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020 _ _ |a 978-981-327-008-4
024 7 _ |a 10.1142/9789813270091_0015
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024 7 _ |a 10.3204/PUBDB-2019-04626
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037 _ _ |a PUBDB-2019-04626
041 _ _ |a English
082 _ _ |a 522.6862
100 1 _ |a Maier, Gernot
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245 _ _ |a Appendix: Simulating CTA
260 _ _ |a Singapore
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295 1 0 |a Science with the Cherenkov Telescope Array
300 _ _ |a 299 - 300
336 7 _ |a BOOK_CHAPTER
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490 0 _ |a 1712968
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500 _ _ |a Includes bibliographical references
520 _ _ |a The expectations for the scientific capabilities of CTA presented in this document are based on sensitivity and response functions derived from detailed Monte Carlo simulations of the CTA observatory. The simulations model extensive air showers initiated by high-energy (HE) primary particles (gamma rays or background cosmic-ray nuclei and electrons), the Cherenkov light production by the shower particles, and the measurement processes of imaging atmospheric Cherenkov telescopes…
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650 _ 7 |a Cherenkov counter: atmosphere
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650 _ 7 |a nucleus: cosmic radiation
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650 _ 7 |a showers: atmosphere
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650 _ 7 |a numerical calculations: Monte Carlo
|2 INSPIRE
650 _ 7 |a radiation: Cherenkov
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650 _ 7 |a Cherenkov Telescope Array
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650 _ 7 |a observatory
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650 _ 7 |a sensitivity
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650 _ 7 |a background
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650 _ 7 |a gamma ray
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650 _ 7 |a electron
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650 _ 7 |a imaging
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650 _ 7 |a air
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693 _ _ |0 EXP:(DE-H253)CTA-20150101
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773 _ _ |a 10.1142/9789813270091_0015
787 0 _ |a The CTA Consortium
|d New Jersey : World Scientific, 2019
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856 4 _ |u https://www.worldscientific.com/doi/abs/10.1142/9789813270091_0015
856 4 _ |u https://bib-pubdb1.desy.de/record/428603/files/maier-2019-appendix-simulating-cta.pdf
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910 1 _ |a Deutsches Elektronen-Synchrotron
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913 1 _ |a DE-HGF
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920 1 _ |0 I:(DE-H253)ZEU-CTA-20120731
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980 _ _ |a contb
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