Table 3: X-ray luminosities (corrected for interstellar absorption) of HD 223460 in the 0.3-2 keV and 2-10 keV measured with the combined EPIC MOS and pn cameras. The percentage contribution in luminosity of hot plasmas (kT> 1 keV) is indicated between bracketts. The hardness ratio (hr) is defined as $hr = (L_{\rm >2~ ~keV}-L_{\rm 0.3-2~~keV})/(L_{\rm >2 ~keV}+L_{\rm 0.3- 2~keV})$ .
Obs. $L_{\rm0.3-2 ~keV}$ $L_{\rm >2~~keV}$ hr

(10³⁰ erg s^-1) (10³⁰ erg s^-1)

Rev. 107 27.0 10.7 -0.43

(78%) (98%)

Rev. 200 22.7 7.3 -0.51

(78%) (98%)

**Table 3:** X-ray luminosities (corrected for interstellar absorption) of HD 223460 in the 0.3-2 keV and 2-10 keV measured with the combined EPIC MOS and pn cameras. The percentage contribution in luminosity of hot plasmas (kT> 1 keV) is indicated between bracketts. The hardness ratio (hr) is defined as $hr = (L_{\rm >2~ ~keV}-L_{\rm 0.3-2~~keV})/(L_{\rm >2 ~keV}+L_{\rm 0.3- 2~keV})$ .
Obs.	$L_{\rm0.3-2 ~keV}$	$L_{\rm >2~~keV}$	hr
	(10³⁰ erg s^-1)	(10³⁰ erg s^-1)
Rev. 107	27.0	10.7	-0.43
	(78%)	(98%)
Rev. 200	22.7	7.3	-0.51
	(78%)	(98%)

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