Table 3.
X-ray spectral parameters from XMM-Newton, NuSTAR, and AstroSat-SXT observations using a log-parabola model during the deep exposures with MAGIC.
Epoch/date | Instruments | Flux | α | β | χ2/d.o.f. | νsynch, p |
---|---|---|---|---|---|---|
[10−11 erg cm−2 s−1] | [keV] | |||||
Deep exposure 1 | ||||||
July 23, 2020 | XMM-Newton | 1.06 ± 0.01 | 1.94 ± 0.01 | 0.26 ± 0.02 | 476.7/449 | 1.32 ± 0.04 |
XMM-Newton + NuSTAR | 1.05 ± 0.01 | 1.94 ± 0.01 | 0.25 ± 0.02 | 794.6/782 | 1.33 ± 0.04 | |
Deep exposure 2 | ||||||
August 6, 2021 | XMM-Newton | 0.75 ± 0.01 | 2.07 ± 0.01 | 0.41 ± 0.02 | 518.4/429 | 0.82 ± 0.03 |
AstroSat-SXT | 0.93 ± 0.02 | 2.01 ± 0.14 | 0.51 ± 0.27 | 108/113 | 0.97 ± 0.12 |
Notes. In the case of XMM-Newton and XMM-Newton + NuSTAR fits, the fluxes are given in the 2−10 keV band. The AstroSat-SXT flux is computed in the 0.7−7 keV band. The normalisation energy is 1 keV and the Galactic column density of hydrogen is fixed to NH = 1.41 × 1021 cm−2.
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