A cryogenic imaging X-ray spectrometer for XEUS read out by frequency-division SQUID multiplexers

被引:4
作者
de Korte, PAJ [1 ]
van Baar, JJ [1 ]
Baars, NHR [1 ]
Bakker, FE [1 ]
Tiest, WMB [1 ]
Bruijn, MP [1 ]
Germeau, A [1 ]
Hoevers, HFC [1 ]
Kiviranta, M [1 ]
Krouwer, E [1 ]
van der Kuur, J [1 ]
Lubbers, MP [1 ]
Mels, WA [1 ]
Ridder, ML [1 ]
Seppae, H [1 ]
Wiegerink, RJ [1 ]
机构
[1] SRON, Natl Inst Space Res, NL-3584 CA Utrecht, Netherlands
来源
HIGH-ENERGY DETECTORS IN ASTRONOMY | 2004年 / 5501卷
关键词
cryogenic micro-calorimeters; transition-edge sensors (TES); SQUIDs; imaging X-ray spectrometer; X-ray astronomy; XEUS; frequency-domain multiplexing (FDM);
D O I
10.1117/12.552933
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
A micro-calorimeter array with superconducting transition-edge sensors read out by a SQUID-based frequency-domain multiplexer is under development for the X-ray imaging spectrometer on board ESA's X-ray Evolving Universe Spectroscopy (XEUS) mission. The XEUS requirements are 2 and 5 eV FWHM energy resolution for 2 and 7 keV X-rays, respectively. An array of 32 x 32 pixels with 250 micron square pixels is envisaged. SRON and MESA(+) have developed 5 x 5 imaging micro-calorimeter prototype arrays along a bulk micromachining and a surface micromachining route. The present state of array design and development with emphasis on pixel-to-pixel performance measurements of thermal and I-V characteristics, sensor noise and energy resolution are presented. SRON and VTT are developing frequency-domain multiplexing with SQUID current amplifiers to read out the 32 x 32 array. The concept for the frequency division multiplexing read-out will be presented and its performance characteristics discussed. Recent results of sensor operation under AC-bias (500 kHz) are presented.
引用
收藏
页码:167 / 176
页数:10
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