L. Maraschi

TL;DR: The connection between the accretion process that powers AGN and the formation of jets is still poorly understood as discussed by the authors, and the authors of this paper use deep Chandra and xmm observations of the cores of three powerful radio loud quasars: 1136--135, 1150+497 (\chandra), and 0723+679 (\xmm), in the redshift range $z$=0.3-0.8.

TL;DR: In this paper, the authors present a re-analysis of the simultaneous ∼30 day IUE/XTE observation of NGC 7469 done in 1996, which allows one to fit simultaneously the data from the UV to the hard X-ray band in a selfconsistent way.

TL;DR: In this paper, the authors proposed a method to use the Fermi Guest Investigator grant for the Spanish MINECO under the NASA Earth and Space Science Fellowship Program (ESF).

TL;DR: In this article, the authors presented the evidence for the existence of a fourth extended X-ray jet in the classical radio-selected source S5 2007+777, which for its hybrid FR I and FR II radio morphology has been classified as a HYMOR (HYbrid MOrphology Radio source).

TL;DR: In this article, BeppoSAX observations of two Seyfert 1 galaxies have been used to establish the presence of soft excesses in both sources, even if for Mrk 841 a warm absorber provides a t almost as good as the one with a true excess.