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Published in 2018 at "Journal of Astrophysics and Astronomy"
DOI: 10.1007/s12036-017-9502-5
Abstract: Precise measurement of the coronal properties of Active Galactic Nuclei (AGN) requires the availability of high signal-to-noise ratio data covering a wide range of X-ray energies. The Nuclear Spectroscopic Telescope Array (NuSTAR) which is highly…
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Keywords:
measurement coronal;
coronal properties;
seyfert galaxies;
ray spectrum ... See more keywords