Extragalactic source population studies at very high energies in the Cherenkov Telescope Array era

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F18%3A00552990" target="_blank" >RIV/68378271:_____/18:00552990 - isvavai.cz</a>

Result on the web

<a href="https://pos.sissa.it/301/632/pdf" target="_blank" >https://pos.sissa.it/301/632/pdf</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.22323/1.301.0632" target="_blank" >10.22323/1.301.0632</a>

Result language

angličtina

Original language name

Extragalactic source population studies at very high energies in the Cherenkov Telescope Array era

Original language description

The Cherenkov Telescope Array (CTA) is the next generation ground-based γ-ray observatory. It will provide an order of magnitude better sensitivity and an extended energy coverage, 20 GeV--300 TeV, relative to current Imaging Atmospheric Cherenkov Telescopes (IACTs). IACTs, despite featuring an excellent sensitivity, are characterized by a limited field of view that makes the blind search of new sources very time inefficient. Fortunately, the Fermi-LAT collaboration recently released a new catalog of 1,556 sources detected in the 10 GeV -- 2 TeV range by the Large Area Telescope (LAT) in the first 7 years of its operation (the 3FHL catalog).n

Czech name

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Czech description

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Type

D - Article in proceedings

CEP classification

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OECD FORD branch

10303 - Particles and field physics

Project

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Continuities

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Publication year

2018

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection

Proceedings of Science

ISBN

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ISSN

1824-8039

e-ISSN

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Number of pages

8

Pages from-to

1-8

Publisher name

Sissa Medilab srl

Place of publication

Trieste

Event location

Busan

Event date

Jul 10, 2017

Type of event by nationality

WRD - Celosvětová akce

UT code for WoS article

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