Open Access
Table D.2.
Physical properties of the H II region related to each SN.
SN Name | Hα EW | D16 | N2 | O3N2 | ΣSFR | E(B − V) |
---|---|---|---|---|---|---|
(Å) | (12 + log(O/H)) | (12 + log(O/H)) | (12 + log(O/H)) | (log M⊙ yr−1 kpc−2) | (mag) | |
SN2018eog | 3.45 (0.26) | 8.28 (0.12) | 8.45 (0.05) | - | -3.68 (-0.00) | - |
SN2018ant | 8.94 (0.75) | 8.37 (0.11) | 8.49 (0.04) | - | -2.90 (-0.02) | - |
ASASSN-18oa | 27.22 (0.79) | 8.49 (0.03) | 8.51 (0.01) | 8.46 (0.01) | -2.34 (-0.05) | 0.16 (0.07) |
SN2018bl | 171.54 (5.87) | 8.54 (0.02) | 8.47 (0.01) | 8.44 (0.01) | -1.47 (-0.52) | 0.24 (0.05) |
SN2018evy | 108.29 (3.37) | 8.86 (0.01) | 8.56 (0.00) | 8.60 (0.02) | -1.22 (-1.09) | 0.44 (0.04) |
SN2018cho | 17.32 (0.52) | 8.79 (0.02) | 8.58 (0.01) | - | -1.90 (-0.15) | 0.27 (0.13) |
SN2018ie | 342.46 (19.46) | 8.56 (0.01) | 8.47 (0.00) | 8.44 (0.00) | -1.15 (-1.35) | 0.28 (0.03) |
SN2018yo | - | 8.28 (0.03) | 8.36 (0.05) | 8.36 (0.05) | - | - |
... |
Notes. The entire table is available at the CDS. Some CCSNe could not have their oxygen abundance in the O3N2 index and extinction estimated due to the low SNR (< 3) of Hβ or [O III]λ5007 in their spectra.
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