- Table 1:
44 Bootis observation log during revolution 274.
- 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 (
1 keV) is indicated
- Table 3:
Best fit parameters to EPIC data using a 3 components MEKAL model (Mewe et al. 1985).
The spectral fitting was conducted in the 0.3-5 keV band with the same abundance relative to the Sun for all components.
- Table 4:
Best fit parameters to EPIC data using a plasma emission
model built from the MEKAL code in which the emission measure
distribution follows a power-law in temperature of the forme
- Table 5:
Positions, transition, temperatures of maximum line formation
and fluxes of the strongest lines in RGS spectra.