980703 | 990712 | 020405 | 020903 | 030329 | 031203 | 060218 | 060505g | 060505h | |
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- | -2.36 | - | -1.47 | -2.12 | -1.23 | -1.45 | -1.36 | -0.52 |
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AVe |
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Notes. (a) Electronic
density estimated from the
flux ratio:
I(6716)/I(6731).
(b) Temperature
in K estimated from the following flux ratios:
I(4959+5007)/I(4363).
(c) Metallicity,
(O/H),
estimated using the effective temperature method. (d) Metallicity,
(O/H),
estimated following Kobulnicky
et al. (1999). K99
(their Eq. (8)) is valid for the lower branch; K99
(their Eq. (9)) is valid for the upper branch. (e) Extinction
coefficient, AV
(in magnitude) is derived using the standard Balmer ratio of H
and H
.
For GRB 980703 and 020405, AV
from the ratio of H
and H
is adopted. (f) Adopted
metallicity in this work. The R23
degeneracy are broken using the
/H
and
/
ratios. (g) The
GRB
site. (h) The
entire host galaxy.
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