Speaker
Konstancja Satalecka
(Universidad Complutense de Madrid, Spain)
Description
The planned Cherenkov Telescope Array (CTA), a future ground-based Very-High-Energy (VHE) gamma-ray observatory, will be the largest Cherenkov project of its kind. It aims to provide an order of magnitude increase in sensitivity compared to currently operating VHE experiments and open access to guest observers. These features, together with the thirty years lifetime planned for the installation, impose severe constraints on the data model currently being developed for the project.
In this contribution we analyze the challenges faced by the CTA data model development and present the requirements imposed to face them. While the full data model is still not completed we show the organization of the work, status of the design, and an overview of the prototyping efforts carried out so far. We also show examples of specific aspects of the data model currently under development.
| Registration number following "ICRC2015-I/" | 197 |
|---|---|
| Collaboration | CTA |
Author
Jose Luis Contreras
(Universidad Complutense de Madrid)
Co-authors
Andrea Bulgarelli
(IASF, Bologna, Italy)
Andrea Zoli
(INAF/IASF, Bologna, Italy)
Catherine Boisson
(LUTH, Observatoire de Paris, France)
Claudia Lavalley
(LUPM, Montpellier, France)
Etienne Lyard
(University of Geneva)
Giovanni de Ceasare
(INAF/IASF, Bologna, Italy)
Dr
Javier Rico
(IFAE)
Johan Bregeon
(LUPM, Montpellier, France)
John E Ward
(IFAE)
Karl Kosack
(CEA Saclay)
Konrad Bernloer
(MPIK, Heidelberg, Germany)
Konstancja Satalecka
(Universidad Complutense de Madrid, Spain)
Mathieu Servillat
(LUTH, Observatoire de Paris, France)
Michele Sanguillot
(LUPM, Montpellier, France)
Ramin Marx
(MPIK, Heidelberg, Germany)
Raquel de los Reyes
(MPIK, Heidelberg, Germany)
Roland Walter
(University of Geneva)
Valentina Fioretti
(IASF, Bologna, Italy)
