Table 7: X-ray fluxes and luminosities of HD 168112. The third column gives the absorbed flux, and the fourth one yields the flux corrected for interstellar absorption. Luminosities corrected for interstellar absorption were determined for the two exposures between 0.4 and 10.0 keV and are given in the fifth column. These luminosities were calculated adopting a 2 kpc distance (see Table 4).
Observation Data set Abs. flux Corr. Flux Corr. luminosity

(erg cm^-2 s^-1) (erg cm^-2 s^-1) (erg s^-1)

April 2002 MOS1 + MOS2 4.77 $\times$ 10^-13 1.93 $\times$ 10^-12 9.15 $\times$ 10³²

MOS1 + MOS2 + pn 4.79 $\times$ 10^-13 1.98 $\times$ 10^-12 9.38 $\times$ 10³²

Sept. 2002 MOS1 + MOS2 3.59 $\times$ 10^-13 1.84 $\times$ 10^-12 8.72 $\times$ 10³²

MOS1 + MOS2 + pn 3.44 $\times$ 10^-13 1.79 $\times$ 10^-12 8.48 $\times$ 10³²

**Table 7:** X-ray fluxes and luminosities of HD 168112. The third column gives the absorbed flux, and the fourth one yields the flux corrected for interstellar absorption. Luminosities corrected for interstellar absorption were determined for the two exposures between 0.4 and 10.0 keV and are given in the fifth column. These luminosities were calculated adopting a 2 kpc distance (see Table 4).
Observation	Data set	Abs. flux	Corr. Flux	Corr. luminosity
		(erg cm^-2 s^-1)	(erg cm^-2 s^-1)	(erg s^-1)
April 2002	MOS1 + MOS2	4.77 $\times$ 10^-13	1.93 $\times$ 10^-12	9.15 $\times$ 10³²
	MOS1 + MOS2 + pn	4.79 $\times$ 10^-13	1.98 $\times$ 10^-12	9.38 $\times$ 10³²
Sept. 2002	MOS1 + MOS2	3.59 $\times$ 10^-13	1.84 $\times$ 10^-12	8.72 $\times$ 10³²
	MOS1 + MOS2 + pn	3.44 $\times$ 10^-13	1.79 $\times$ 10^-12	8.48 $\times$ 10³²

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