The Chinese-French SVOM mission for GRBs studies

TL;DR

The SVOM mission is a joint Chinese-French project designed to detect, localize, and study gamma-ray bursts across multiple wavelengths, enhancing our understanding of these energetic cosmic events with innovative instruments and coordinated ground support.

Contribution

This paper introduces the SVOM mission, a novel multi-instrument satellite with ground-based support, aimed at comprehensive GRB detection and analysis, including high-redshift events.

Findings

First real-time localizations of GRBs with arcminute accuracy.

Broadband spectral and temporal measurements of GRB prompt emission.

Enhanced follow-up capabilities with ground-based telescopes.

Abstract

We present the SVOM (Space-based multi-band astronomical Variable Objects Monitor) mission that the Chinese National Space Agency and the French Space Agency have decided to jointly implement. SVOM has been designed to detect all known types of gamma-ray bursts (GRBs), to provide fast and reliable GRB positions, to measure the broadband spectral shape and temporal properties of the GRB prompt emission, and to quickly identify the optical/near-infrared afterglows of detected GRBs, including high-redshift ones. Scheduled to be in orbit in the second half of the present decade, the SVOM satellite will carry a very innovative scientific payload combining for the first time a wide field X- and gamma-ray coded mask imager for GRB real-time localizations to few arcmin, a non-imaging gamma-ray monitor, and two narrow-field instruments for the study of the GRB early afterglow emission in the X-ray and visible bands. The SVOM payload is complemented by ground-based instruments including a wide-field camera to catch the GRB prompt emission in the visible band and two robotic telescopes to measure the photometric properties of the early afterglow. A particular attention is paid to the GRB follow-up in facilitating the observation of the SVOM detected GRB by the largest ground based telescopes.