Automatic mirror alignment for the medium-sized telescopes of the Cherenkov Telescope Array using the Bokeh method

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F18%3A00552616" target="_blank" >RIV/68378271:_____/18:00552616 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1117/12.2313517" target="_blank" >https://doi.org/10.1117/12.2313517</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1117/12.2313517" target="_blank" >10.1117/12.2313517</a>

Result language
angličtina
Original language name
Automatic mirror alignment for the medium-sized telescopes of the Cherenkov Telescope Array using the Bokeh method
Original language description
The Cherenkov Telescope Array (CTA) will be the next-generation ground-based detector for gamma rays with very high energies. Telescopes will be located at one site each in both the northern and southern hemisphere. The arrays will comprise, in total, more than 100 telescopes of different sizes and designs. The sensitivity of CTA in its central energy range, i.e. between approximately 100 GeV and 1 TeV, will be driven by the performance of the Medium-Sized Telescopes (MSTs). This performance crucially depends on an exact alignment of the facets of the tessellated mirror surface of each telescope. In this contribution, an automated mirror alignment procedure for MSTs is presented.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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