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Overview of Image Sensors for X-ray Astronomy

X-ray astronomy observations in the 0.5-10 keV band are typically made using a combination of X-ray imagers and Walter-type X-ray mirrors mounted on an astronomical satellite. X-ray CCDs are widely used, but a shift to active pixel sensors is expected in the future.

The International Display Workshops

Proceedings of the International Display Workshops Volume 30 (IDW '23)

Proceedings of the International Display Workshops Volume 30 (IDW '23)

[IST1-2 (Invited)]Overview of Image Sensors for X-ray Astronomy

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