activity
20002007
most citedStatistics of relativistically broadened Fe K-alpha lines in AGN

51 citations · 51 across the 4 of their papers we have counts for

collaborators

9 papers

astro-ph2007

PopStar: A new grid of Evolutionary Synthesis Models in the Virtual Observatory

Marisa García-Vargas, Mercedes Mollá, Alessandro Bressan +1

We present a new set of theoretical evolutionary synthesis models, PopStar. This grid of Single Stellar Populations covers a wide range in both, age and metallicity. The models use…

astro-ph2007

A new grid of evolutionary synthesis models

M. Mollá, M. L. García-Vargas, Alessandro Bressan +1

We present new evolutionary synthesis models for Single Stellar Populations covering a wide range in age and metallicity. The most important difference with existing models is the…

astro-ph200651 cited

Statistics of relativistically broadened Fe K-alpha lines in AGN

M. Guainazzi, S. Bianchi, M. Dovciak

We present preliminary results on the properties of relativistically broadened Fe K-alpha lines in a collection of more then 100 Active Galactic Nuclei (AGN) observed by the XMM-Ne…

astro-ph2005

The hard X-ray view of Giga-Hertz Peaked Spectrum Radio Galaxies

M. Guainazzi, A. Siemiginowska, C. Stanghellini +3

We present the first broadband X-ray observations of four Giga-Hertz Peaked Spectrum (GPS) radio galaxies at redshift <~1 performed by Chandra and XMM-Newton. These observations mo…

astro-ph2004

The early stage of a cosmic collision? XMM-Newton unveils two obscured AGN in the galaxy pair ESO509-IG066

M. Guainazzi, E. Piconcelli, E. Jimenez-Bailon +1

We report the XMM-Newton discovery of a X-ray bright AGN pair in the interacting galaxy system ESO509-IG066. Both galaxies host an X-ray luminous (L_X ~10^{43} erg/s) obscured nucl…

astro-ph2004

An ISOCAM survey through gravitationally lensing galaxy clusters. III. New results from mid-infrared observations of th e cluster Abell 2219

D. Coia, L. Metcalfe, B. McBreen +7

The massive cluster of galaxies Abell 2219 (z = 0.228) was observed at 14.3 m with the Infrared Space Observatory and results were published by Barvainis et al. (1999). These ob…