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000434497 041__ $$aEnglish
000434497 1001_ $$0P:(DE-H253)PIP1018733$$aBühler, Rolf$$b0$$udesy
000434497 245__ $$aCapabilities beyond Gamma Rays
000434497 260__ $$aHackensack$$bWORLD SCIENTIFIC$$c2019
000434497 29510 $$aScience with the Cherenkov Telescope Array
000434497 300__ $$a291-299
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000434497 4900_ $$2Author$$a1712966
000434497 500__ $$aIncludes bibliographical references
000434497 520__ $$aAlthough designed as a gamma-ray observatory, CTA is a powerful tool for a range of other astrophysics and astroparticle physics. For example, CTA can make precision studies of charged cosmic rays in the energy range from ∼100 GeV up to PeV energies, and it can be used as an instrument for optical intensity interferometry, to provide unprecedented angular resolution in the optical for bright sources. Below, we briefly summarise these possibilities. Most of the topics we discuss can be explored in parallel with gamma-ray data-taking, without interfering with the major science operations of CTA. Those studies (such as intensity interferometry) which require specific observations can likely make use of bright moonlight time, thus enhancing the CTA science return without negative impact on the key science goals.
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000434497 650_7 $$2INSPIRE$$aCherenkov Telescope Array
000434497 650_7 $$2INSPIRE$$agamma ray
000434497 650_7 $$2INSPIRE$$ainterferometer
000434497 650_7 $$2INSPIRE$$aoptical
000434497 650_7 $$2INSPIRE$$aangular resolution
000434497 650_7 $$2INSPIRE$$acosmic radiation
000434497 650_7 $$2INSPIRE$$alunar
000434497 650_7 $$2INSPIRE$$aobservatory
000434497 693__ $$0EXP:(DE-H253)CTA-20150101$$5EXP:(DE-H253)CTA-20150101$$eCherenkov Telescope Array$$x0
000434497 7001_ $$aDravins, D.$$b1
000434497 7001_ $$aEgberts, K.$$b2
000434497 7001_ $$aHinton, J. A.$$b3
000434497 7001_ $$aParsons, R. D.$$b4
000434497 773__ $$a10.1142/9789813270091_0014
000434497 7870_ $$0PUBDB-2019-02494$$aThe CTA Consortium$$dNew Jersey : World Scientific, 2019$$iIsMemberOf$$tScience with the Cherenkov Telescope Array
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