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.

引用

页码：339 / 342

页数：4