All Tables

Table 1: MOS2 count rate to flux conversion factors.
Table 5: The extragalactic Log $(N>S)-{\rm Log}~ S$ maximum likelihood best fit parameters: N(>S) = K $\times$ ( S/10^-13) $^{-\alpha }$ , where N(>S) is the surface densities of sources having a flux greater than S in deg^-2.
Table 6: The current optical breakdown of the BSS and HBSSsamples.
Table 7: HR2 statistic for some relevant BSS and HBSS sub-sample(s).
Table 8: Optically type 2 AGN fraction in few representative X-ray surveys.
Table 2: Basic information on the XMM-Newton MOS2 fields used for the sample selection.
Table 3: Basic information on the XMM-Newton BSS sample.
Table 4: Basic information on the XMM-Newton HBSS sample.
Table B.1: Basic information on the sources excluded from the sample(s) since their "Illumination Factor'' is less than 0.8.