CESAR: Cryogenic Electronics for Space Applications

被引：0

作者：

V. Revéret

X. de la Broïse

C. Fermon

M. Pannetier-Lecoeur

C. Pigot

L. Rodriguez

J.-L. Sauvageot

Y. Jin

S. Marnieros

D. Bouchier

J. Putzeys

Y. Long

C. Kiss

S. Kiraly

M. Barbera

U. Lo Cicero

P. Brown

C. Carr

B. Whiteside

机构：

[1] Laboratoire AIM,Dipartimento di Fisica e Chimica

[2] Paris-Saclay,Space & Atmospheric Physics Group, The Blackett Laboratory

[3] CEA/IRFU/SAp,undefined

[4] CNRS,undefined

[5] Université Paris Diderot,undefined

[6] CEA,undefined

[7] IRFU,undefined

[8] SEDI,undefined

[9] CEA,undefined

[10] IRAMIS/SPEC,undefined

[11] CNRS,undefined

[12] LPN,undefined

[13] CNRS,undefined

[14] CSNSM,undefined

[15] CNRS,undefined

[16] IEF,undefined

[17] IMEC,undefined

[18] Konkoly Observatory,undefined

[19] Università degli Studi di Palermo,undefined

[20] INAF - Osservatorio Astronomico di Palermo G.S. Vaiana,undefined

[21] Imperial College London,undefined

来源：

Journal of Low Temperature Physics | 2014年 / 176卷

关键词：

Cryogenic electronics; High impedance detectors; X-ray microcalorimeters; Far-infrared bolometers;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

Ultra-low temperature sensors provide unprecedented performances in X-ray and far infrared astronomy by taking advantage of physical properties of matter close to absolute zero. CESAR is an FP7 funded project started in December 2010, that gathers six European laboratories around the development of high performances cryogenic electronics. The goal of the project is to provide far-IR, X-ray and magnetic sensors with signal-processing capabilities at the heart of the detectors. We present the major steps that constitute the CESAR work, and the main results achieved so far.

引用

页码：446 / 452

页数：6

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