Fiore, F.F.FioreVignali, C.C.VignaliGiommi, PaoloPaoloGiommiTamburelli, F.F.Tamburelli2020-09-172020-09-172002-01-01https://hdl.handle.net/20.500.13025/175VizieR On-line Data Catalog J/MNRAS/327/771. Originally published in 2001MNRAS.327..771FThe BeppoSAX High Energy Large Area Survey (HELLAS) has surveyed about 85deg<SUP>2</SUP> of sky in the 5-10keV band down to a flux of 4-5x10<SUP>-14</SUP>erg/cm<SUP>2</SUP>/s. The source surface density of 16.9+/-6.4deg<SUP>2</SUP> at the survey limit corresponds to a resolved fraction of the 5-10keV X-ray background (XRB) of the order of 20-30 per cent. Hardness ratio analysis indicates that the spectra of a substantial fraction of the HELLAS sources (at least one-third) are harder than a alpha<SUB>E</SUB>=0.6 power law. This hardness may be caused by large absorbing columns. The hardness ratio analysis also indicates that many HELLAS sources may have a spectrum more complex than a single absorbed power law. A soft component, superimposed on a strongly cut-off power law, is likely to be present in several sources. (1 data file).BeppoSAX Comment table2.dat 147x77 HELLAS samplehttp://adsabs.harvard.edu/abs/2002yCat..73270771F2002yCat..73270771F