activity
20092013
most citedStudying the relationship between X-ray emission and accretion in AGNs using the XMM-Newton Bright Serendipitous Survey

56 citations · 166 across the 9 of their papers we have counts for

collaborators
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6 papers · 1 filter

astro-ph.CO2012★ 6 cited

Black-hole masses of type 1 AGN in the XMM-Newton bright serendipitous survey

A. Caccianiga, R. Fanali, P. Severgnini +3

We derive masses of the central super-massive black hole (SMBH) and accretion rates for 154 type1 AGN belonging to a well-defined X-ray-selected sample, the XMM-Newton Serendipitou…

astro-ph.CO2012★ 48 cited

NGC454: unveiling a new "changing look" AGN

Elena Marchese, Valentina Braito, Roberto Della Ceca +2

We present a detailed analysis of the X-ray spectrum of the Seyfert 2 galaxy NGC454E, belonging to the interacting system NGC454. Observations performed with Suzaku, XMM-Newton and…

astro-ph.CO2011★ 48 cited

The optical-UV spectral energy distribution of the unabsorbed AGN population in the XMM-Newton Bright Serendipitous Survey

E. Marchese, R. Della Ceca, A. Caccianiga +3

Active galactic nuclei (AGN) emit radiation over a wide range of wavelengths, with a peak of emission in the far-UV region of the electromagnetic spectrum, a spectral region that i…

astro-ph.CO2011

X-ray selected Narrow-Line Seyfert 1 Galaxies

A. Caccianiga, P. Severgnini, R. Della Ceca +3

We present and discuss the properties of a complete and well defined sample of X-ray selected type 1 AGNs including 26 Narrow-Line Seyfert 1 and 129 Broad-Line Seyfert 1 galaxies d…

astro-ph.CO2009

GALEX measurements of the Big Blue Bump as a tool to study bolometric corrections in AGNs

Elena Marchese, R. Della Ceca, A. Caccianiga +2

Active Galactic Nuclei emit over the entire electromagnetic spectrum with the peak of the accretion disk emission in the far-UV, a wavelength range historically difficult to invest…

astro-ph.CO2009★ 1 cited

The XBS sample of type 1 AGNs: Radio loudness vs. physical parameters

A. Caccianiga, P. Severgnini, R. Della Ceca +2

We have studied the relationship between the AGN radio-loudness and the mass of the central black-hole by using the ~190 type 1 AGN selected in the XMM-Newton Bright Survey (XBS).…