Cherenkov Telescope Array (CTA) - challenges in systems engineering and project management

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F18%3A00552738" target="_blank" >RIV/68378271:_____/18:00552738 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1117/12.2317639" target="_blank" >https://doi.org/10.1117/12.2317639</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1117/12.2317639" target="_blank" >10.1117/12.2317639</a>

Result language
angličtina
Original language name
Cherenkov Telescope Array (CTA) - challenges in systems engineering and project management
Original language description
The Cherenkov Telescope Array (CTA) is the next generation ground-based observatory for gamma-ray astronomy at very high energies. With more than 100 telescopes at two sites, CTA will be the world's largest and most sensitive high-energy gamma-ray observatory covering the full sky with a northern array located at the Roque de los Muchachos astronomical observatory on the island of La Palma (Spain) and a southern array near the European Southern Observatory site at Paranal (Chile). Three classes of telescope types with imaging Cherenkov cameras, calibration, clock and timing systems, site infrastructure as well as control and data handling/processing software, developed in a large international collaboration, are required to build the CTA observatory system.n
Czech name
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Czech description
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Publication year
2018
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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