Microcalorimeter array development for X-ray astronomy

被引：2
|
作者：
Pigot, C [1 ]
Agnese, P
Navick, XF
Pelliciari, C
Sauvageot, JL
机构：
[1] CEA Saclay, DSM, DAPNIA, Serv Astrophys, F-91191 Gif Sur Yvette, France
[2] CEA, DTA, DOPT, LETI,LIR, Grenoble, France
[3] CEA Saclay, DSM, DAPNIA, SEDI, Gif Sur Yvette, France
来源：
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT | 2003年 / 504卷 / 1-3期
关键词：
X-ray; microcalorimeters; spectroimagery;
D O I：
10.1016/S0168-9002(03)00765-4
中图分类号：
TH7 [仪器、仪表];
学科分类号：
0804 ; 080401 ; 081102 ;
摘要：
A development of X-ray sensitive microcalorimeter arrays is presently being undertaken to provide a spectroimager of high-energy resolution which could fit the focal plane of the X-ray astronomy spatial missions of the new generation (ESLAB 1999/093/SA). The infrared-sensitive arrays which have been realized at LETI in collaboration with the SAp, for the PACS experiment on board the Herschel satellite (Proceedings of the SPIE Conference of Orlando, 5-9 April 1999, 3698-38), are taken as the basis of this development which will rely conservatively on standard technology. (C) 2003 Elsevier Science B.V. All rights reserved.
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页码：339 / 342
页数：4
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