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Table 3.

Best-fit fluxes.

Observation (1) Γ (2) (3) (4) (5)
Chandra 2002 1.9
XMM-Newton 2003
Chandra 2017

Notes. (1) X-ray observation of J1030 + 0524. (2) Photon index found or used in the fit. (3) Flux in the observed-frame 0.5–7 keV band in units of 10−15 erg cm−2 s−1. (4) Flux in the rest-frame 2–8 keV band in units of 10−15 erg cm−2 s−1. (5) Luminosity in the rest-frame 2–8 keV band in units of 1045 erg s−1. Errors are reported at the 1σ level.

For the 2002 Chandra observation we report the values derived from PIMMS, assuming a power-law model of Γ = 1.9.

For the XMM-Newton observation we provide the photon index obtained from the joint fit and the fluxes and luminosity obtained averaging the values from the three detectors (pn, MOS1, MOS2).

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