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Table 2

Best-fit parameters and observed fluxes for the continuum derived with the joint fit of the Suzaku and Chandra data.

Parameter Units
Γ
N H 1022 cm-2
A Scatt a 10-5 ph cm-2 s-1
A PL b 10-3 ph cm-2 s-1
A PEX c 10-3 ph cm-2 s-1
kT keV
A ThSuzaku d 10-4 cm-5
A ThChandra e 10-4 cm-5
F (0.5–2) keVChandra 10-13 erg cm-2 s-1 1.9 ± 0.1
F (0.5–2) keVSuzaku 10-13 erg cm-2 s-1 4.3 ± 0.2
F (2–10) keVChandra 10-12 erg cm-2 s-1
F (2–10) keVSuzaku 10-12 erg cm-2 s-1

Notes.

(a)

Normalization of the scattered power-law component.

(b)

Primary power-law component normalization.

(c)

Compton reflection component normalization.

(d)

Normalization of the thermal component is defined as , where DA is the angular size distance to the source (cm), ne is the electron density (cm-3), and nH is the hydrogen density (cm-3) as defined in the mekal model.

(e)

Normalization of the thermal component for the Chandra spectra obtained after fixing the photon index of the scattered component.

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