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Table 6:

Metallicities of GRB host galaxies.
  980703 990712 020405 020903 030329 031203 060218 060505g 060505h

${N_{\rm e}}[{\rm SII}]$a
- $20\sim200$ - $20\sim200$ $20\sim200$ $52.63\pm43.20$ $120.68\pm32.22$ - -
${T_{\rm e}}[{\rm OIII}]$b - $16434.9\pm425.8$ - $13~517.1\pm335.2$ $17911.7\pm325.0$ $12902.2\pm305.2$ $15113.3\pm335.5 $ - -
$\rm {12 + \log{(O/H)} }(Te)^{c}$ - $7.812\pm0.15$ - $8.014\pm0.15$ $7.653\pm0.14$ $8.142\pm0.07$ $7.883\pm0.09$ - -
$\rm {12+\log{(O/H)}}$d $8.28\pm0.14$ $8.18\pm0.12$f $ 8.10\pm0.12$ $8.11\pm0.12$f $8.06\pm0.10$f $8.11\pm0.11$f $8.16\pm0.14$f $8.06\pm0.14$f $7.99\pm0.09$
$(K99\_l)$                  
$\rm {12+\log{(O/H)}}$d $8.44\pm0.15$ $8.47\pm0.15$ $8.53\pm0.15$ $8.50\pm0.15$ $8.56\pm0.16$ $8.51\pm0.15$ $8.50\pm0.16$ $8.57\pm0.15$ $8.66\pm0.16$f
$(K99\_u)$                  
$\log([{\rm NII}]6583$ - -2.36 - -1.47 -2.12 -1.23 -1.45 -1.36 -0.52
$/{\rm [OII]}3727)$                  
AVe $0.144\pm0.532$ $0.551\pm0.025$ $1.927\pm0.359$ $0.146\pm0.086$ $0.244\pm0.046$ $0.280\pm0.040$ $0.000\pm0.018$ $0.526\pm0.081$ $1.601\pm0.310$

Notes. (a) Electronic density estimated from the $\rm {[S\ II]}$flux ratio: I(6716)/I(6731). (b) Temperature in K estimated from the following flux ratios: $\rm {[O\ III]}$ I(4959+5007)/I(4363). (c) Metallicity, $12+\log$(O/H), estimated using the effective temperature method. (d) Metallicity, $12+\log$(O/H), estimated following Kobulnicky et al. (1999). K99$\_l$ (their Eq. (8)) is valid for the lower branch; K99$\_u$ (their Eq. (9)) is valid for the upper branch. (e) Extinction coefficient, AV (in magnitude) is derived using the standard Balmer ratio of H$\alpha $ and H$\beta $. For GRB 980703 and 020405, AV from the ratio of H$\gamma$ and H$\beta $ is adopted. (f) Adopted metallicity in this work. The R23 degeneracy are broken using the $\rm {[N\ II]}$/H$\alpha $ and $\rm {[N\ II]}$/ $\rm {[O\ II]}$ratios. (g) The GRB site. (h) The entire host galaxy.


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