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Merge branch 'main' into xmm-contrib
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mservillat authored Sep 27, 2024
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*.pdf
*.toc
ivoatexmeta.tex
.project
.project
28 changes: 23 additions & 5 deletions VOHE-Note.tex
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Expand Up @@ -256,11 +256,29 @@ \subsubsection{XMM-Newton}

\subsubsection{SVOM}

The SVOM mission (Space-based multi-band astronomical Variable Objects Monitor) is a Franco-Chinese mission dedicated
to the study of the most distant explosions of stars, the gamma-ray bursts. It is to be launched in 2024.

\todo[inline]{To be completed}

SVOM (Space-based multi-band astronomical Variable Objects Monitor) \footnote{https://www.svom.eu/en/home/}
is a Sino-French mission dedicated
to the study of the transient high-energy sky, and in particular to the detection, localization and
study of Gamma Ray Bursts (GRBs).
Gamma-ray bursts are sudden, intense flashes of X-ray and gamma-ray light.
They are associated with the cataclysmic formation of black holes, either by the merger of two compact stars
(neutron star or black hole) or by the sudden explosion of a massive star, twenty to one hundred times the mass of our Sun.
The birth of a black hole is accompanied by the ejection of jets of matter that reach speeds close to the speed of light.
These jets of matter then decelerate in the circumstellar medium, sweeping away everything in their path.
Gamma-ray bursts can be observed at the very edge of the universe, acting as lighthouses that illuminate
the dark ages of its creation. Although they have been studied extensively over the past fifteen years,
gamma-ray bursts are still poorly understood phenomena. To better understand them, China and France have decided
to join forces with the SVOM satellite, which is specifically dedicated to the study of gamma-ray bursts.

The special feature of the SVOM mission is that it combines ground-based and space-based observations,
providing a spectral bandwidth from the visible to the high-energy range. By guaranteeing multi-wavelength
observations of about one hundred bursts of all types per year, the SVOM mission will make a unique contribution
to two of the most fruitful areas of research in recent decades: the use of bursts in cosmology and the understanding
of the phenomenon. Looking further ahead, the SVOM mission will work in close synergy with a new generation of
instruments dedicated to the search for neutrinos and gravitational waves of cosmic origin, in order to confirm
the astrophysical origin of the signals detected by these future instruments.

SVOM has been successfully launched on June 22 2024 from Xichang lauchpad.


\subsection{KM3Net and neutrino detection}
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