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researcher

G. Giovannini

154 papers hereh-index 478.1k citations341 works total

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

author position
  • sole author2
  • first author21
  • middle author89
  • last author11

Across the 123 of 154 papers where every author was matched, so the position is known.

fields
  • astro-ph57
  • astro-ph.HE42
  • astro-ph.CO36
  • astro-ph.GA17
  • astro-ph.IM2
same name
  • G. Giovannini — 75 papers, h 28
  • G. Giovannini — 7 papers
  • G. Giovannini — 5 papers, h 1
  • G. Giovannini — 3 papers, 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
19942024
most citedClusters of galaxies : observational properties of the diffuse radio emission

644 citations · 8k across the 148 of their papers we have counts for

collaborators
Showing 1998Show all

4 papers · 1 filter

astro-ph1998★ 26 cited

The Radio-Optical Jet in NGC 3862 from Parsec tu Sub-Kiloparsec Scales

L. Lara, L. Feretti, G. Giovannini +4

We have observed the radio source NGC 3862 (3C264) simultaneously with the EVN and the MERLIN arrays, obtaining detailed images of its radio structure from parsec to sub-kiloparsec…

astro-ph1998

VLBI Observations of Mkn 501 and Mkn 421

G. Giovannini, L. Feretti, T. Venturi +2

We present here two epochs of Space VLBI observations at 18 cm of the BL-Lac type object Mkn 501. Thanks to the high resolution of these new data we have found that the inner jet i…

astro-ph1998★ 1 cited

Space VLBI Observations of MKN501

G. Giovannini, W. D. Cotton, L. Feretti +2

We present here two epochs of Space VLBI Observations at 18 cm of the BL-Lac type object MKN 501. Thanks to the high resolution of these new data, we have found that the inner jet…

astro-ph1998★ 1 cited

Beppo-Sax Observation of the Coma cluster

R. Fusco-Femiano, D. Dal Fiume, L. Feretti +3

We present first results of the BeppoSAX observation of the Coma Cluster. Thanks to the unprecedented sensitivity of the PDS instrument, the source has been detected up to ~80 keV.…

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