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@INBOOK{Bhler:434497,
author = {Bühler, Rolf and Dravins, D. and Egberts, K. and Hinton,
J. A. and Parsons, R. D.},
title = {{C}apabilities beyond {G}amma {R}ays},
address = {Hackensack},
publisher = {WORLD SCIENTIFIC},
reportid = {PUBDB-2020-00090},
isbn = {9789813270084},
series = {1712966},
pages = {291-299},
year = {2019},
note = {Includes bibliographical references},
comment = {Science with the Cherenkov Telescope Array},
booktitle = {Science with the Cherenkov Telescope
Array},
abstract = {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.},
keywords = {Cherenkov Telescope Array (INSPIRE) / gamma ray (INSPIRE) /
interferometer (INSPIRE) / optical (INSPIRE) / angular
resolution (INSPIRE) / cosmic radiation (INSPIRE) / lunar
(INSPIRE) / observatory (INSPIRE)},
cin = {ZEU-CTA},
cid = {I:(DE-H253)ZEU-CTA-20120731},
pnm = {613 - Matter and Radiation from the Universe (POF3-613)},
pid = {G:(DE-HGF)POF3-613},
experiment = {EXP:(DE-H253)CTA-20150101},
typ = {PUB:(DE-HGF)7},
doi = {10.1142/9789813270091_0014},
url = {https://bib-pubdb1.desy.de/record/434497},
}