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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.
Document ID
20210010804
Acquisition Source
Goddard Space Flight Center
Document Type
Accepted Manuscript (Version with final changes)
Authors
Date Acquired
March 2, 2021
Publication Date
April 30, 2021
Publication Information
Publication: Experimental Astronomy
Publisher: Springer
Volume: 51
Issue: 3
Issue Publication Date: June 1, 2021
ISSN: 0922-6435
e-ISSN: 1572-9508
Subject Category
Funding Number(s)
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
External Peer Committee
Keywords
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