用于忒修斯和其他任务机会的X/伽马射线成像光谱仪(XGIS)

L. Amati, C. Labanti, S. Mereghetti, F. Frontera, R. Campana, N. Auricchio, G. Baldazzi, P. Bellutti, G. Bertuccio, M. Branchesi, R. C. Butler, M. Caballero-Garcia, A. Camisasca, A. Castro-Tirado, L. Cavazzini, R. Ciolfi, A. De Rosa, F. Evangelisti, R. Farinelli, L. Ferro, F. Ficorella, M. Fiorini, F. Fuschino, J. Gasent-Blesa, G. Ghirlanda, M. Grassi, C. Guidorzi, P. Hedderman, I. Kuvvetli, G. La Rosa, P. Lorenzi, P. Malcovati, E. Marchesini, M. Marisaldi, M. Melchiorri, F. Mele, Malgorzata Mikhalska, M. Orlandini, P. Orleanski, S. Pedersen, R. Piazzolla, A. Rachevski, I. Rashevskaya, P. Rosati, V. Reglero, S. Ronchini, A. Santangelo, R. Salvaterra, P. Sarra, F. Sortino, G. Sottile, G. Stratta, S. Squerzanti, J. Stephen, C. Tenzer, L. Terenzi, A. Trois, A. Vacchi, E. Virgilli, A. Volpe, M. Winkler, G. Zampa, N. Zampa, A. Zdziarski
{"title":"用于忒修斯和其他任务机会的X/伽马射线成像光谱仪(XGIS)","authors":"L. Amati, C. Labanti, S. Mereghetti, F. Frontera, R. Campana, N. Auricchio, G. Baldazzi, P. Bellutti, G. Bertuccio, M. Branchesi, R. C. Butler, M. Caballero-Garcia, A. Camisasca, A. Castro-Tirado, L. Cavazzini, R. Ciolfi, A. De Rosa, F. Evangelisti, R. Farinelli, L. Ferro, F. Ficorella, M. Fiorini, F. Fuschino, J. Gasent-Blesa, G. Ghirlanda, M. Grassi, C. Guidorzi, P. Hedderman, I. Kuvvetli, G. La Rosa, P. Lorenzi, P. Malcovati, E. Marchesini, M. Marisaldi, M. Melchiorri, F. Mele, Malgorzata Mikhalska, M. Orlandini, P. Orleanski, S. Pedersen, R. Piazzolla, A. Rachevski, I. Rashevskaya, P. Rosati, V. Reglero, S. Ronchini, A. Santangelo, R. Salvaterra, P. Sarra, F. Sortino, G. Sottile, G. Stratta, S. Squerzanti, J. Stephen, C. Tenzer, L. Terenzi, A. Trois, A. Vacchi, E. Virgilli, A. Volpe, M. Winkler, G. Zampa, N. Zampa, A. Zdziarski","doi":"10.1117/12.2630178","DOIUrl":null,"url":null,"abstract":"We describe the science case, design and expected performances of the X/Gamma-ray Imaging Spectrometer (XGIS), a GRB and transients monitor developed and studied for the THESEUS mission project, capable of covering an exceptionally wide energy band (2 keV – 10 MeV), with imaging capabilities and location accuracy <15 arcmin up to 150 keV over a Field of View of 2sr, a few hundreds eV energy resolution in the X-ray band (<30 keV) and few micro seconds time resolution over the whole energy band. Thanks to a design based on a modular approach, the XGIS can be easily re-scaled and adapted for fitting the available resources and specific scientific objectives of future high-energy astrophysics missions, and especially those aimed at fully exploiting GRBs and high-energy transients for multi-messenger astrophysics and fundamental physics.","PeriodicalId":137463,"journal":{"name":"Astronomical Telescopes + Instrumentation","volume":"12 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2022-08-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":"{\"title\":\"The X/Gamma-ray Imaging Spectrometer (XGIS) for THESEUS and other mission opportunities\",\"authors\":\"L. Amati, C. Labanti, S. Mereghetti, F. Frontera, R. Campana, N. Auricchio, G. Baldazzi, P. Bellutti, G. Bertuccio, M. Branchesi, R. C. Butler, M. Caballero-Garcia, A. Camisasca, A. Castro-Tirado, L. Cavazzini, R. Ciolfi, A. De Rosa, F. Evangelisti, R. Farinelli, L. Ferro, F. Ficorella, M. Fiorini, F. Fuschino, J. Gasent-Blesa, G. Ghirlanda, M. Grassi, C. Guidorzi, P. Hedderman, I. Kuvvetli, G. La Rosa, P. Lorenzi, P. Malcovati, E. Marchesini, M. Marisaldi, M. Melchiorri, F. Mele, Malgorzata Mikhalska, M. Orlandini, P. Orleanski, S. Pedersen, R. Piazzolla, A. Rachevski, I. Rashevskaya, P. Rosati, V. Reglero, S. Ronchini, A. Santangelo, R. Salvaterra, P. Sarra, F. Sortino, G. Sottile, G. Stratta, S. Squerzanti, J. Stephen, C. Tenzer, L. Terenzi, A. Trois, A. Vacchi, E. Virgilli, A. Volpe, M. Winkler, G. Zampa, N. Zampa, A. Zdziarski\",\"doi\":\"10.1117/12.2630178\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We describe the science case, design and expected performances of the X/Gamma-ray Imaging Spectrometer (XGIS), a GRB and transients monitor developed and studied for the THESEUS mission project, capable of covering an exceptionally wide energy band (2 keV – 10 MeV), with imaging capabilities and location accuracy <15 arcmin up to 150 keV over a Field of View of 2sr, a few hundreds eV energy resolution in the X-ray band (<30 keV) and few micro seconds time resolution over the whole energy band. Thanks to a design based on a modular approach, the XGIS can be easily re-scaled and adapted for fitting the available resources and specific scientific objectives of future high-energy astrophysics missions, and especially those aimed at fully exploiting GRBs and high-energy transients for multi-messenger astrophysics and fundamental physics.\",\"PeriodicalId\":137463,\"journal\":{\"name\":\"Astronomical Telescopes + Instrumentation\",\"volume\":\"12 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2022-08-31\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"2\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Astronomical Telescopes + Instrumentation\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1117/12.2630178\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomical Telescopes + Instrumentation","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1117/12.2630178","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 2

摘要

我们描述科学的情况下,设计和预期性能的X /伽马射线成像光谱仪(图诚科技),伽马线暴和瞬态监测忒修斯任务项目的开发和研究,能够覆盖异常宽能带(2凯文- 10兆电子伏),与成像功能和定位精度< 15弧分150 keV的视野2 sr,几百电动汽车能量分辨率X射线波段(< 30 keV)和几个微秒时间分辨率在整个能带。由于基于模块化方法的设计,XGIS可以很容易地重新缩放和调整,以适应未来高能天体物理任务的可用资源和特定科学目标,特别是那些旨在充分利用grb和高能瞬变的多信使天体物理和基础物理。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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
The X/Gamma-ray Imaging Spectrometer (XGIS) for THESEUS and other mission opportunities
We describe the science case, design and expected performances of the X/Gamma-ray Imaging Spectrometer (XGIS), a GRB and transients monitor developed and studied for the THESEUS mission project, capable of covering an exceptionally wide energy band (2 keV – 10 MeV), with imaging capabilities and location accuracy <15 arcmin up to 150 keV over a Field of View of 2sr, a few hundreds eV energy resolution in the X-ray band (<30 keV) and few micro seconds time resolution over the whole energy band. Thanks to a design based on a modular approach, the XGIS can be easily re-scaled and adapted for fitting the available resources and specific scientific objectives of future high-energy astrophysics missions, and especially those aimed at fully exploiting GRBs and high-energy transients for multi-messenger astrophysics and fundamental physics.
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
期刊最新文献
MARVEL: optical fiber link Development of a laser projection system for the ELT Commissioning a laser metrology truss for active optics on the Large Binocular Telescope SMATT, a tool that measures the mechanical loads on the support points of the TMT primary mirror supports Enhanced X-ray Timing and Polarimetry mission: eXTP: an update on its scientific cases, mission profile and development status
×
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