SIMBAD references

We analyze X-ray sources detected over 4.2 pseudo-contiguous sq. deg. in the 0.5-2keV and 2-10keV bands down to fluxes of 2x10^–15 and 8x10^–15erg/s/cm2 respectively, as part of the XMM-Newton Large Scale Structure Survey. The logN-logS in both bands shows a steep slope at bright fluxes, but agrees well with other determinations below ∼2x10^–14erg/s/cm2. The detected sources resolve close to 30 per cent of the X-ray background in the 2-10keV band. We study the two-point angular clustering of point sources using nearest neighbours and correlation function statistics and find a weak, positive signal for ∼1130 sources in the 0.5-2keV band, but no correlation for ∼400 sources in the 2-10 keV band below scales of 100arcsec. A sub-sample of ∼200 faint sources with hard X-ray count ratios, that is likely to be dominated by obscured AGN, does show a positive signal with the data allowing for a large angular correlation length, but only at the ∼2(3)σ level, based on re-sampling (Poisson) statistics. We discuss possible implications and emphasize the importance of wider, complete surveys in order to fully understand the large scale structure of the X-ray sky.