Table A.2
Best-fit parameters obtained from spectral fitting of HD 93250 as observed from XMM-Newton-EPIC.
Obs. ID | ϕ | norm1 | norm2 | norm3 | ![]() |
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(10−3 cm−5) | (10−4 cm−5) | (1022 cm−2) | (10−12 erg cm−2 s−1) | |||||||||
0112580601 | 0.013 | ![]() |
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1.25 (368) |
0112580701 | 0.022 | ![]() |
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1.24 (156) |
0109530101 | 0.791 | ![]() |
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1.21 ( 76) |
0109530201 | 0.810 | ![]() |
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0.93 ( 71) |
0109530301 | 0.828 | ![]() |
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0.80 ( 67) |
0109530401 | 0.004 | ![]() |
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1.14 (112) |
0112560101 | 0.732 | ![]() |
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1.05 (214) |
0112560201 | 0.748 | ![]() |
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1.00 (196) |
0112560301 | 0.758 | ![]() |
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1.23 (246) |
0145740101 | 0.713 | ![]() |
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0.80 ( 84) |
0145740201 | 0.720 | ![]() |
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0.96 ( 85) |
0145740301 | 0.725 | ![]() |
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1.06 ( 91) |
0145740401 | 0.731 | ![]() |
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1.09 (105) |
0145740501 | 0.736 | ![]() |
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1.33 ( 87) |
0160160101 | 0.403 | ![]() |
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1.04 (175) |
0160160901 | 0.431 | ![]() |
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1.12 (273) |
0145780101 | 0.626 | ![]() |
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1.27 (113) |
0160560101 | 0.687 | ![]() |
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1.19 (181) |
0160560201 | 0.719 | ![]() |
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0.96 ( 79) |
0160560301 | 0.768 | ![]() |
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1.18 (250) |
0311990101 | 0.387 | ![]() |
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1.32 (312) |
0560580101 | 0.890 | ![]() |
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1.01 (187) |
0560580201 | 0.912 | ![]() |
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1.06 (146) |
0560580301 | 0.942 | ![]() |
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1.13 (297) |
0560580401 | 0.034 | ![]() |
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1.04 (282) |
0742850301 | 0.072 | ![]() |
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0.78 ( 95) |
0742850401 | 0.339 | ![]() |
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1.17 (307) |
0762910401 | 0.152 | ![]() |
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0.07† | ![]() |
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1.15 (166) |
0804950201 | 0.703 | ![]() |
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1.19 (311) |
0804950301 | 0.652 | ![]() |
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1.46 (271) |
0830191801 | 0.984 | ![]() |
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0.17† | ![]() |
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1.49 (166) |
0845030201 | 0.472 | ![]() |
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0.12† | ![]() |
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1.44 (309) |
0845030301 | 0.416 | ![]() |
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0.04† | ![]() |
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1.13 (315) |
Notes. Fit parameters are derived from joint spectral fitting of XMM-Newton–MOS1 and MOS2 spectra of HD 93250 using model PHABS(ISM)*PHABS(LOCAL)*(APEC+APEC+APEC) with fixed values of and kT1 = 0.26 keV, kT2 = 1.0 keV, and kT3 =3.3 keV. norm1, norm2, and norm3 are the normalization parameters for three temperature components whereas
is the equivalent local H-column density.
,
, and
are the observed and
,
, and
are the ISM corrected X-ray fluxes of HD 93250 in broad, soft, and hard energy bands, respectively.
is the reduced χ2 and dof is degrees of freedom. Errors quoted on different parameters refer to 90% confidence level. † Mentioned values correspond to the upper limit on the specified parameter.
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