The SVOM mission

Author:

Atteia J.-L.1,Cordier B.2,Wei J.3

Affiliation:

1. IRAP, Université de Toulouse, CNRS, CNES, UPS, (Toulouse), France

2. Lab AIM – CEA, CNRS, Université Paris-Saclay, Université de Paris, 91191, Gif-sur-Yvette, France

3. Key Laboratory of Space Astronomy and Technology, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China

Abstract

The Sino-French space mission SVOM is mainly designed to detect, localize and follow-up Gamma-Ray Bursts and other high-energy transients. The satellite, to be launched mid 2023, embarks two wide-field gamma-ray instruments and two narrow-field telescopes operating at X-ray and optical wavelengths. It is complemented by a dedicated ground segment encompassing a set of wide-field optical cameras and two 1-m class follow-up telescopes. In this contribution, we describe the main characteristics of the mission and discuss its scientific rationale and some original GRB studies that it will enable.

Publisher

World Scientific Pub Co Pte Ltd

Subject

Space and Planetary Science,Astronomy and Astrophysics,Mathematical Physics

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