4161. Searching for PeVatrons in the CTA Galactic Plane SurveyC. Trichard, Christopher Eckner, Gašper Kukec Mezek, Samo Stanič, Serguei Vorobiov, Lili Yang, Gabrijela Zaharijas, Danilo Zavrtanik, Marko Zavrtanik, 2017, objavljeni znanstveni prispevek na konferenci Ključne besede: Cherenkov Telescope Array, Galactic Plane Survey, cosmic PeVatrons
Objavljeno v RUNG: 16.02.2018; Ogledov: 3444; Prenosov: 133
 Celotno besedilo (629,89 KB) |
4162. Cherenkov Telescope Array: The Next Generation Gamma-ray ObservatoryRene A. Ong, Christopher Eckner, Gašper Kukec Mezek, Samo Stanič, Serguei Vorobiov, Lili Yang, Gabrijela Zaharijas, Marko Zavrtanik, Danilo Zavrtanik, 2017, objavljeni znanstveni prispevek na konferenci Opis: The Cherenkov Telescope Array (CTA) will be the next-generation gamma-ray observatory,
investigating gamma-ray and cosmic ray astrophysics at energies from 20 GeV to more than 300 TeV. The observatory, consisting of large arrays of imaging atmospheric Cherenkov telescopes in both the southern and northern hemispheres, will provide full-sky coverage and will achieve a sensitivity improved by up to an order of magnitude compared to existing instruments such as H.E.S.S., MAGIC and VERITAS. CTA is expected to discover hundreds of new TeV gammaray sources, allowing it to significantly advance our understanding of the origin of cosmic rays, to probe much larger distances in the universe, and to search for WIMP dark matter with unprecedented sensitivity in TeV mass range.
The development of CTA is being carried out by a worldwide consortium of scientists from
32 countries. Consortium scientists have developed the core scientific programme of CTA and
institutes of the Consortium are expected to provide the bulk of the CTA components. The
construction of CTA is overseen by the CTA Observatory that will in the future manage
observatory operations, the guest observer programme, and data dissemination.
This talk will review the scientific motivation for CTA, focusing on the key science projects
that form the core programme of research. The talk will outline the design of CTA, including the
science drivers, overall concept, performance optimization, and array layouts. The current
status of CTA, including sites, prototype telescope progress, and steps forward will also be
described.
Ključne besede: CTA, next-generation gamma-ray observatory, gamma rays
Objavljeno v RUNG: 16.02.2018; Ogledov: 3835; Prenosov: 140
Celotno besedilo (1,35 MB) |
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4164. EIQAS - Enhancing Internal Quality Assurance Systems : ERASMUS+ PROJECT 2014-2016 : Final methodology for identification of good practice in internal quality assurance (IQA) : Descriptions of examples of good practice in IQAVeronika Piccinini, Mieczyslaw W. Socha, Izabela Kwiatkowska-Sujka, Maciej Markowski, 2016, elaborat, predštudija, študija Ključne besede: zagotavljanje kakovosti, visoko šolstvo, evropske smernice
Objavljeno v RUNG: 14.02.2018; Ogledov: 4487; Prenosov: 314
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4167. An Indication of Anisotropy in Arrival Directions of Ultra-high-energy Cosmic Rays through Comparison to the Flux Pattern of Extragalactic Gamma-Ray SourcesA. Aab, Andrej Filipčič, Gašper Kukec Mezek, Ahmed Saleh, Samo Stanič, Marta Trini, Darko Veberič, Serguei Vorobiov, Lili Yang, Danilo Zavrtanik, Marko Zavrtanik, 2018, izvirni znanstveni članek Ključne besede: astroparticle physics, cosmic rays, active galaxies, starburst galaxies, data analysis methods
Objavljeno v RUNG: 14.02.2018; Ogledov: 3466; Prenosov: 0
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