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ASCA observations of Deep ROSAT fields - II. The 2-10keV AGN luminosity function | B.J.Boyle
; I.Georgantopoulos
; A.J.Blair
; G.C.Stewart
; R.E.Griffiths
; T.Shanks
; K.F.Gunn
; O.Almaini
; | Date: |
1 Oct 1997 | Subject: | astro-ph | Affiliation: | AAO), I.Georgantopoulos (Athens), A.J.Blair (Leicester), G.C.Stewart (Leicester), R.E.Griffiths (Carnegie-Mellon), T.Shanks (Durham), K.F.Gunn (Durham), O.Almaini (IoA | Abstract: | We present additional optical spectroscopic identifications of sources identified in three deep ASCA GIS fields which also form part of a deep ROSAT survey. In total, 26 ASCA sources have been detected down to a 2-10keV flux limit of S = 5e-14 erg/cm/s. LDSS observations have increased the spectroscopic completeness of the survey to between 65 and 85 per cent, with identifications for up to 13 QSOs with broad emission lines and 6 objects with narrow emission lines. Combining these objects with the AGN identified in the LMA/HEAO-1 sample by Grossan, we find evidence for significant cosmological evolution in the 2-10keV band (=0.63+/-0.03), fit by a pure luminosity evolution model; L propto (1+z)^k, k=2.04^{+0.16}_{-0.22}$. The present-epoch 2-10keV AGN X-ray luminosity function, Phi(L_X), is best represented by a two power law function: Phi(L_X) propto L^{-3.0}, L*>10^{44.1}erg/s; $Phi (L_X) propto L^{-1.9}$, L*<10^{44.1}erg/s. Depending on the extent to which we extrapolate the z=0 AGN luminosity function, we predict a total contribution to the 2-10keV X-ray background from QSOs and narrow-emission-line galaxies which ranges from 48 per cent (for AGN with L>10^{42}erg/s) to 80 per cent (L>10^{39}erg/s). | Source: | arXiv, astro-ph/9710002 | Services: | Forum | Review | PDF | Favorites |
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