The BeppoSAX High Energy Large Area Survey (HELLAS) has surveyed several tens of deg(2) of the sky in the 5-10 keV band down to a flux of about 5 x 10(-14) erg cm(-2) s(-1). The source surface density of 16.9 +/- 6.4 deg(-2) at the survey limit corresponds to a resolved fraction of the 5-10 keV X-ray background (XRB) of the order of 20-30 per cent. The extrapolation of the HELLAS log N-log S towards fainter fluxes with a Euclidean slope is consistent with the first XMM-Newton measurements, in the same energy band, which are a factor of 20 times more sensitive. The source counts in the hardest band so far surveyed by X-ray satellites are used to constrain XRB models. It is shown that in order to reproduce the 5-10 keV counts over the range of fluxes covered by BeppoSAX and XMM-Newton a large fraction of highly absorbed (log N-H = 23-24 cm(-2)), luminous (L-x > 10(44) erg s(-1)) active galactic nuclei is needed. A sizeable number of more heavily obscured, Compton-thick, objects cannot be ruled out but they are not required by the present data. The model predicts an absorption distribution consistent with that found from the hardness ratios analysis of the so far identified HELLAS sources. Interestingly enough, there is evidence of a decoupling between X-ray absorption and optical reddening indicators, especially at high redshifts/luminosities where several broad-line quasars show hardness ratios typical of absorbed power-law models with log N-H = 22-24 cm(-2).
Comastri, A., Fiore, F., Vignali, C., Matt, G., Perola, G.c., LA FRANCA, F. (2001). The BeppoSAX High Energy Large Area Survey (HELLAS) - III. Testing synthesis models for the X-ray background. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 327(3), 781-787 [10.1046/j.1365-8711.2001.04737.x].
The BeppoSAX High Energy Large Area Survey (HELLAS) - III. Testing synthesis models for the X-ray background
MATT, Giorgio;LA FRANCA, Fabio
2001-01-01
Abstract
The BeppoSAX High Energy Large Area Survey (HELLAS) has surveyed several tens of deg(2) of the sky in the 5-10 keV band down to a flux of about 5 x 10(-14) erg cm(-2) s(-1). The source surface density of 16.9 +/- 6.4 deg(-2) at the survey limit corresponds to a resolved fraction of the 5-10 keV X-ray background (XRB) of the order of 20-30 per cent. The extrapolation of the HELLAS log N-log S towards fainter fluxes with a Euclidean slope is consistent with the first XMM-Newton measurements, in the same energy band, which are a factor of 20 times more sensitive. The source counts in the hardest band so far surveyed by X-ray satellites are used to constrain XRB models. It is shown that in order to reproduce the 5-10 keV counts over the range of fluxes covered by BeppoSAX and XMM-Newton a large fraction of highly absorbed (log N-H = 23-24 cm(-2)), luminous (L-x > 10(44) erg s(-1)) active galactic nuclei is needed. A sizeable number of more heavily obscured, Compton-thick, objects cannot be ruled out but they are not required by the present data. The model predicts an absorption distribution consistent with that found from the hardness ratios analysis of the so far identified HELLAS sources. Interestingly enough, there is evidence of a decoupling between X-ray absorption and optical reddening indicators, especially at high redshifts/luminosities where several broad-line quasars show hardness ratios typical of absorbed power-law models with log N-H = 22-24 cm(-2).I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
