Table 6
Best-fit model to the continuum of the EPIC spectra in the 0.35–10 keV range.
| Hard power law | Black body | Soft power law |  /d.o.f. |
||||||
| Γ | K pwlw | kT | K bb | Γ | K pwlw | ||||
|
|
|||||||||
| ESO 359-G19 |
|
|
|
|
— | — | 0.76/716 | ||
| HE 1143-1810 |
|
|
— | — |
|
|
0.90/1914 | ||
| CTS A08.12 |
|
|
|
|
— | — | 0.88/1486 | ||
| Mrk 110 |
|
|
— | — |
|
|
0.90/2187 | ||
Notes. Power-law normalizations (Kpwlw) in
units of 10-4 ph keV-1 cm-2 s-1 at 1 keV;
kT in keV; Kbb in
10-5 
where L39
is the source luminosity in units of 1039 erg s-1 and
D10 is the distance to the source in units of 10 kpc.
The Galactic NH values are fixed (see Table 1). Errors quoted are at 90% confidence level.
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