The Simbol-X view of the unresolved X-ray background
A. Comastri (1), R. Gilli (1), F. Fiore (2), C. Vignali (3,1), R., Della Ceca (4), G. Malaguti (5) ((1) INAF - Osservatorio Astronomico di, Bologna; (2) INAF - Osservatorio Astronomico di Roma; (3) Dipartimento di, Astronomia
TL;DR
This paper emphasizes the significance of high-energy X-ray observations, particularly above 10 keV, for understanding supermassive black hole emissions and the evolution of obscured active galactic nuclei.
Contribution
It highlights the potential of Simbol-X observations to advance knowledge of the unresolved X-ray background and AGN evolution.
Findings
High-energy X-ray data reveal obscured AGN populations.
Simbol-X can improve understanding of black hole emission mechanisms.
Insights into the cosmological evolution of AGNs.
Abstract
We will briefly discuss the importance of sensitive X-ray observations above 10 keV for a better understanding of the physical mechanisms associated to the Supermassive Black Hole primary emission and to the cosmological evolution of the most obscured Active Galactic Nuclei.
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Relativity and Gravitational Theory · Experimental and Theoretical Physics Studies