activity
19982026
most citedGeneral physical properties of bright Fermi blazars

593 citations · 28.6k across the 519 of their papers we have counts for

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9 papers · 1 filter

astro-ph.GA2025

X-ray investigation of possible super-Eddington accretion in a radio-loud quasar at

L. Ighina, A. Caccianiga, T. Connor +19

We present radio and X-ray observations of the recently discovered radio-powerful quasar RACS J032021.44352104.1 using uGMRT, ATCA, LBA, and Chandra. The observed radio…

astro-ph.GA2025★ 6 cited

High- radio Quasars in RACS I: Selection, identification, and multi-wavelength properties

L. Ighina, A. Caccianiga, A. Moretti +21

Radio-bright, jetted quasars at serve as unique laboratories for studying supermassive black hole activity in the early Universe. In this work, we present a sample of high-$z…

astro-ph.GA2023★ 86 cited

Uncovering the geometry of the hot X-ray corona in the Seyfert galaxy NGC4151 with IXPE

V. E. Gianolli, D. E. Kim, S. Bianchi +106

We present an X-ray spectro-polarimetric analysis of the bright Seyfert galaxy NGC4151. The source has been observed with the Imaging X-ray Polarimetry Explorer (IXPE) for 700 ks,…

astro-ph.GA2018★ 44 cited

Detection of persistent VHE gamma-ray emission from PKS 1510-089 by the MAGIC telescopes during low states between 2012 and 2017

MAGIC Collaboration, V. A. Acciari, S. Ansoldi +165

PKS 1510-089 is a flat spectrum radio quasar strongly variable in the optical and GeV range. We search for low-state VHE gamma-ray emission from PKS 1510-089. We aim to characteriz…

astro-ph.GA2018★ 3 cited

On the orientation of Narrow Line Seyfert I

Tullia Sbarrato, Massimo Dotti, Giancarlo Ghirlanda +1

We study a sample of Narrow-line Seyfert 1 galaxies (NLS1) in their optical and radio features, in order to understand the differences between their radio silent, radio-loud and ra…

astro-ph.GA2017★ 24 cited

CMB-induced radio quenching of high-redshift jetted AGNs with highly magnetic hotspots

Jianfeng Wu, Gabriele Ghisellini, Edmund Hodges-Kluck +5

In an effort to understand the cause of the apparent depletion in the number density of radio-loud AGNs at , this work investigates the viability of the so-called Cosmic Micro…