Characterization of gamma-ray burst prompt emission spectra down to soft X-rays

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Table B.1.

List of the 34 GRBs analyzed in this work.

GRB	Redshift	N_H 10²² cm⁻²	LTI 10⁴ s
060510B	4.940	0.00	0.05–62.41
060814	1.92	1.93	16.83–137.78
061121	1.314	0.82	3.46–9.25
070616	...	0.49	0.46–37.11
070721B	3.626	0.00	0.02–13.95
080906	...	0.34	0.54–73.69
080928	1.69	0.62	0.42–3.34
081008	1.969	0.69	0.06–1.77
090709A	...	0.27	0.41–6.27
090715B	3.000	2.02	0.02–164.88
100413A	...	0.25	0.63–17.46
100619A	...	0.45	5.34–100.59
100704A	...	0.37	1.26–131.81
100725B	...	0.59	2.18–80.35
100728A	1.567	3.43	0.50–68.29
100814A	1.440	0.25	21.20–671.30
100906A	1.727	0.94	1.06–46.86
110102A	...	0.19	1.04–24.32
110119A	...	0.16	0.49–26.09
110205A	2.22	0.70	0.14–38.29
111103B	...	0.35	4.55–30.06
111123A	3.152	4.81	0.42–4.06
121123A	...	0.05	1.66–13.91
121217A	...	0.63	2.87–547.65
130514A	...	0.36	1.15–38.81
130606A	5.913	9.12	0.53–1.26
130907A	1.238	1.05	0.76–238.41
140108A	...	1.70	1.05–43.16
140206A	2.73	2.03	2.12–8.71
140323A	...	0.39	2.82–9.84
140512A	0.725	0.44	2.79–32.94
141031A	...	0.30	4.57–84.70
150724A	...	0.55	0.13–13.26
151021A	2.330	2.40	0.49–67.93

Notes. The GRB’s name and redshift are reported in the first and second columns. The third column lists the values of the intrinsic N_H, derived from spectral analysis of late time XRT observations (see Sect. 4 for the method used to estimate N_H for GRBs with and without measured redshift). The late time interval (LTI, from the BAT trigger time) chosen for the estimate of N_H can be found in the last column.

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