X-ray detector boards with integrator/multiplexer ASIC

Product catalog summary

General Characteristics:
X-Card models are available with varying pixel configurations and sizes, including 0.2-256G, 0.4-128G, 0.8-64G, 0.8-128G, and 1.5-64G. Each model has specific pixel dimensions and active area lengths, with pixel pitches ranging from 0.2 mm to 1.5 mm.

Specifications:

Detectable Energy Range: 20-160 keV (with an alternative scintillator material, CdWO4, the range extends to 100-450 keV).
Scintillator: GOS with a thickness of 0.3 mm.
Minimum Integration Time: 0.2 ms.
Maximum Read Out Rate: 1 MHz.
Dynamic Range: Greater than 4,000 (defined as the saturation signal level divided by the RMS noise in darkness).
Linearity: Less than 1% non-linearity.
Operational Voltage: +5 V DC.

Dimensions:

Outline dimensions vary by model, with lengths ranging from 51.3 mm to 102.5 mm, widths from 29 mm to 40 mm, and heights consistently at 5 mm or 7.9 mm.

Additional Notes:

CdWO4 is available as an alternative scintillator material, affecting the detectable energy range.

Contact Information:
Detection Technology, Inc., Piisilta 1, 91100 Ii, Finland. Tel: +358 8 553 6600, Fax: +358 8 553 6611, Website: www.deetee.com, Email: [email protected].

Catalog excerpts

X-ray detector boards with integrator/multiplexer ASIC-1

X-Card 0.2-256G 0.4-128G 0.8-64G 0.8-128G 1.5-64G X-ray detector boards with integrator/multiplexer ASIC general characteristics i i X-Card 0.2-256G Detectable Energy Range Scintillator Thickness Active Area Length Pixel Pitch Pixel Height Pixel Width Dynamic Range (@1pf feedback capacity) Linearity (Non-Linearity) Operational Voltage Outline Dimensions (length x width x height mm) Note 1) CdWO4 is also available as scintillator material. With CdWO4 the detectable energy range is 100 - 450 keV Detection Technology, Inc. | Piisilta 1, 91100 Ii, FINLAND | Tel. +358 8 553 6600 | Fax +358 8 553 6611 | http://www.deetee.com | [email protected] Note 2) Dynamic Range is defined as the saturation signal level divided by the rms noise in darkness

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