Table 8
Continuum parameters of the comprehensive EPIC-pn, EPIC-MOS, and RGS best-fit model for ESO 359-G19, HE 1143-1810, CTS A08.12, and Mrk 110.
Hard power law | Black body | Soft power law | ![]() |
||||||
|
|
|
|||||||
Γ | K pwlw | kT | K bb | Γ | K pwlw | ||||
|
|||||||||
ESO 359-G19 |
![]() |
![]() |
![]() |
0.3![]() |
– | – | 0.78/921 | ||
HE 1143-1810 |
![]() |
![]() |
– | – |
![]() |
![]() |
0.92/2097 | ||
CTS A08.12 |
![]() |
![]() |
![]() |
![]() |
– | – | 0.91/1665 | ||
Mrk 110 |
![]() |
![]() |
– | – |
![]() |
![]() |
0.89/2513 |
Notes.
Unconstrained. 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. Normalizations
Kpwlw and Kbb correspond
to the EPIC-pn spectrum. The galactic NH values are
fixed (see Table 1). Errors quoted are at
90% confidence level.
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