M. Boutelier

ORCID: 0000-0001-9645-1436
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About
Contact & Profiles
Research Areas
  • Gamma-ray bursts and supernovae
  • Astrophysical Phenomena and Observations
  • Pulsars and Gravitational Waves Research
  • Astronomical Observations and Instrumentation
  • Astrophysics and Cosmic Phenomena
  • Particle Detector Development and Performance
  • Astronomy and Astrophysical Research

Centre National d'Études Spatiales
2018-2023

The SVOM (Space-based multi-band astronomical Variable Objects Monitor) French-Chinese mission is dedicated to the detection, localization and study of Gamma Ray Bursts (GRBs) other high-energy transient phenomena. We first present general description French payload composed ECLAIRs instrument, GRB detection MXT follow-up observation in soft X-ray band. Then paper describes more detail design performances finally a status development will be given.

10.1117/12.2313561 article EN Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray 2018-07-06

Abstract The Space-based multiband astronomical Variableonboard computing resources. This Object Monitor (SVOM) is a Sino–French space mission targeting high-energy transient astrophysical objects such as gamma-ray bursts. soft X-ray part of the spectrum covered by Microchannel Telescope (MXT), which narrow field telescope designed to localize sources precisely. paper presents methods implemented on board characterize and with MXT. A specific localization method was developed accommodate...

10.3847/1538-4357/acb539 article EN cc-by The Astrophysical Journal 2023-02-01

Abstract The Microchannel X-ray Telescope (MXT) will be the first focusing telescope based on a "Lobster-Eye" optical design to flown Sino-French mission SVOM. SVOM dedicated study of Gamma-Ray Bursts and more generally time-domain astrophysics. MXT is compact (focal length ∼ 1.15 m) light (< 42 kg) instrument, sensitive in 0.2–10 keV energy range. It composed an system, micro-pore optics (MPOs) 40 µm pore size, coupled low-noise pnCDD detector. In this paper we describe expected...

10.21203/rs.3.rs-2064925/v1 preprint EN cc-by Research Square (Research Square) 2022-09-27
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