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20192026
most citedThe space density of z>4 blazars

39 citations · 223 across the 22 of their papers we have counts for

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astro-ph.GA2026

Extreme Enrichment at Cosmic Dawn: Three FeII-Strong Quasars at z > 6 from the JWST Aether survey

Anniek J. Gloudemans, Emanuele Paolo Farina, Roberto Decarli +22

We present three outliers on the quasar main sequence at z>6, as revealed by JWST/NIRSpec IFU observations from the Aether survey, a program targeting ~200 quasars at cosmic dawn.…

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

The Road to Identifying the Earliest Radio-Powerful AGN with the SKA

Jose Afonso, Stergios Amarantidis, Stas Shabala +20

The Epoch of Reionization (EoR) is one of the most pivotal frontiers in modern astrophysics, marking the emergence of the first galaxies, stars, and supermassive black holes (SMBHs…

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.GA2025

The Centre of Attention: a Powerful Radio Galaxy Pinpoints a NIR-Dark Protocluster at z~3.9

A. J. Hedge, N. Seymour, J. W. Broderick +8

We report the discovery of a protocluster identified from Atacama Large Millimetre/sub-millimetre Array Band 3 spectral scans of a bright radio source selected from the…

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.GA2025★ 11 cited

ESPRESSO reveals a single but perturbed broad-line region in the supermassive black hole binary candidate PG 1302-102

Fabio Rigamonti, Paola Severgnini, Erika Sottocorno +12

We present a new, Bayesian analysis of the highest-resolution optical spectrum of the supermassive black hole (SMBH) binary candidate PG 1302-102, obtained with ESPRESSO@VLT (R \si…

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.GA2024

Obscuration in high redshift jetted QSO

A. Caccianiga, L. Ighina, A. Moretti +6

Obscuration in high-redshift quasi-stellar objects (QSO) has a profound impact on our understanding of the evolution of supermassive black holes across the cosmic time. An accurate…

astro-ph.GA2022★ 21 cited

New Radio-Loud QSOs at the end of the Re-ionisation Epoch

L. Ighina, A. Caccianiga, A. Moretti +5

We present the selection of high-redshift () radio-loud (RL) quasi-stellar object (QSO) candidates from the combination of the radio Rapid ASKAP Continuum Survey (RACS…

astro-ph.GA2022

Impact of the CMB on the evolution of AGNs and their relativisitc jets at the highest redshift

Luca Ighina

Radio-Loud (RL) Active Galactic Nuclei (AGNs) are among the brightest astrophysical sources at all wavelengths. Their relativistic jets can affect both their Supermassive Black Hol…

astro-ph.GA2022★ 14 cited

Constraining the Radio Properties of the =6.44 QSO VIK J23183113

Luca Ighina, James K. Leung, Jess W. Broderick +19

The recent detection of the quasi-stellar object (QSO) VIKING J231818.3311346 (hereafter VIK J23183113) at redshift in the Rapid ASKAP Continuum Survey (RACS) uncove…

astro-ph.GA2021★ 11 cited

The Impact of the CMB on the Evolution of high-z Blazars

L. Ighina, A. Caccianiga, A. Moretti +3

Different works have recently found an increase of the average X-ray-to-radio luminosity ratio with redshift in the blazar population. We evaluate here whether the inverse Compton…

astro-ph.GA2021★ 39 cited

Radio Detection of VIK J23183113, the Most Distant Radio-Loud Quasar (=6.44)

L. Ighina, S. Belladitta, A. Caccianiga +4

We report the 888 MHz radio detection in the Rapid ASKAP Continuum Survey (RACS) of VIK J23183113, a =6.44 quasar. Its radio luminosity (1.2 W Hz at 5…

astro-ph.GA2019★ 20 cited

An extremely X--ray weak blazar at z=5

S. Belladitta, A. Moretti, A. Caccianiga +5

We present the discovery and properties of DESJ014132.4-542749.9 (DES0141-54), a new powerful radio-loud active galactic nucleus (AGN) in the early Universe (z=5.0). It was discove…

astro-ph.GA2019★ 39 cited

The space density of z>4 blazars

Alessandro Caccianiga, Alberto Moretti, Silvia Belladitta +9

High redshift blazars are an important class of Active Galactic Nuclei (AGN) that can provide an independent estimate of the supermassive black-hole mass function in high redshift…