Table 3
Best-fit spectral parameters and count rates of 2XMM J104608.7-594306 per XMM-Newton observation and EPIC camera.
Ref. | MJD | NH (× 1021 cm-2) | kT (eV) | Net count rate (× 10-2 s-1) | ||||||||
(days) | pn | MOS1 | MOS2 | pn | MOS1 | MOS2 | pn | MOS1 | MOS2 | |||
|
||||||||||||
AO9 | 55 536.531753 |
![]() |
![]() |
![]() |
135(3) | 128(8) | 131(7) | 7.39(12) | 1.54(6) | 1.66(6) | ||
AO11 | 56 282.326597 |
![]() |
![]() |
4.3(5) |
![]() |
131(6) | 125(5) | 7.39(12) | 1.63(5) | 1.73(5) | ||
|
||||||||||||
Simultaneous (per camera) | 2.98(18) |
![]() |
4.1(4) | 134.2(2.4) | 130(5) | 127(4) | 7.39(17) | 1.58(8) | 1.70(8) | |||
Simultaneous (EPIC) | 3.20(15) | 133.1(1.9) | 21.34(20) | |||||||||
Combined | 2.69(13) | 136.7(1.8) | 21.94(19) |
Notes. Errors are 1σ confidence levels. The model fitted to the
data is a simple absorbed blackbody (tbabs∗bbody). Reduced values are within 0.9 and 3.4, for 23
to 30 degrees of freedom (individual fits). Count rates in energy band 0.3−12 keV are subtracted for the
background.
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