TES microcalorimeter development for future Japanese X-ray astronomy missions

被引:3
|
作者
Fujimoto, R
Mitsuda, K
Yamasaki, NY
Iyomoto, N
Oshima, T
Takei, Y
Futamoto, K
Ichitsubo, T
Fujimori, T
Yoshida, K
Ishisaki, Y
Morita, U
Koga, T
Shinozaki, K
Sato, K
Takai, N
Ohashi, T
Kudo, H
Sato, H
Arakawa, T
Kobayashi, H
Izumi, T
Ohtsuka, S
Mori, K
Shoji, S
Osaka, T
Homma, T
Kuroda, Y
Onishi, M
Goto, M
Beppu, F
Tanaka, T
Morooka, T
Nakayama, S
Chinone, K
机构
[1] ISAS, Sagamihara, Kanagawa 2298510, Japan
[2] Tokyo Metropolitan Univ, Tokyo 1920397, Japan
[3] Waseda Univ, Tokyo 1698555, Japan
[4] Mitsubishi Heavy Ind Co Ltd, Aichi 4858561, Japan
[5] Panason Commun Co LTD, Kumamoto 8650193, Japan
[6] Seiko Instruments Inc, Matsudo, Chiba 2702222, Japan
关键词
X-ray astronomy; microcalorimeter; transition edge sensor;
D O I
10.1016/j.nima.2003.11.356
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
We are developing a Ti/Au TES microcalorimeter array for future Japanese X-ray astronomy missions. The goal is an energy resolution of 2-5 eV at 6 keV, and an array of 100-1000 pixels to achieve a geometrical area of >1 cm(2) and a moderate spatial resolution simultaneously. The energy resolution was improved to similar to6 eV at 6 keV with a very fast time constant (<100 mus). To achieve a high coverage fraction, it is necessary to fabricate mushroom-shaped X-ray microabsorbers. We are developing an electrodeposition fabrication technique that is suitable for our process. Sn was used as absorber material, but the energy resolution was not good due to the existence of long-lived quasiparticles. Bi is also used, and the process is under optimization now. The readout strategy is to multiplex signals in the frequency domain, using a bridge circuit. So far, we succeeded in multiplexing two pixels modulated with 50 and 20 kHz at 440 mK. The energy resolution obtained at 110 mK was 33 eV (25 kHz). (C) 2003 Elsevier B.V. All rights reserved.
引用
收藏
页码:431 / 434
页数:4
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