雅典娜/X-IFU端到端演示读出链状态

Gilles Roudil, François Pajot, Florent Castellani, Sophie Beaumont, Michel Dupieux, David Murat, Yann Parot, Laurent Ravera, Joseph Adams, Simon Bandler, James Chervenak, Edoardo Cucchetti, Christophe Daniel, William Doriese, Malcolm Durking, Hervé Geoffray, Gene Hilton, Baptiste Mot, Philippe Peille, Damien Prêle, Carl Reintsema, Kazuhiro Sakai, Joel Ullom, Nicholas Wakeham, Alexei Molin
{"title":"雅典娜/X-IFU端到端演示读出链状态","authors":"Gilles Roudil, François Pajot, Florent Castellani, Sophie Beaumont, Michel Dupieux, David Murat, Yann Parot, Laurent Ravera, Joseph Adams, Simon Bandler, James Chervenak, Edoardo Cucchetti, Christophe Daniel, William Doriese, Malcolm Durking, Hervé Geoffray, Gene Hilton, Baptiste Mot, Philippe Peille, Damien Prêle, Carl Reintsema, Kazuhiro Sakai, Joel Ullom, Nicholas Wakeham, Alexei Molin","doi":"10.21203/rs.3.rs-3544860/v1","DOIUrl":null,"url":null,"abstract":"Abstract The X-ray Integral Field Unit (X-IFU) of the Athena observatory, scheduled for launch in the mid 2030's, will provide X-ray imaging spectroscopy data with unprecedented spectral and spatial resolution. The detection chain, based on a ~ 1.5 kilo-pixel array of transition edge sensors (TESs) cooled down to 55 mK, is under development by a large international collaboration. In order to perform an end-to-end demonstration of the X-IFU readout chain, a 50 mK test bench (Elsa), is being developed at IRAP in collaboration with CNES. Based on a commercial ADR cryostat, it includes a 1024-pixel TES array provided by NASA/GSFC with its associated cold readout chain provided by NIST. The validation of the performance of the system was performed using a NIST and NASA/GSFC laboratory warm readout chain. These laboratory electronics will be replaced step by step by the demonstration models of the space qualified electronics designed for the X-IFU: the digital readout electronics by IRAP and the warm front-end electronics by APC. We present here the status of the 50 mK test bench, its performance budget, and the demonstration of a prototype of a first element of the flight electronics.","PeriodicalId":500086,"journal":{"name":"Research Square (Research Square)","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2023-11-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Status of the end-to-end demonstration readout chain for Athena/X-IFU\",\"authors\":\"Gilles Roudil, François Pajot, Florent Castellani, Sophie Beaumont, Michel Dupieux, David Murat, Yann Parot, Laurent Ravera, Joseph Adams, Simon Bandler, James Chervenak, Edoardo Cucchetti, Christophe Daniel, William Doriese, Malcolm Durking, Hervé Geoffray, Gene Hilton, Baptiste Mot, Philippe Peille, Damien Prêle, Carl Reintsema, Kazuhiro Sakai, Joel Ullom, Nicholas Wakeham, Alexei Molin\",\"doi\":\"10.21203/rs.3.rs-3544860/v1\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Abstract The X-ray Integral Field Unit (X-IFU) of the Athena observatory, scheduled for launch in the mid 2030's, will provide X-ray imaging spectroscopy data with unprecedented spectral and spatial resolution. The detection chain, based on a ~ 1.5 kilo-pixel array of transition edge sensors (TESs) cooled down to 55 mK, is under development by a large international collaboration. In order to perform an end-to-end demonstration of the X-IFU readout chain, a 50 mK test bench (Elsa), is being developed at IRAP in collaboration with CNES. Based on a commercial ADR cryostat, it includes a 1024-pixel TES array provided by NASA/GSFC with its associated cold readout chain provided by NIST. The validation of the performance of the system was performed using a NIST and NASA/GSFC laboratory warm readout chain. These laboratory electronics will be replaced step by step by the demonstration models of the space qualified electronics designed for the X-IFU: the digital readout electronics by IRAP and the warm front-end electronics by APC. We present here the status of the 50 mK test bench, its performance budget, and the demonstration of a prototype of a first element of the flight electronics.\",\"PeriodicalId\":500086,\"journal\":{\"name\":\"Research Square (Research Square)\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2023-11-14\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Research Square (Research Square)\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.21203/rs.3.rs-3544860/v1\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Research Square (Research Square)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.21203/rs.3.rs-3544860/v1","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0

摘要

雅典娜天文台的x射线积分场单元(X-IFU)计划于2030年代中期发射,将提供前所未有的光谱和空间分辨率的x射线成像光谱数据。探测链,基于~ 1.5千像素的过渡边缘传感器阵列(TESs),冷却至55 mK,正在由大型国际合作开发中。为了执行X-IFU读出链的端到端演示,IRAP正在与CNES合作开发一个50 mK测试台(Elsa)。它基于商用ADR低温恒温器,包括NASA/GSFC提供的1024像素TES阵列和NIST提供的相关冷读出链。使用NIST和NASA/GSFC实验室温度读出链对系统的性能进行了验证。这些实验室电子设备将逐步被为X-IFU设计的空间合格电子设备的演示模型所取代:IRAP的数字读出电子设备和APC的热前端电子设备。我们在这里介绍了50 mK测试台的现状,它的性能预算,以及飞行电子设备第一元素的原型演示。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Status of the end-to-end demonstration readout chain for Athena/X-IFU
Abstract The X-ray Integral Field Unit (X-IFU) of the Athena observatory, scheduled for launch in the mid 2030's, will provide X-ray imaging spectroscopy data with unprecedented spectral and spatial resolution. The detection chain, based on a ~ 1.5 kilo-pixel array of transition edge sensors (TESs) cooled down to 55 mK, is under development by a large international collaboration. In order to perform an end-to-end demonstration of the X-IFU readout chain, a 50 mK test bench (Elsa), is being developed at IRAP in collaboration with CNES. Based on a commercial ADR cryostat, it includes a 1024-pixel TES array provided by NASA/GSFC with its associated cold readout chain provided by NIST. The validation of the performance of the system was performed using a NIST and NASA/GSFC laboratory warm readout chain. These laboratory electronics will be replaced step by step by the demonstration models of the space qualified electronics designed for the X-IFU: the digital readout electronics by IRAP and the warm front-end electronics by APC. We present here the status of the 50 mK test bench, its performance budget, and the demonstration of a prototype of a first element of the flight electronics.
求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
自引率
0.00%
发文量
0
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信