activity
19942022
most citedA 3 dimensional diagnostic diagram for Seyfert 2s: probing X-ray absorption and Compton thickness

453 citations · 3.3k across the 50 of their papers we have counts for

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Showing astro-ph.GAShow all

9 papers · 1 filter

astro-ph.GA2017★ 5 cited

AGN with discordant optical and X-ray classification are not a physical family: Diverse origin in two AGN

I. Ordovás-Pascual, S. Mateos, F. J. Carrera +7

Approximately 3-17 percent of Active Galactic Nuclei (AGN) without detected rest-frame UV/optical broad emission lines (type-2 AGN) do not show absorption in X-rays. The physical o…

astro-ph.GA2016★ 6 cited

Water masers in Compton-thick AGN I. Detailed study of the new water megamaser in IRAS15480-0344

P. Castangia, A. Tarchi, A. Caccianiga +2

A relationship between the water maser detection rate and large nuclear column densities in AGN has often been cited in the literature. Indeed, detailed studies of luminous water m…

astro-ph.GA2015★ 7 cited

Exploring the Active Galactic Nuclei population with extreme X-ray to optical flux ratios (Fx/Fo >50)

R. Della Ceca, F. J. Carrera, A. Caccianiga +8

The cosmic history of the growth of supermassive black holes in galactic centers parallels that of star-formation in the Universe. However, an important fraction of this growth occ…

astro-ph.GA2014★ 33 cited

A Focused, Hard X-ray Look at Arp 299 with NuSTAR

A. Ptak, A. Hornschemeier, A. Zezas +19

We report on simultaneous observations of the local starburst system Arp 299 with NuSTAR and Chandra, which provides the first resolved images of this galaxy up to energies of ~ 45…

astro-ph.GA2014★ 9 cited

The XMM-Newton Bright Survey sample of absorbed quasars: X-ray and accretion properties

L. Ballo, P. Severgnini, R. Della Ceca +5

Although absorbed quasars are extremely important for our understanding of the energetics of the Universe, the main physical parameters of their central engines are still poorly kn…

astro-ph.GA2014★ 50 cited

SDSSJ143244.91+301435.3: a link between radio-loud narrow-line Seyfert 1 galaxies and compact steep-spectrum radio sources?

A. Caccianiga, S. Antón, L. Ballo +12

We present SDSSJ143244.91+301435.3, a new case of radio-loud narrow line Seyfert 1 (RL NLS1) with a relatively high radio power (P1.4GHz=2.1x10^25 W Hz^-1) and large radioloudness…

astro-ph.GA2014★ 28 cited

X-ray observation of ULAS J1120+0641, the most distant quasar at z=7.08

A. Moretti, L. Ballo, V. Braito +6

We aim at probing the emission mechanism of the accreting super massive black holes in the high redshift Universe. We study the X-ray spectrum of ULAS1120+0641, the highest redshif…

astro-ph.GA2013★ 7 cited

The variable ionized absorber in the Seyfert 2 Mrk 348

E. Marchese, V. Braito, J. N Reeves +6

We present the results of the analysis of the X-ray spectrum of the Seyfert 2 Mrk 348, observed by Suzaku and XMM-Newton. The overall spectrum of Mrk 348 can be described by a prim…

astro-ph.GA2009★ 20 cited

A Suzaku observation of the ULIRG IRAS19254-7245: disclosing the AGN component

V. Braito, J. N. Reeves, R. Della Ceca +3

We discuss here a long Suzaku observation of IRAS 19254-7245 (also known as the Superantennae), one of the brightest and well studied Ultra Luminous Infrared Galaxies in the local…