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Flesh up XMM section #27

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33 changes: 28 additions & 5 deletions VOHE-Note.tex
Original file line number Diff line number Diff line change
Expand Up @@ -224,11 +224,34 @@ \subsubsection{Chandra}\label{sec:chandra}

\subsubsection{XMM-Newton}

The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched in 1999. XMM-Newton is ESA's
second cornerstone of the Horizon 2000 Science Program. It carries 3 high throughput X-ray telescopes with an
unprecedented effective area, and an optical monitor, dedicated to the study of celestial X-ray sources.

\todo[inline]{To be completed: XMM catalogs, data... and VO access.}
The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) \footnote{https://www.cosmos.esa.int/web/xmm-newton}
was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme.
It carries 3 high throughput X-ray telescopes with an unprecedented effective area, 2 reflexion grating spectrometers and an optical monitor.
The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations.
The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes
to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community,
applying for observational periods on a competitive basis.

One of the mission's ground segment modules, the SSC /footnote{http://xmmssc.irap.omp.eu/}, is in charge of maximizing the scientific return of
this space observatory by exhaustively analyzing
the content of the instruments' fields of view. During the development phase (1996-1999), the SSC,
in collaboration with the SOC (ESAC), designed and produced the scientific analysis software (SAS).
Since then, it has contributed to its maintenance and development. This software is publicly available.

The general pipeline is operated as ESAC (Villafranca, Spain) since 2012, except for the part concerning cross-correlation
with astronomical archives which runs in Strasbourg.
The information thus produced is intended for the guest observer and, after a proprietary period of one year,
for the international community.
In parallel, the SSC regularly compiles an exhaustive catalog of all X-ray sources detected by EPIC cameras.
The SSC validates these catalogs, enriches them with multi-wavelength data and exploits them in several scientific programs.

The XMM catalog is published through various WEB applications: XSA \footnote{https://www.cosmos.esa.int/web/xmm-newton/xsa},
XCatDB \footnote{https://xcatdb.unistra.fr/4xmm}, IRAP \footnote{http://xmm-catalog.irap.omp.eu/} and
HEASARCH \footnote{http://heasarc.gsfc.nasa.gov/db-perl/W3Browse/w3browse.pl}.
It is also published in the VO, mainly as TAP services.
It is to be noted that the TAP service operated in Strasbourg (\url{https://xcatdb.unistra.fr/xtapdb} - to be deployed in 10/2024) returns responses where data is mapped on the MANGO model with MIVOT.

\todo[inline]{To be validated by ADA.}


\subsubsection{SVOM}
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