Introducing the CTA concept
By B. Acharya, M. Actis, T. Aghajani, G. Agnetta, J. Aguilar, F. Aharonian, M. Ajello, A. Akhperjanian, M. Alcubierre, J. Aleksic and 965 more. 2013
645 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/9810716cac84800cbfce3a7a45da35a030af03b6
How researchers see this paper
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In Astronomy and Astrophysics
- E. Orlando
- Anna Franckowiak
- Troy A. Porter
- J. Hinton
- W. Hofmann
- J. Biteau
- David A. Williams
- M. Raidal
In Nuclear and High Energy Physics
- J. Biteau
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- Anna Franckowiak
- E. Orlando
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- G. Arcadi
- Troy A. Porter
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Citations in the corpus
- Dark Matter through the Higgs portal (2019, background): “This can be done using earth based telescopes such as HESS [264, 265] and CTA [266, 267], or space detectors such as AMS [268] and Fermi–LAT [269].”
- The extragalactic background light revisited and the cosmic photon–photon opacity (Corrigendum) (2017, background): “Ultimately, the Cherenkov Telescope Array (CTA) will offer vast, factor 10 sensitivity improvement compared to current instrumentation over a very wide energy range (Acharya et al. 2013).”
- The population of TeV pulsar wind nebulae in the H.E.S.S. Galactic Plane Survey (2017, methodology): “On the analysis side, it would be beneficial to (i) improve the angular resolution and get to smaller scales of extension, (ii) find ways to reliably disentangle overlapping sources and their spectra, and (iii) aim for detecting objects larger than the IACT camera FOV.”
- 2FHL: THE SECOND CATALOG OF HARD FERMI-LAT SOURCES (2015, background): “With a factor of 10 improvement in sensitivity and the extension to energies below 100 GeV, all 2FHL sources should be detectable by the future Cherenkov Telescope Array (Acharya et al. 2013).”
- 3FHL: The Third Catalog of Hard Fermi-LAT Sources (2017, background): “Given that the Cherenkov Telescope Array (CTA) is expected to have an energy threshold below 50 GeV (Acharya et al. 2013), the 3FHL catalog offers an excellent opportunity to relate observations from space and those that will be possible in the near future from the ground.”
- THE EXTRAGALACTIC BACKGROUND LIGHT, THE HUBBLE CONSTANT, AND ANOMALIES: CONCLUSIONS FROM 20 YEARS OF TeV GAMMA-RAY OBSERVATIONS (2015, background): “The combination of next-generation local constraints with the tremendous gamma-ray sensitivity of the Chenrekov Telescope Array (CTA, Acharya et al. 2013) above 30 GeV could significantly refine the binning of the EBL spectrum.”
- The 2HWC HAWC Observatory Gamma-Ray Catalog (2017, neutral): “The next generation of observatories, including LHAASO (Sciascio 2016) and CTA (Acharya et al. 2013), should allow the TeV sky to be surveyed with greater sensitivity.”