙
12cg68203.00.52
14atg710303.01.2
17cbv36163.00.56
18oh510254.01.1
19np510203.50.87
19yvq1.531535.04.3
21aefx38181.50.37
SNeR1R2R3|$\dot{M}_{\text{w}}(0)$|MCSM/10−4 M⊙
12cg68203.00.52
14atg710303.01.2
17cbv36163.00.56
18oh510254.01.1
19np510203.50.87
19yvq1.531535.04.3
21aefx38181.50.37
Table 1.
Open in new tab

Here are the parameter values of Model_ext for fitting the early flux excess of SNe Ia except for SN 2020hvf. The unit of parameters R1, R2, and R3 is 1014 cm, and that of |$\dot{M}_{\text{w}}(0)$| is 10−6 M⊙ yr−1. MCSM is the total mass of CSM integrated to the distance of R3.

SNeR1R2R3|$\dot{M}_{\text{w}}(0)$|MCSM/10−4 M⊙
12cg68203.00.52
14atg710303.01.2
17cbv36163.00.56
18oh510254.01.1
19np510203.50.87
19yvq1.531535.04.3
21aefx38181.50.37
SNeR1R2R3|$\dot{M}_{\text{w}}(0)$|MCSM/10−4 M⊙
12cg68203.00.52
14atg710303.01.2
17cbv36163.00.56
18oh510254.01.1
19np510203.50.87
19yvq1.531535.04.3
21aefx38181.50.37
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