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Active Galactic Nuc...
Active Galactic Nuclei population studies with the Cherenkov Telescope Array
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- Brown, Anthony M. (författare)
- Durham University
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- Acharyya, Atreya (författare)
- Durham University
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- Dominguez, Alberto (författare)
- Complutense University of Madrid
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- Hassan, Tarek (författare)
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT)
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- Lenain, Jean-Philippe (författare)
- Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE)
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- Pita, Santiago (författare)
- Université Paris Cité
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- Abdalla, H. (författare)
- North-West University
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- Carlile, C. (författare)
- Lund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science
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- Dravins, D. (författare)
- Lund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science
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- Zmija, A. (författare)
- Friedrich-Alexander University Erlangen-Nürnberg
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(creator_code:org_t)
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- Trieste, Italy : Sissa Medialab, 2022
- 2022
- Engelska.
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Ingår i: 37th International Cosmic Ray Conference (ICRC2021) - GAI - Gamma Ray Indirect. - Trieste, Italy : Sissa Medialab. - 1824-8039. ; 395
- Relaterad länk:
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http://dx.doi.org/10... (free)
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https://pos.sissa.it...
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https://lup.lub.lu.s...
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https://doi.org/10.2...
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Abstract
Ämnesord
Stäng
- The Cherenkov Telescope Array (CTA) observatory is the next generation of ground-based imaging atmospheric Cherenkov telescopes (IACTs). Building on the strengths of current IACTs, CTA is designed to achieve an order of magnitude improvement in sensitivity, with unprecedented angular and energy resolution. CTA will also increase the energy reach of IACTs, observing photons in the energy range from 20 GeV to beyond 100 TeV. These advances in performance will see CTA heralding in a new era for high-energy astrophysics, with the emphasis shifting from source discovery, to population studies and precision measurements. In this talk we discuss CTA’s ability to conduct source population studies of γ-ray bright active galactic nuclei and how this ability will enhance our understanding on the redshift evolution of this dominant γ-ray source class. © Copyright owned by the author(s) under the terms of the Creative Commons.
Ämnesord
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
Nyckelord
- Active Galactic Nuclei
- Astrophysics
- Cosmic rays
- Germanium compounds
- Telescopes
- Tellurium compounds
- Active galactic nuclei
- Angular resolution
- Cherenkov telescope arrays
- Current imaging
- Energy
- Energy resolutions
- Ground based
- Imaging atmospheric Cherenkov telescopes
- Orders of magnitude
- Population studies
- Gamma rays
Publikations- och innehållstyp
- kon (ämneskategori)
- ref (ämneskategori)
Hitta via bibliotek
Till lärosätets databas
- Av författaren/redakt...
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Brown, Anthony M ...
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Acharyya, Atreya
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Dominguez, Alber ...
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Hassan, Tarek
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Lenain, Jean-Phi ...
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Pita, Santiago
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visa fler...
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Abdalla, H.
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Carlile, C.
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Dravins, D.
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Zmija, A.
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visa färre...
- Om ämnet
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- NATURVETENSKAP
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NATURVETENSKAP
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och Fysik
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och Astronomi astrof ...
- Artiklar i publikationen
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37th Internation ...
- Av lärosätet
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Lunds universitet