Astron. Astrophys. Suppl. Ser. 138, 581-582
M. Bringer1 - M. Boër1 - C. Peignot1 - G. Fontan2 - C. Merce2
Send offprint request: M. Bringer, bringer@cesr.fr
1 -
Centre d'Études Spatiales des Rayonnements, CNRS, 9 Av. du Colonel Roche, 31028
Toulouse Cedex 04, France
2 -
Laboratoire d'Analyses et d'Architectures des Systèmes, 7 Av. du Colonel Roche, 31077
Toulouse Cedex 04, France
Received December 18, 1998; accepted March 12, 1999
TAROT (Télescope à Action Rapide pour les Objets Transitoires, Rapid Action
Telescope for Transient Objects) is an autonomous ground based observatory (Calern,
France) whose primary goal is the rapid detection of variable objects, peculiarly
optical counterparts of Gamma Ray Burst (GRB) sources. We present the observatory data
management architecture which is composed of 3 main modules: The MAJORDOME module
whose aim is to optimally schedule the observation requests sent to the telescope
through socket connections, e-mail or even a web interface, The CONTROL module which
monitors the hardware, and a data processing software TAITAR which detects, deblends,
measures, classifies sources and detects variable objects by comparison with a
catalogue. This paper will mainly focus on the MAJORDOME.
Key words: technique: image processory -- telescopes GRB
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