activity
19972026
most citedTemporal and spectral gamma-ray properties of Mkn421 above 250 GeV from CAT observations between 1996 and 2000

146 citations · 1k across the 39 of their papers we have counts for

collaborators

40 papers

astro-ph.HE2026

The GRB joint scientific analysis pipeline of the ECLAIRs and GRM instruments on board SVOM

F. Piron, F. Daigne, T. Maiolino +35

The study of the prompt high-energy emission of Gamma-Ray Bursts (GRBs) with SVOM relies on the observations performed by ECLAIRs (4-150 keV) and the Gamma-Ray Monitor (GRM, 0.015-…

astro-ph.IM2026

SVOM/ECLAIRs detection plane: main features and performance

O. Godet, J. -L. Atteia, R. Pons +21

The detection plane of the high-energy transient camera ECLAIRs onboard SVOM is made of 200 XRDPIX detection modules, each consisting of a matrix of Schottky-type CdTe…

astro-ph.HE2026

ECLAIRs: the SVOM high-energy transient trigger camera

O. Godet, J. -L. Atteia, S. Schanne +51

The core instrument of the SVOM Gamma-ray burst mission launched in June 2024 is the 4-150 keV 2-D coded mask camera ECLAIRs responsible for the autonomous trigger and localization…

astro-ph.HE2025★ 6 cited

GRB 221009A and the Apparently Most Energetic Gamma-Ray Bursts

J-L. Atteia, L. Bouchet, J-P. Dezalay +7

Gamma-Ray Bursts (GRBs) are often referred to as the most luminous explosions in the Universe, due to their short and highly luminous prompt emission. This apparent luminosity, how…

astro-ph.IM2019★ 2 cited

Designing large pixelated CdTe detection planes for hard X-ray transients detection

K. Lacombe, C. Amoros, J. -L. Atteia +10

We discuss the need for very large detection planes for the detection of hard X-ray transients in the multi-messenger era that started with the quasi-simultaneous detection of GRB~…

astro-ph.HE2016★ 12 cited

Investigating the impact of optical selection effects on observed rest frame prompt GRB properties

Damien Turpin, Vincent Heussaff, Jean-Pascal Dezalay +3

Measuring gamma-ray burst (GRB) properties in their rest-frame is crucial to understand the physics at work in gamma-ray bursts. This can only be done for GRBs with known redshift.…