Initial ground calibration of the Resolve detector system on XRISM

F. Porter, M. Eckart, M. Leutenegger, Tomomi Watanabe, C. Kilbourne, R. Kelley, Michael C. Witthoeft, R. Cumbee, M. Sawada, N. Hell, G. Brown, Y. Ishisaki, S. Yamada
{"title":"Initial ground calibration of the Resolve detector system on XRISM","authors":"F. Porter, M. Eckart, M. Leutenegger, Tomomi Watanabe, C. Kilbourne, R. Kelley, Michael C. Witthoeft, R. Cumbee, M. Sawada, N. Hell, G. Brown, Y. Ishisaki, S. Yamada","doi":"10.1117/12.2561477","DOIUrl":null,"url":null,"abstract":"The Resolve detector system is calibrated on the ground in three stages: at the focal plane assembly, at the calorimeter spectrometer insert, and at the full instrument level. We have just completed the first two stages and have measured the detailed core line shape and spectral redistribution functions, by pixel, and as a function of energy. In addition, we have measured the energy scale function that translates instrument units into spectral units, by pixel, and as a function of detector heat sink temperature. We discuss the results of the Resolve calibration program to date as well as implications for the calibration of future high resolution x-ray spectrometers.","PeriodicalId":170593,"journal":{"name":"Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray","volume":"19 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2020-12-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"3","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1117/12.2561477","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 3

Abstract

The Resolve detector system is calibrated on the ground in three stages: at the focal plane assembly, at the calorimeter spectrometer insert, and at the full instrument level. We have just completed the first two stages and have measured the detailed core line shape and spectral redistribution functions, by pixel, and as a function of energy. In addition, we have measured the energy scale function that translates instrument units into spectral units, by pixel, and as a function of detector heat sink temperature. We discuss the results of the Resolve calibration program to date as well as implications for the calibration of future high resolution x-ray spectrometers.
查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
XRISM上Resolve探测器系统的初始地面标定
Resolve探测器系统在地面上分三个阶段进行校准:焦平面组装、量热计光谱仪插入和整个仪器水平。我们刚刚完成了前两个阶段,并测量了详细的核心线形状和光谱再分布函数,按像素计算,并作为能量的函数。此外,我们还测量了能量标度函数,该函数将仪器单位转换为光谱单位,按像素计算,并作为探测器散热器温度的函数。我们讨论了Resolve校准程序到目前为止的结果以及对未来高分辨率x射线光谱仪校准的影响。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 去求助
来源期刊
自引率
0.00%
发文量
0
期刊最新文献
GrailQuest and HERMES: hunting for gravitational wave electromagnetic counterparts and probing space-time quantum foam Frontiers of astrophysics with SmallSats SUAVE, a disruptive far UV telescope designed for long lasting performances in space Frequency domain multiplexing technology of transition-edge sensors for x-ray astronomy Improving the performance and stability of ultraviolet optical coatings using atomic layer deposition
×
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
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术
文献互助 智能选刊 最新文献 互助须知 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 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1