Table 3.

Upper and lower limits for the free parameters in the IGM models. Continuum parameters were also free parameters. The fixed parameters are Galactic log(⁠|${\it N}\small {\rm HX}$|⁠), the IGM slab at half the GRB redshift, and any known intervening object log(⁠|${\it N}\small {\rm HX}$|⁠).

IGM parameterrange in xspec models
Column density19 ≤ log(⁠|${\it N}\small {\rm HX}$|⁠) ≤23
Temperature4 ≤ log(T/K) ≤8
Metallicity−4 ≤ [X/H] ≤ −0.7
IGM parameterrange in xspec models
Column density19 ≤ log(⁠|${\it N}\small {\rm HX}$|⁠) ≤23
Temperature4 ≤ log(T/K) ≤8
Metallicity−4 ≤ [X/H] ≤ −0.7
Table 3.

Upper and lower limits for the free parameters in the IGM models. Continuum parameters were also free parameters. The fixed parameters are Galactic log(⁠|${\it N}\small {\rm HX}$|⁠), the IGM slab at half the GRB redshift, and any known intervening object log(⁠|${\it N}\small {\rm HX}$|⁠).

IGM parameterrange in xspec models
Column density19 ≤ log(⁠|${\it N}\small {\rm HX}$|⁠) ≤23
Temperature4 ≤ log(T/K) ≤8
Metallicity−4 ≤ [X/H] ≤ −0.7
IGM parameterrange in xspec models
Column density19 ≤ log(⁠|${\it N}\small {\rm HX}$|⁠) ≤23
Temperature4 ≤ log(T/K) ≤8
Metallicity−4 ≤ [X/H] ≤ −0.7
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