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PHEMTO: the polarimetric high energy modular telescope observatory
Experimental Astronomy ( IF 2.7 ) Pub Date : 2021-04-27 , DOI: 10.1007/s10686-021-09723-x
P. Laurent , F. Acero , V. Beckmann , S. Brandt , F. Cangemi , M. Civitani , M. Clavel , A. Coleiro , R. Curado , P. Ferrando , C. Ferrigno , F. Frontera , F. Gastaldello , D. Götz , C. Gouiffès , V. Grinberg , L. Hanlon , D. Hartmann , P. Maggi , F. Marin , A. Meuris , T. Okajima , G. Pareschi , G. W. Pratt , N. Rea , J. Rodriguez , M. Rossetti , D. Spiga , E. Virgilli , S. Zane

Based upon dual focusing techniques, the Polarimetric High-Energy Modular Telescope Observatory (PHEMTO) is designed to have performance several orders of magnitude better than the present hard X-ray instruments, in the 1–600 keV energy range. This, together with its angular resolution of around one arcsecond, and its sensitive polarimetry measurement capability, will give PHEMTO the improvements in scientific performance needed for a mission in the 2050 era in order to study AGN, galactic black holes, neutrons stars, and supernovae. In addition, its high performance will enable the study of the non-thermal processes in galaxy clusters with an unprecedented accuracy.



中文翻译:

PHEMTO:偏振高能模块化望远镜天文台

基于双聚焦技术,极化高能模块化望远镜天文台(PHEMTO)在1–600 keV能量范围内的性能比目前的硬X射线仪器好几个数量级。加上约1弧秒的角分辨率和灵敏的偏振测量功能,PHEMTO可以改善2050年代任务所需的科学性能,以便研究AGN,银河黑洞,中子星和超新星。 。此外,它的高性能将使人们能够以前所未有的精度研究星系团中的非热过程。

更新日期:2021-04-28
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