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researcher

S. Belladitta

62 papers hereh-index 9259 citations68 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author7
  • middle author45

Across the 52 of 62 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA48
  • astro-ph.HE11
  • astro-ph.IM2
  • astro-ph.CO1
same name
  • S. Belladitta — 1 paper, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20192026
most citedThe first blazar observed at z>6

92 citations · 553 across the 58 of their papers we have counts for

collaborators
Showing 2021Show all

4 papers · 1 filter

astro-ph.HE2021★ 26 cited

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

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

We report on the direct observation of an extended X-ray jet in the z=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…

astro-ph.GA2021★ 39 cited

Radio Detection of VIK J2318−3113, the Most Distant Radio-Loud Quasar (z=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 J2318−3113, a z=6.44 quasar. Its radio luminosity (1.2 ×1026 W Hz−1 at 5…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.