activity
20242026
most citedThe Wide Field Monitor (WFM) of the China-Europe eXTP (enhanced X-ray Timing and Polarimetry) mission

4 citations · 5 across the 11 of their papers we have counts for

collaborators
Showing 2026Show all

7 papers · 1 filter

astro-ph.HE2026

GRB 250424A: A Case Study of Energy Injection with Multiwavelength Observations

Yifang Liang, Yun Wang, WeiKang Zheng +61

We present a comprehensive multiwavelength analysis of the long-duration gamma-ray burst (GRB) 250424A. Our dataset spans from the prompt gamma-ray emission to late-time optical mo…

astro-ph.IM2026

Building on SVOM : the CATCH satellite constellation for transient astronomy

Stéphane Schanne

Building on the success of the French-Chinese SVOM mission, our consortium proposes CATCH (Chasing All Transients Constellation of Hunters), targeting Gamma-Ray Bursts and X-ray tr…

astro-ph.HE2026

The coded mask of the ECLAIRs telescope onboard the SVOM space mission

C. Lachaud, A. Givaudan, M. Karakac +9

ECLAIRs is a hard X-ray coded-mask telescope onboard the SVOM space mission, designed to detect and localize high-energy transients, in particular gamma-ray bursts. Operating over…

astro-ph.HE2026

Overview of the ECLAIRs Trigger for SVOM gamma-ray burst detection

S. Schanne, F. Château, N. Dagoneau +3

The French-Chinese SVOM satellite mission (Space-based multi-band astronomical Variable Objects Monitor) was launched in mid-2024, with science objectives focused on the detection…

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.HE2026

XRF 241001A/SN 2024aiiq: A faint soft X-ray transient detected by SVOM with a broad-line type Ic supernova revealed by JWST

B. Schneider, M. Brunet, B. P. Gompertz +61

X-ray flashes (XRFs) are a type of gamma-ray burst (GRB) with prompt emission predominantly below 30 keV and have been poorly detected by previous missions. The advent of the SVOM…