The SVOM Mission
arXiv:2203.10962 · doi:10.1142/S0218271822300087
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-meter 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.
19 pages, 12 figures, Based on a talk presented at the Sixteenth Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories, online, July 2021. International Journal of Modern Physics, Pub Date : 2021-12-17
References in corpus (10)
- The Zwicky Transient Facility: System Overview, Performance, and First Results
- No supernovae associated with two long-duration gamma ray bursts
- An enigmatic long-lasting gamma-ray burst not accompanied by a bright supernova
- Science with ASKAP - the Australian Square Kilometre Array Pathfinder
- Teraelectronvolt emission from the -ray burst GRB 190114C
- A very-high-energy component deep in the Gamma-ray Burst afterglow
- MeerKAT Key Project Science, Specifications, and Proposals
- The new SOXS instrument for the ESO NTT
- The Microchannel X-ray Telescope for the Gamma-Ray Burst mission SVOM
- Detection of short high-energy transients in the localuniverse with SVOM/ECLAIRs