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researcher

G. Bernardi

4 papers hereh-index 29 citations5 works total

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

author position
  • middle author2
  • last author2

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • astro-ph.CO1
  • astro-ph.GA1
same name
  • G. Bernardi — 133 papers, h 7
  • G. Bernardi — 96 papers, h 77
  • G. Bernardi — 89 papers
  • G. Bernardi — 78 papers, h 64
  • G. Bernardi — 53 papers
  • G. Bernardi — 39 papers

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

most citedRadio-loud fraction of z>6 quasars

11 citations · 11 across the 3 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2026

The spectrum of the persistent radio source associated with FRB 20190417A

L. Bruno, D. Pelliciari, G. Bernardi +3

Persistent radio sources (PRSs) are (sub-)parsec-scale compact non-thermal continuum sources associated with some repeating fast radio bursts (FRBs). Their nature is debated, but t…

astro-ph.CO2026

WIMP Dark Matter Searches in Reticulum II Using MeerKAT

Shibre Semane, Geoff Beck, Sphesihle Makhathini +2

In the last decade radio astronomy has emerged as a powerful technique for detecting signatures of Weakly Interacting Massive Particles (WIMPs). Dwarf spheroidal galaxies (dSphs) a…

astro-ph.HE2024

The MeerKAT Massive Distant Clusters Survey: A Radio Halo in a Massive Galaxy Cluster at z = 1.23

S. P. Sikhosana, M. Hilton, G. Bernardi +9

In the current paradigm, high redshift radio halos are expected to be scarce due to inverse Compton energy losses and redshift dimming, which cause them to be intrinsically faint.…

astro-ph.GA2024★ 11 cited

Radio-loud fraction of z>6 quasars

Pascal M. Keller, Nithyanandan Thyagarajan, Ajay Kumar +2

Quasars at redshifts z>6 are an excellent probe of the formation and evolution of supermassive black holes in the early Universe. The population of radio-luminous quasars is of p…

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