All Tables

Table 1: Journal of XMM-Newton observations of NGC 300 X-1 and IC 10 X-1. For each observation, we provide the target, date, revolution number, exposure and good time interval.
Table 2: Fits to the 0.3-10 keV PDS of NGC 300 X-1 from Obs. 1-4. We give the observation number, as well the best fit spectral index with the $\chi ^2$ /d.o.f.. We also give the $\chi ^2$ /d.o.f. for zero power. Finally we give the fractional r.m.s. variability. We note that the PDS for Obs. 3 is more complex than for the other observations, due to an eclipse.
Table 3: Fits to the spectra of NGC 300 X-1 from Obs. 1-4, and of IC 10 X-1. The first model is an absorbed power law plus Gaussian emission line, as favoured by Carpano et al. (2007a). For this model, we give absorption, normalised to 10²² H atom cm^-2, spectral index, line energy and width (in keV), and $\chi ^2$ /d.o.f., with good fit probability in square brackets. We only apply the Gaussian to NGC 300 X-1. We also give the 0.3-10 keV luminosity normalised to 10³⁷ erg s^-1. We next provide the best fits for a disk blackbody + power law model that is often used when describing the high state of disc-accreting BH XBs. We give the absorption, temperature of the disk blackbody, spectral index of the power law component and $\chi ^2$ . We then give 0.3-10 keV luminosity as before, and the fractional contribution of the power law model.