Graph 4: Expected logN - logS curve of stars(green), CVs(red) and AGNs(black, continous line is for NHI = 1021 cm-2, dotted line is for NHI = 1020 cm-2) in the galactic plane, at soft X-rays (0.1-2 keV). At hard X-ray energies the AGN populations become more dominant.

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