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Hitomi Science Gallery

SXS line resolving power Abell 2029 field of view
SXS line resolving power SXS effective area
Abell 2029 field of view
Perseus Cluster Chandra (right) overlaid with the Hitomi SXS detector (yellow line) to show the location from where the Hitomi 6-7 keV spectrum was derived (left)
Figure 1 from Nature 535, 117–121 (2016) doi:10.1038/nature18627
Full array spectrum of the core of the Perseus cluster obtained by the Hitomi observatory
Figure 2 from Nature 535, 117–121 (2016) doi:10.1038/nature18627
Spectra of Fe XXV Heα, Fe XXVI Lyα and Fe XXV Heβ from the outer region
Figure 3 from Nature 535, 117–121 (2016) doi:10.1038/nature18627
The region of the Perseus Cluster observed by Hitomi
The three figures above come from “The Hitomi Collaboration,” Nature, 535, 117–121 (2016) doi:10.1038/nature18627