Notes. We report the observed luminosities L_X^obs, uncorrected for absorption, and the absorption-corrected values L_X^cor. The 0.5 − 8 keV X-ray luminosities (L_X) were calculated from the best-fit spectral models applied to the data (Table 2). The luminosities in the 0.054 − 12 keV range were derived by extrapolating the absorption-corrected models. The galaxy $L_{0.054-12\mathrm{keV}}^{\mathrm{model}}$ was corrected for the intrinsic absorption for ULX1 and 2, but not for ULX3, 4, and 5, as extending a power law to UV energies would yield unrealistically high luminosities.