activity
19982022
most citedThe shock break-out of GRB 060218/SN 2006aj

789 citations · 5.9k across the 76 of their papers we have counts for

collaborators

77 papers

astro-ph.GA2022★ 11 cited

A powerful (and likely young) radio-loud quasar at z=5.3

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

We present the discovery of PSO J191.0569686.43172 (hereafter PSO J19186), a new powerful radio-loud quasar (QSO) in the early Universe (z = 5.32). We discovered it by cross-…

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.HE2022★ 16 cited

The central engine of the highest redshift blazar

Silvia Belladitta, Alessandro Caccianiga, Alessandro Diana +8

We report on a LUCI/Large Binocular Telescope near-infrared (NIR) spectrum of PSO J030947.49+271757.31 (hereafter PSO J0309+27), the highest redshift blazar known to date (z6…

astro-ph.HE2021★ 26 cited

Direct observation of an extended X-ray jet at =6.1

L. Ighina, A. Moretti, F. Tavecchio +6

We report on the direct observation of an extended X-ray jet in the =6.1 radio-loud Active Galactic Nucleus PSO J030947.49+271757.31 from a deep Chandra X-ray observation (128 k…

astro-ph.HE2021★ 1 cited

Minute-timescale variability in the X-ray emission of the highest redshift blazar

Alberto Moretti, Gabriele Ghisellini, Alessandro Caccianiga +9

We report on two Chandra observations of the quasar PSO J0309+27, the most distant blazar observed so far (z=6.1), performed eight months apart, in March and November 2020. Previou…

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…