Table 2: X-ray luminosities of 44 Boo in the 0.3-2 keV and 2-5 keV energy bands averaged over the different observations periods and corrected for interstellar absorption. The percentage contribution in flux of hot plasmas ( $kT \ge$ 1 keV) is indicated between bracketts.
Obs. $L_{\rm0.3-2 keV}$ $L_{\rm > 2 keV}$ hr

(10²⁸ erg s^-1) (10²⁸ erg s^-1)

Rev. 274 24.3 2.0 -0.85

(flares) (30%) (77%)

Rev. 274 22.4 1.3 -0.89

(steady rate) (36%) (78%)

**Table 2:** X-ray luminosities of 44 Boo in the 0.3-2 keV and 2-5 keV energy bands averaged over the different observations periods and corrected for interstellar absorption. The percentage contribution in flux of hot plasmas ( $kT \ge$ 1 keV) is indicated between bracketts.
Obs.	$L_{\rm0.3-2 keV}$	$L_{\rm > 2 keV}$	hr
	(10²⁸ erg s^-1)	(10²⁸ erg s^-1)
Rev. 274	24.3	2.0	-0.85
(flares)	(30%)	(77%)
Rev. 274	22.4	1.3	-0.89
(steady rate)	(36%)	(78%)

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