activity
19972009
most citedXMM-Newton observations of a sample of gamma-ray loud active galactic nuclei

52 citations · 184 across the 20 of their papers we have counts for

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astro-ph2005

BeppoSAX view of radio-loud Active Galactic Nuclei

Paola Grandi, Giuseppe Malaguti, Mariateresa Fiocchi +1

A systematic analysis of a large sample of radio-loud Active Galactic Nuclei available in the BeppoSAX public archive has been performed. The sample includes 3 Narrow Line Radio Ga…

astro-ph2005

INTEGRAL and XMM-Newton observations of the X-ray pulsar IGR J16320-4751/AX J1631.9-4752

J. Rodriguez, A. Bodaghee, P. Kaaret +16

We report on observations of the X-ray pulsar IGR J16320-4751 (a.k.a. AX J1631.9-4752) performed simultaneously with INTEGRAL and XMM-Newton. We refine the source position and iden…

astro-ph2005

A new XMM-Newton observation of Pictor A radio lobes confirms the non-thermal origin of the X-ray emission

G. Migliori, P. Grandi, G. G. C. Palumbo +3

X-ray emission from the eastern radio lobe of the FRII Radio Galaxy Pictor A was serendipitously discovered by a short observation of XMM-Newton in 2001. The X-ray spectrum, accumu…

astro-ph2005

The XMM-Newton view of gamma-ray loud active nuclei

L. Foschini, G. Ghisellini, C. M. Raiteri +8

Notwithstanding the big efforts devoted to the investigation of the mechanisms responsible for the high-energy (E>100 MeV) gamma-ray emission in active galactic nuclei (AGN), the d…

astro-ph2005

X-ray Spectral Survey with XMM--Newton of a Complete Sample of Nearby Seyfert Galaxies

M. Cappi, F. Panessa, L. Bassani +15

Results obtained from an X-ray spectral survey of nearby Seyfert galaxies using XMM--Newton are reported. The sample was optically selected, well defined, complete in B mag, and di…

astro-ph2005

Active and passive shielding design optimization and technical solutions for deep sensitivity hard X-ray focusing telescopes

G. Malaguti, G. Pareschi, P. Ferrando +12

The 10-100 keV region of the electromagnetic spectrum contains the potential for a dramatic improvement in our understanding of a number of key problems in high energy astrophysics…