Low energy performance boost through a hardware stereoscopic trigger between CTA LST1 and MAGIC

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F24%3A00598924" target="_blank" >RIV/67985815:_____/24:00598924 - isvavai.cz</a>
Alternative codes found
RIV/68378271:_____/24:00598924 RIV/61989592:15310/24:73629082
Result on the web
<a href="https://pos.sissa.it/444/700/pdf" target="_blank" >https://pos.sissa.it/444/700/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.444.0700" target="_blank" >10.22323/1.444.0700</a>

Result language
angličtina
Original language name
Low energy performance boost through a hardware stereoscopic trigger between CTA LST1 and MAGIC
Original language description
The next generation facility for gamma-ray ground-based observations is the Cherenkov Telescope Array (CTA) observatory, which comprises three types of imaging atmospheric Cherenkov telescopes (IACTs). The Large-Sized Telescopes (LSTs) of CTA are the largest telescope type with a mirror dish of 23 m diameter. They cover the low energy end of the accessible gamma-ray energies for IACTs, starting from about 20 GeV up to a few TeV. The first LST prototype, known as LST-1, was officially inaugurated at the Observatorio del Roque de Los Muchachos in La Palma (Canary Islands, Spain) in 2018 and has since performed calibration observations of various known gamma-ray sources. Additionally, the site houses the MAGIC telescopes, two 17 m IACTs situated approximately 100 m away from LST-1, which have been performing stereo observations since 2009.
Czech name
—
Czech description
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Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2024
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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