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image/svg+xml Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Closed Access logo, derived from PLoS Open Access logo. This version with transparent background. http://commons.wikimedia.org/wiki/File:Closed_Access_logo_transparent.svg Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Recolector de Cienci...arrow_drop_down
image/svg+xml Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Closed Access logo, derived from PLoS Open Access logo. This version with transparent background. http://commons.wikimedia.org/wiki/File:Closed_Access_logo_transparent.svg Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao
Recolector de Ciencia Abierta, RECOLECTA
Article . 2022
Data sources: Recolector de Ciencia Abierta, RECOLECTA
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PHEMTO: the polarimetric high energy modular telescope observatory

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 2022 English Publisher:Springer Nature
Authors: Laurent, P.; Acero, F.; Beckmann, V.; Brandt, S.; Cangemi, F.; Civitani, M.; Clavel-Henry, Morane; +24 Authors

handle: 10261/261209

PHEMTO: the polarimetric high energy modular telescope observatory

Abstract

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.

Open access funding provided by Istituto Nazionale di Astrofisica within the CRUI-CARE Agreement.

Keywords

Active galactic nuclei, Clusters of galaxies, Accretion/ejection phenomena, Space mission concept, Magnetic fields, Supernovae and supernovae remnants, X-y-ray focussing telescopes, Galaxy clusters, ESA voyage 2050, Non-thermal emission

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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