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Table A.1

Time-resolved spectral analysis results of the BEST models.

GRB name spectrum Tstart:Tstop BEST A α β E p E b CSTAT/dof photon flux energy flux
(s) model (ph s-1 cm-2 keV-1) (keV) (keV) (ph s-1 cm-2) (erg s-1 cm-2)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)

080817161 1 –6.144:4.344 COMP 0.0067 ± 0.0010 −0.835 ± 0.060 637.80 ± 96.70 570.4/480 2.1682±0.24 5.7087E-07±5.5E-08
080817161 2 4.344:5.885 COMP 0.0313 ± 0.0034 −0.829 ± 0.047 668.50 ± 79.10 492.51/480 10.172±0.82 2.7450E-06±1.8E-07
080817161 3 5.885:7.150 COMP 0.0444 ± 0.0053 −0.827 ± 0.048 512.90 ± 53.90 529.13/480 13.263±1.1 3.1743E-06±2.2E-07
080817161 4 7.150:8.200 SBPL 0.0439 ± 0.0048 −0.863 ± 0.056 −2.121 ± 0.122 388.69 ± 137.52 191.10 ± 30.90 517.04/479 15.266±1.4 3.3723E-06±2.6E-07
080817161 5 8.200:10.956 COMP 0.0303 ± 0.0049 −0.871 ± 0.057 348.20 ± 36.10 522.13/480 8.1164±0.93 1.5151E-06±1.4E-07
080817161 6 10.956:12.591 COMP 0.0288 ± 0.0041 −0.865 ± 0.052 479.60 ± 56.60 497.74/480 8.5970±0.92 1.9294E-06±1.7E-07

Notes. Column (1) lists the GRB names using the Fermi GBM trigger designation. Column (2) lists the spectrum numbers within individual burst. Column (3) lists the start times Tstart and end times Tstop for the time bins. Column (4) lists the BEST models. Columns (5)(9) list the best-fit parameters of the BEST models, if applicable. Column (10) lists the values of CSTAT per degrees of freedom. Columns (11) and (12) list the 10 keV1 MeV photon and energy fluxes, respectively. The full Table is available at the CDS.

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