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| 001 | 434497 | ||
| 005 | 20250905212737.0 | ||
| 020 | _ | _ | |a 9789813270084 |
| 024 | 7 | _ | |a 10.1142/9789813270091_0014 |2 doi |
| 024 | 7 | _ | |a altmetric:26573755 |2 altmetric |
| 024 | 7 | _ | |a 10.3204/PUBDB-2020-00090 |2 datacite_doi |
| 024 | 7 | _ | |a openalex:W2909922504 |2 openalex |
| 037 | _ | _ | |a PUBDB-2020-00090 |
| 041 | _ | _ | |a English |
| 100 | 1 | _ | |a Bühler, Rolf |0 P:(DE-H253)PIP1018733 |b 0 |u desy |
| 245 | _ | _ | |a Capabilities beyond Gamma Rays |
| 260 | _ | _ | |a Hackensack |c 2019 |b WORLD SCIENTIFIC |
| 295 | 1 | 0 | |a Science with the Cherenkov Telescope Array |
| 300 | _ | _ | |a 291-299 |
| 336 | 7 | _ | |a BOOK_CHAPTER |2 ORCID |
| 336 | 7 | _ | |a Book Section |0 7 |2 EndNote |
| 336 | 7 | _ | |a bookPart |2 DRIVER |
| 336 | 7 | _ | |a INBOOK |2 BibTeX |
| 336 | 7 | _ | |a Output Types/Book chapter |2 DataCite |
| 336 | 7 | _ | |a Contribution to a book |b contb |m contb |0 PUB:(DE-HGF)7 |s 1757057741_2492737 |2 PUB:(DE-HGF) |
| 490 | 0 | _ | |a 1712966 |2 Author |
| 500 | _ | _ | |a Includes bibliographical references |
| 520 | _ | _ | |a Although designed as a gamma-ray observatory, CTA is a powerful tool for a range of other astrophysics and astroparticle physics. For example, CTA can make precision studies of charged cosmic rays in the energy range from ∼100 GeV up to PeV energies, and it can be used as an instrument for optical intensity interferometry, to provide unprecedented angular resolution in the optical for bright sources. Below, we briefly summarise these possibilities. Most of the topics we discuss can be explored in parallel with gamma-ray data-taking, without interfering with the major science operations of CTA. Those studies (such as intensity interferometry) which require specific observations can likely make use of bright moonlight time, thus enhancing the CTA science return without negative impact on the key science goals. |
| 536 | _ | _ | |a 613 - Matter and Radiation from the Universe (POF3-613) |0 G:(DE-HGF)POF3-613 |c POF3-613 |f POF III |x 0 |
| 588 | _ | _ | |a Dataset connected to CrossRef Book |
| 650 | _ | 7 | |a Cherenkov Telescope Array |2 INSPIRE |
| 650 | _ | 7 | |a gamma ray |2 INSPIRE |
| 650 | _ | 7 | |a interferometer |2 INSPIRE |
| 650 | _ | 7 | |a optical |2 INSPIRE |
| 650 | _ | 7 | |a angular resolution |2 INSPIRE |
| 650 | _ | 7 | |a cosmic radiation |2 INSPIRE |
| 650 | _ | 7 | |a lunar |2 INSPIRE |
| 650 | _ | 7 | |a observatory |2 INSPIRE |
| 693 | _ | _ | |0 EXP:(DE-H253)CTA-20150101 |5 EXP:(DE-H253)CTA-20150101 |e Cherenkov Telescope Array |x 0 |
| 700 | 1 | _ | |a Dravins, D. |b 1 |
| 700 | 1 | _ | |a Egberts, K. |b 2 |
| 700 | 1 | _ | |a Hinton, J. A. |b 3 |
| 700 | 1 | _ | |a Parsons, R. D. |b 4 |
| 773 | _ | _ | |a 10.1142/9789813270091_0014 |
| 787 | 0 | _ | |a The CTA Consortium |0 PUBDB-2019-02494 |t Science with the Cherenkov Telescope Array |i IsMemberOf |d New Jersey : World Scientific, 2019 |
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| 910 | 1 | _ | |a Deutsches Elektronen-Synchrotron |0 I:(DE-588b)2008985-5 |k DESY |b 0 |6 P:(DE-H253)PIP1018733 |
| 913 | 1 | _ | |a DE-HGF |b Forschungsbereich Materie |l Materie und Universum |1 G:(DE-HGF)POF3-610 |0 G:(DE-HGF)POF3-613 |3 G:(DE-HGF)POF3 |2 G:(DE-HGF)POF3-600 |4 G:(DE-HGF)POF |v Matter and Radiation from the Universe |x 0 |
| 914 | 1 | _ | |y 2019 |
| 915 | _ | _ | |a OpenAccess |0 StatID:(DE-HGF)0510 |2 StatID |
| 920 | 1 | _ | |0 I:(DE-H253)ZEU-CTA-20120731 |k ZEU-CTA |l Cherenkov Telescope Array |x 0 |
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