361 citations · 8.4k across the 127 of their papers we have counts for
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A Simultaneous RXTE and XMM-Newton Observation of the Broad-Line Radio Galaxy 3C 111
Karen T. Lewis, Michael Eracleous, Mario Gliozzi +2
We present the results of simultaneous XMM-Newton and RXTE observations of the Broad-Line Radio Galaxy 3C 111. We find that the Compton reflection bump is extremely weak, however,…
A Chandra Snapshot Survey of IR-bright LINERs: A Possible Link Between Star Formation, AGN Fueling, and Mass Accretion
R. P. Dudik, S. Satyapal, M. Gliozzi +1
We present results from a high resolution X-ray imaging study of nearby LINERs observed by Chandra. This study complements and extends previous X-ray studies of LINERs, focusing on…
An X-ray view of WLRGs/LINERs
Alexander S. Rinn, Rita M. Sambruna, Mario Gliozzi
We present X-ray observations of nine Weak-Line Radio Galaxies (WLRGs), optically classified as confirmed or possible Low Ionization Nuclear Emission-line Regions (LINERs). The dat…
Non-stationary variability in AGN: the case of 3C 390.3
M. Gliozzi, I. E. Papadakis, R. M. Sambruna +1
We use data from a two-year intensive RXTE monitoring campaign of the broad-line radio galaxy 3C 390.3 to investigate its stationarity. In order to exploit the potential informatio…
Obscuration and Origin of Nuclear X-ray emission in FR I Radio Galaxies
D. Donato, R. M. Sambruna, M. Gliozzi
We present X-ray observations of the nuclear region of 25 Fanaroff-Riley I radio galaxies from the 3CRR and B2 catalogs, using data from the Chandra and XMM archives. We find the p…
Jets from Sub-Parsec to Kiloparsec Scales: A Physical Connection
F. Tavecchio, L. Maraschi, R. M. Sambruna +4
The Chandra discovery of bright X-ray emission from kpc-scale jets allows insight into the physical parameters of the jet flow at large scale. At the opposite extreme, extensive st…
A survey of extended radio jets with Chandra and HST
R. M. Sambruna, J. K. Gambill, L. Maraschi +5
We present the results from an X-ray and optical survey of a sample of 17 radio jets in AGN performed with Chandra and HST. The sample was selected from the radio and is unbiased t…