Table 4.
Open in new tab

De-absorbed power-law parameters describing the differential photon flux obtained with xspec for the available XRT observations, along with the 0.4–4.0 keV de-absorbed integrated energy flux featured in the light curve shown in Fig. 6. See Section 3.3.1 for more details.

Our IDPhoton indexNormalization at 1 keV|$\chi _{\mathrm{ red}}^2$|(d.o.f.)F
(⁠|$\rm keV^{-1} \, s^{-1} \, cm^{-2}$|⁠)(10−12|$\rm erg \, cm^{-2}\, s^{-1}$|⁠)
OBS12.35 |$_{-0.06}^{+0.05}$|(2.32 ± 0.07) × 10−31.08 (52)8.09|$_{-0.46}^{+0.46}$|
OBS22.30 |$_{-0.15}^{+0.15}$|(1.13 ± 0.09) × 10−30.76 (8)3.95|$_{-0.34}^{+0.24}$|
OBS32.42 |$_{-0.07}^{+0.06}$|(1.51 ± 0.06) × 10−30.86 (35)5.26|$_{-0.40}^{+0.40}$|
OBS42.14 |$_{-0.09}^{+0.09}$|(2.59 ± 0.13) × 10−31.10 (21)9.27|$_{-0.31}^{+0.31}$|
OBS62.67 |$_{-0.17}^{+0.17}$|(1.01 ± 0.09) × 10−31.01 (7)3.47|$_{-0.52}^{+0.52}$|
OBS72.36 |$_{-0.07}^{+0.07}$|(1.27 ± 0.05) × 10−31.30 (25)4.57|$_{-0.31}^{+0.33}$|
OBS82.43 |$_{-0.18}^{+0.19}$|(1.17 ± 0.06) × 10−31.10 (15)4.06|$_{-0.80}^{+0.81}$|
Our IDPhoton indexNormalization at 1 keV|$\chi _{\mathrm{ red}}^2$|(d.o.f.)F
(⁠|$\rm keV^{-1} \, s^{-1} \, cm^{-2}$|⁠)(10−12|$\rm erg \, cm^{-2}\, s^{-1}$|⁠)
OBS12.35 |$_{-0.06}^{+0.05}$|(2.32 ± 0.07) × 10−31.08 (52)8.09|$_{-0.46}^{+0.46}$|
OBS22.30 |$_{-0.15}^{+0.15}$|(1.13 ± 0.09) × 10−30.76 (8)3.95|$_{-0.34}^{+0.24}$|
OBS32.42 |$_{-0.07}^{+0.06}$|(1.51 ± 0.06) × 10−30.86 (35)5.26|$_{-0.40}^{+0.40}$|
OBS42.14 |$_{-0.09}^{+0.09}$|(2.59 ± 0.13) × 10−31.10 (21)9.27|$_{-0.31}^{+0.31}$|
OBS62.67 |$_{-0.17}^{+0.17}$|(1.01 ± 0.09) × 10−31.01 (7)3.47|$_{-0.52}^{+0.52}$|
OBS72.36 |$_{-0.07}^{+0.07}$|(1.27 ± 0.05) × 10−31.30 (25)4.57|$_{-0.31}^{+0.33}$|
OBS82.43 |$_{-0.18}^{+0.19}$|(1.17 ± 0.06) × 10−31.10 (15)4.06|$_{-0.80}^{+0.81}$|
Table 4.
Open in new tab

De-absorbed power-law parameters describing the differential photon flux obtained with xspec for the available XRT observations, along with the 0.4–4.0 keV de-absorbed integrated energy flux featured in the light curve shown in Fig. 6. See Section 3.3.1 for more details.

Our IDPhoton indexNormalization at 1 keV|$\chi _{\mathrm{ red}}^2$|(d.o.f.)F
(⁠|$\rm keV^{-1} \, s^{-1} \, cm^{-2}$|⁠)(10−12|$\rm erg \, cm^{-2}\, s^{-1}$|⁠)
OBS12.35 |$_{-0.06}^{+0.05}$|(2.32 ± 0.07) × 10−31.08 (52)8.09|$_{-0.46}^{+0.46}$|
OBS22.30 |$_{-0.15}^{+0.15}$|(1.13 ± 0.09) × 10−30.76 (8)3.95|$_{-0.34}^{+0.24}$|
OBS32.42 |$_{-0.07}^{+0.06}$|(1.51 ± 0.06) × 10−30.86 (35)5.26|$_{-0.40}^{+0.40}$|
OBS42.14 |$_{-0.09}^{+0.09}$|(2.59 ± 0.13) × 10−31.10 (21)9.27|$_{-0.31}^{+0.31}$|
OBS62.67 |$_{-0.17}^{+0.17}$|(1.01 ± 0.09) × 10−31.01 (7)3.47|$_{-0.52}^{+0.52}$|
OBS72.36 |$_{-0.07}^{+0.07}$|(1.27 ± 0.05) × 10−31.30 (25)4.57|$_{-0.31}^{+0.33}$|
OBS82.43 |$_{-0.18}^{+0.19}$|(1.17 ± 0.06) × 10−31.10 (15)4.06|$_{-0.80}^{+0.81}$|
Our IDPhoton indexNormalization at 1 keV|$\chi _{\mathrm{ red}}^2$|(d.o.f.)F
(⁠|$\rm keV^{-1} \, s^{-1} \, cm^{-2}$|⁠)(10−12|$\rm erg \, cm^{-2}\, s^{-1}$|⁠)
OBS12.35 |$_{-0.06}^{+0.05}$|(2.32 ± 0.07) × 10−31.08 (52)8.09|$_{-0.46}^{+0.46}$|
OBS22.30 |$_{-0.15}^{+0.15}$|(1.13 ± 0.09) × 10−30.76 (8)3.95|$_{-0.34}^{+0.24}$|
OBS32.42 |$_{-0.07}^{+0.06}$|(1.51 ± 0.06) × 10−30.86 (35)5.26|$_{-0.40}^{+0.40}$|
OBS42.14 |$_{-0.09}^{+0.09}$|(2.59 ± 0.13) × 10−31.10 (21)9.27|$_{-0.31}^{+0.31}$|
OBS62.67 |$_{-0.17}^{+0.17}$|(1.01 ± 0.09) × 10−31.01 (7)3.47|$_{-0.52}^{+0.52}$|
OBS72.36 |$_{-0.07}^{+0.07}$|(1.27 ± 0.05) × 10−31.30 (25)4.57|$_{-0.31}^{+0.33}$|
OBS82.43 |$_{-0.18}^{+0.19}$|(1.17 ± 0.06) × 10−31.10 (15)4.06|$_{-0.80}^{+0.81}$|
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