X-ray detection with Micromegas with background levels below 10-6keV-1cm-2s-1

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IOP Publishing

Erişim Hakkı

info:eu-repo/semantics/openAccess

Özet

Micromegas detectors are an optimum technological choice for the detection of low energy x-rays. The low background techniques applied to these detectors yielded remarkable background reductions over the years, being the CAST experiment beneficiary of these developments. In this document we report on the latest upgrades towards further background reductions and better understanding of the detectors' response. The upgrades encompass the readout electronics, a new detector design and the implementation of a more efficient cosmic muon veto system. Background levels below 10-6keV-1cm -2s-1 have been obtained at sea level for the first time, demonstrating the feasibility of the expectations posed by IAXO, the next generation axion helioscope. Some results obtained with a set of measurements conducted in the x-ray beam of the CAST Detector Laboratory will be also presented and discussed.

Açıklama

Yıldız, Süleyman Cenk (Dogus Author)

Anahtar Kelimeler

Dark Matter Detectors, Gaseous Detectors, Micropattern Gaseous Detectors, X-ray Detectors

Kaynak

Journal of Instrumentation

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Cilt

8

Sayı

12

Künye

Aune, S., Aznar, F., Calvet, D., Dafni, T., Diago, A., Druillole, F. ... Yıldız, S. C. (2013). X-ray detection with Micromegas with background levels below 10-6keV-1cm-2s-1. Journal of Instrumentation, 8(12), 1-14. https://dx.doi.org/10.1088/1748-0221/8/12/C12042

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