Table A.1.
List of the observations used in this work and fits results.
| ObsID | Date | Γ index | NH | Fbol (0.1–300 keV) |  |
|
|---|---|---|---|---|---|---|
| (mm-dd-yyyy) | (×1022 cm−2) | (×10−10 erg × cm−2 × s−1 ) | (d.o.f.) | |||
| 1 | 80145-02-01-01 | 06-07-2003 | 1.600 ± 0.020 | < 0.48 | 6.80 ± 0.68 | 1.45(47) |
| 2 | 80418-01-02-06 | 06-15-2003 | 1.706 ± 0.012 | 0.89 ± 0.16 | 8.69 ± 0.87 | 0.99(46) |
| 3* | ||||||
| 4 | 80418-01-03-12 | 06-20-2003 | 1.659 ± 0.015 | 0.40 ± 0.20 | 8.27 ± 0.83 | 0.90(46) |
| 5 | 80418-01-03-08 | 06-24-2003 | 1.670 ± 0.020 | 0.45 ± 0.30 | 8.78 ± 0.88 | 0.86(46) |
| 6 | 80418-01-05-00 | 07-04-2003 | 1.700 ± 0.030 | 0.50 ± 0.40 | 6.85 ± 0.69 | 0.71(46) |
| 7 | 80418-01-05-09 | 07-09-2003 | 1.760 ± 0.013 | 0.300† | 6.96 ± 0.70 | 0.93(48) |
| 8 | 80418-01-06-02 | 07-13-2003 | 1.840 ± 0.020 | 0.300† | 2.16 ± 0.22 | 0.97(47) |
| 9* |
Notes. The data have been all analysed using a simple TBABS × POWERLAW model. The quoted errors for Γ and NH were calculated with the ERROR command for the resulting simulated posterior distribution and reflect 90% confidence intervals, while a standard uncertainty of 10% has been attributed to each of the bolometric flux values. (*) Under the assumption that the flux was almost the same between the previous data point and this one, an assumption based on the light curve shape over these time intervals, the bolometric flux at this time was considered equal to the flux reported in the preceding row; (†) the parameter was kept frozen to the reported value for the stability of the fit.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.