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The HELLAS2XMM survey. IX. Spectroscopic identification of super-EROs hosting AGNs

R. Maiolino·M. Mignoli·L. Pozzetti·P. Severgnini·M. Brusa·C. Vignali·S. Puccetti·P. Ciliegi·F. Cocchia·A. Comastri·F. Fiore·F. La Franca·G. Matt·S. Molendi·G. C. Perola
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Abstract

We present VLT near-IR spectroscopic observations of three X-ray sources characterized by extremely high X-ray-to-optical ratios (X/O>40), extremely red colors (6.3<R-K<7.4, i.e. EROs) and bright infrared magnitudes (17.6<K<18.3). These objects are very faint in the optical, making their spectroscopic identification extremely challenging. Instead, our near-IR spectroscopic observations have been successful in identifying the redshift of two of them (z=2.08 and z=1.35), and tentatively even of the third one (z=2.13). When combined with the X-ray properties, our results clearly indicate that all these objects host obscured QSOs (4e44 < L(2-10keV) < 1.5e45 erg/s, 2e22 < N_H < 4e23 cm-2) at high redshift. The only object with unresolved morphology in the K band shows broad Halpha emission, but not broad Hbeta, implying a type 1.9 AGN classification. The other two objects are resolved and dominated by the host galaxy light in the K band, and appear relatively quiescent: one of them has a LINER-like emission line spectrum and the other presents only a single, weak emission line which we tentatively identify with Halpha. The galaxy luminosities for the latter two objects are an order of magnitude brighter than typical local L* galaxies and the derived stellar masses are well in excess of 10^11 Msun. For these objects we estimate black hole masses higher than 10^9 Msun and we infer that they are radiating at Eddington ratios L/L_Edd < 0.1. We discuss the implications of these findings for the coevolution of galaxies and black hole growth. Our results provide further support that X-ray sources with high X/O ratios and very red colors tend to host obscured QSO in very massive galaxies at high redshift.

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R. Maiolino, M. Mignoli, L. Pozzetti, P. Severgnini, M. Brusa, C. Vignali, S. Puccetti, P. Ciliegi, F. Cocchia, A. Comastri, F. Fiore, F. La Franca, G. Matt, S. Molendi, G. C. Perola. 2005-09-09. The HELLAS2XMM survey. IX. Spectroscopic identification of super-EROs hosting AGNs. https://doi.org/10.1051/0004-6361%3A20053486

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