谷歌浏览器插件
订阅小程序
在清言上使用

STROBE-X High Energy Modular Array (HEMA)

Anthony L. Hutcheson, Marco Feroci,Andrea Argan,Matias Antonelli,Marco Barbera,Jorg Bayer, Pierluigi Bellutti,Giuseppe Bertuccio,Valter Bonvicini,Franck Cadoux, Riccardo Campana, Matteo Centis Vignali,Francesco Ceraudo,Marc Christophersen,Daniela Cirrincione, Fabio D'Anca,Nicolas De Angelis, Alessandra De Rosa,Giovanni Della Casa,Ettore Del Monte,Giuseppe Dilillo, Yuri Evangelista,Yannick Favre,Francesco Ficorella,Mauro Fiorini, Jeremy J. Ford,Marco Grassi,J. Eric Grove,Alejandro Guzman, Paul Heddermann, Merlin R. Kole, Ugo Lo Cicero,Giovanni Lombardi,Piero Malcovati,Malgorzata Michalska,Aline Meuris,Gabriele Minervini,Witold Nowosielski,Alessio Nuti, Luigi Pacciani,Giancarlo Pepponi, Steven C. Persyn,Antonino Picciotto,Samuel Pliego, Alexander Rachevski, Irina Rashevskaya, Paul S. Ray, Alina Samusenko,Andrea Santangelo, Stephane Schanne, Carl L. Schwendeman,Clio Sleator,Jacob R. Smith, Libor Sveda, Jiri Svoboda, Christoph Tenzer,Michela Todaro,Alessio Trois, Andrea Vacchi, Hao Xiong,Xianqi Wang,Xin Wu, Eric A. Wulf,Gianluigi Zampa,Nicola Zampa,Andrzej Zdziarski,Nicola Zorzi

arxiv(2024)

引用 0|浏览4
暂无评分
摘要
The High Energy Modular Array (HEMA) is one of three instruments that compose the STROBE-X mission concept. The HEMA is a large-area, high-throughput non-imaging pointed instrument based on the Large Area Detector developed as part of the LOFT mission concept. It is designed for spectral timing measurements of a broad range of sources and provides a transformative increase in sensitivity to X-rays in the energy range of 2–30 keV compared to previous instruments, with an effective area of 3.4 m^2 at 8.5 keV and an energy resolution of better than 300 eV at 6 keV in its nominal field of regard.
更多
查看译文
AI 理解论文
溯源树
样例
生成溯源树,研究论文发展脉络
Chat Paper
正在生成论文摘要