activity
20022008
most citedUnveiling obscured accretion in the Chandra Deep Field South

236 citations · 624 across the 8 of their papers we have counts for

collaborators
Showing astro-phShow all

17 papers · 1 filter

astro-ph2008105 cited

High redshift quasars in the COSMOS survey: the space density of z>3 X-ray selected QSOs

M. Brusa, A. Comastri, R. Gilli +19

We present a new measurement of the space density of high redshift (3.0<z<4.5), X-ray selected QSOs obtained by exploiting the deep and uniform multiwavelength coverage of the COSM…

astro-ph200721 cited

Heavy absorption and soft X-ray emission lines in the XMM-Newton spectrum of the Type 2 radio-loud quasar 3C 234

E. Piconcelli, S. Bianchi, G. Miniutti +4

We report results on a 40 ks XMM-Newton observation of the Type 2 quasar 3C 234. Optical spectropolarimetric data have demonstrated the presence of a hidden broad-line region in th…

astro-ph200721 cited

The contribution of very massive high-redshift SWIRE galaxies to the stellar mass function

S. Berta, C. J. Lonsdale, M. Polletta +18

(Abridged) We selected high-z massive galaxies at 5.8 microns, in the SWIRE ELAIS-S1 field (1 sq. deg.). Galaxies with the 1.6 microns stellar peak redshifted into the IRAC bands (…

astro-ph200732 cited

The XMM-Newton view of IRAS 09104+4109: evidence for a changing-look Type 2 quasar?

E. Piconcelli, F. Fiore, F. Nicastro +4

We analyzed the spectroscopic data from the PN and the MOS cameras in the 0.4-10 keV band. We also used an archival BeppoSAX 1-50 keV observation of IRAS 09104+4109 to investigate…

astro-ph2007236 cited

Unveiling obscured accretion in the Chandra Deep Field South

F. Fiore, A. Grazian, P. Santini +10

A large population of heavily obscured, Compton Thick AGNs is predicted by models of galaxy formation, models of Cosmic X-ray Background and by the ``relic'' super-massive black-ho…

astro-ph200751 cited

The HELLAS2XMM survey. X. The bolometric output of luminous obscured quasars: The Spitzer perspective

F. Pozzi, C. Vignali, A. Comastri +10

Aims: We aim at estimating the spectral energy distributions (SEDs) and the physical parameters related to the black holes harbored in eight high X-ray-to-optical (F_X/F_R>10) obsc…