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researcher

C. Boisson

29 papers hereh-index 6419.7k citations513 works total

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

author position
  • first author1
  • middle author10

Across the 11 of 29 papers where every author was matched, so the position is known.

fields
  • astro-ph27
  • astro-ph.CO1
  • astro-ph.HE1
same name
  • C. Boisson — 16 papers
  • C. Boisson — 2 papers
  • C. Boisson — 2 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

activity
19952009
most citedFast variability of TeV gamma-rays from the radio galaxy M 87

342 citations · 1.3k across the 19 of their papers we have counts for

collaborators
Showing 2008Show all

4 papers · 1 filter

astro-ph2008★ 34 cited

H.E.S.S. Observations of the Prompt and Afterglow Phases of GRB 060602B

HESS Collaboration, F. Aharonian

We report on the first completely simultaneous observation of a gamma-ray burst (GRB) using an array of Imaging Atmospheric Cherenkov Telescopes which is sensitive to photons in th…

astro-ph2008★ 30 cited

Modelling rapid TeV variability of PKS 2155-304

K. Katarzynski, J-P. Lenain, A. Zech +2

We present theoretical modelling for the very rapid TeV variability of PKS 2155--304 observed recently by the H.E.S.S. experiment. To explain the light-curve, where at least five f…

astro-ph2008★ 146 cited

The characteristic blue spectra of accretion disks in quasars as uncovered in the infrared

Makoto Kishimoto, Robert Antonucci, Omer Blaes +4

Quasars are thought to be powered by supermassive black holes accreting surrounding gas. Central to this picture is a putative accretion disk which is believed to be the source of…

astro-ph2008

SSC scenario for VHE emission from 2 radiogalaxies: M 87 and Cen A

Jean-Philippe Lenain, Catherine Boisson, Hélène Sol

M 87 is the first extragalactic source detected in the Very High Energy (VHE; E > 100 GeV) gamma-ray domain that is not a blazar, its large scale jet not being aligned to the line…

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