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Experimental verification of the HERD prototype at CERN SPS
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics.ORCID iD: 0000-0001-7011-7229
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics.ORCID iD: 0000-0002-9769-8016
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Number of Authors: 522016 (English)In: Proceedings of SPIE: SPACE TELESCOPES AND INSTRUMENTATION 2016: ULTRAVIOLET TO GAMMA RAY, SPIE - International Society for Optical Engineering, 2016Conference paper, Published paper (Refereed)
Abstract [en]

The High Energy cosmic-Radiation Detection (HERD) facility is one of several space astronomy payloads of the cosmic light house program onboard China's Space Station, which is planned for operation starting around 2020 for about 10 years. Beam test with a HERD prototype, to verify the HERD specifications and the reading out method of wavelength shifting fiber and image intensified CCD, was taken at CERN SPS in November, 2015. The prototype is composed of an array of 5∗5∗10 LYSO crystals, which is 1/40th of the scale of HERD calorimeter. Experimental results on the performances of the calorimeter are discussed.

Place, publisher, year, edition, pages
SPIE - International Society for Optical Engineering, 2016.
Keywords [en]
3d imaging, Calorimeter, Cosmic ray, Dark matter, Gamma ray, ICCD, Shower, WLSF
National Category
Accelerator Physics and Instrumentation
Identifiers
URN: urn:nbn:se:kth:diva-202109DOI: 10.1117/12.2231804ISI: 000387731500178Scopus ID: 2-s2.0-85003633069OAI: oai:DiVA.org:kth-202109DiVA, id: diva2:1075250
Conference
Conference on Space Telescopes and Instrumentation - Ultraviolet to Gamma Ray, Edinburgh, SCOTLAND, JUN 26-JUL 01, 2016
Note

QC 20170217

Available from: 2017-02-17 Created: 2017-02-17 Last updated: 2017-02-17Bibliographically approved

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Pearce, MarkRyde, Felix

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