activity
20182026
most citedX-ray properties of z>4 blazars

38 citations · 120 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2026

The most extreme high-z radio quasars in the eRASS:1 X-ray survey

L. Ighina, L. Palmieri, L. N. Martínez-Ramírez +7

We present the selection and identification of high-z radio quasars from a combination of X-ray (eROSITA All-Sky Survey), optical/NIR (DECam Local Volume Exploration), and radio (R…

astro-ph.GA2026

SKAVLBI view of AGN jets in the early Universe

C. Spingola, M. Mezcua, Y. Liu +33

Active Galactic Nuclei (AGN) are among the brightest sources in the Universe, and those that are also jetted are uniquely valuable at the earliest epochs, because their relativisti…

astro-ph.GA2026

Milliarcsecond-resolution Radio-imaging Survey of Blazar Candidates at 4 < z < 5.4

Máté Krezinger, Alessandro Caccianiga, Daniele Dallacasa +9

We present a milliarcsecond-resolution radio survey of 17 high-redshift (4 < z < 5.4) blazar candidates observed with the European Very Long Baseline Interferometry (VLBI) Network…

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.HE2025★ 2 cited

Flat Spectrum Radio Quasars as high-energy neutrino sources

Alberto Moretti, Alessandro Caccianiga

The astrophysical sources responsible for the production of high-energy neutrinos remain largely uncertain. The strongest associations suggest a correlation between neutrinos and a…

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.GA2024★ 8 cited

Multi-wavelength properties of three new radio-powerful quasi-stellar objects discovered from RACS

L. Ighina, A. Caccianiga, A. Moretti +12

We present a multi-wavelength study of three new quasi-stellar objects (QSOs) identified from dedicated spectroscopic observations. The three sources were selected as hi…

astro-ph.GA2024★ 7 cited

Comprehensive view on a radio-loud QSO: from the radio to the optical/NIR to the X-ray band

Luca Ighina, Alessandro Caccianiga, Alberto Moretti +9

We present a multi-wavelength analysis, from the radio to the X-ray band, of the redshift VIK J231831 radio-loud (RL) quasi stellar object (QSO), one of the most distan…

astro-ph.GA2022★ 26 cited

The evolution of the heaviest super-massive black-holes in jetted AGNs

Alessandro Diana, Alessandro Caccianiga, Alberto Moretti +3

We present the space density evolution, from z=1.5 up to z=5.5, of the most massive (MM) black holes hosted in jetted Active Galactic Nuclei(AGNs). The analysis…

astro-ph.GA2019★ 38 cited

X-ray properties of z>4 blazars

L. Ighina, A. Caccianiga, A. Moretti +4

We present the X-ray analysis of the largest flux-limited complete sample of blazar candidates at z>4 selected from the Cosmic Lens All Sky Survey (CLASS). After obtaining a nearly…

astro-ph.HE2018★ 33 cited

Swift data hint at a binary Super Massive Black Hole candidate at sub-parsec separation

P. Severgnini, C. Cicone, R. Della Ceca +10

Dual/binary Supermassive Black Hole (SMBH) systems are the inevitable consequence of the current Lambda Cold Dark Matter cosmological paradigm. In this context, we discuss here the…