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19922023
most citedA BLR origin for the iron K line in NGC7213

77 citations · 709 across the 20 of their papers we have counts for

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46 papers · 1 filter

astro-ph2008★ 22 cited

The XMM-Newton survey of the ELAIS-S1 field II: optical identifications and multiwavelength catalogue of X-ray sources

C. Feruglio, F. Fiore, F. La Franca +13

We present optical identifications and a multi-band catalogue of a sample of 478 X-ray sources in the XMM and Chandra surveys of the central 0.6 deg^2 of the ELAIS-S1 field. The op…

astro-ph2008★ 20 cited

The ESO-Spitzer Imaging extragalactic Survey (ESIS) II: VIMOS I,z wide field imaging of ELAIS-S1 and selection of distant massive galaxies

S. Berta, S. Rubele, A. Franceschini +13

(abridged) The ESIS survey is the optical follow up of the SWIRE/Spitzer in the ELAIS-S1 region of the sky. In the era of observational cosmology, the main efforts are focused on t…

astro-ph2008★ 77 cited

A BLR origin for the iron K line in NGC7213

Stefano Bianchi, Fabio La Franca, Giorgio Matt +5

The X-ray spectrum of NGC7213 is known to present no evidence for Compton reflection, a unique result among bright Seyfert 1s. The observed neutral iron K line, therefore, canno…

astro-ph2007★ 21 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-ph2007★ 45 cited

The HELLAS2XMM survey: XI. Unveiling the nature of X-ray Bright Optically Normal Galaxies

F. Civano, M. Mignoli, A. Comastri +8

X-ray Bright Optically Normal Galaxies (XBONGs) constitute a small but not negligible fraction of hard X-ray selected sources in recent Chandra and XMM-Newton surveys. Even though…

astro-ph2007★ 3 cited

AGN counts at 15um. XMM observations of the ELAIS-S1-5 sample

F. La Franca, S. Puccetti, N. Sacchi +7

Context: The counts of galaxies and AGN in the mid infra-red (MIR) bands are important instruments for studying their cosmological evolution. However, the classic spectral line rat…