Uncooled spectrometer for X-ray astrophysics

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21230%2F17%3A00311887" target="_blank" >RIV/68407700:21230/17:00311887 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1117/12.2265744" target="_blank" >http://dx.doi.org/10.1117/12.2265744</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1117/12.2265744" target="_blank" >10.1117/12.2265744</a>

Result language
angličtina
Original language name
Uncooled spectrometer for X-ray astrophysics
Original language description
In the field of X-ray detection for Astrophysics there are mainly two objectives; first is to create 2D images as a result of sensing radiation by detectors consisting of a pixels matrix and the second is a spectral analysis of the incident radiation. For spectral analysis, the basis is usually the principle of diffraction. This paper describes the new design of X-ray spectrometer based on Timepix detector with optics positioned in front of it. The advantage of this setup is the ability to get the image and spectrum from the same devices. With other modifications is possible to shift detection threshold into areas of soft X-ray radiation.
Czech name
—
Czech description
—

Publication year
2017
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
Proc. SPIE 10235, EUV and X-ray Optics: Synergy between Laboratory and Space V
ISBN
978-1-5106-0972-3
ISSN
0277-786X
e-ISSN
1996-756X
Number of pages
7
Pages from-to
—
Publisher name
The International Society for Optical Engineering (SPIE)
Place of publication
Bellingham WA
Event location
Praha
Event date
Apr 24, 2017
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000406801200017

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