ISTEQ Amplitude Grating Spectrometer (AGS) Spectrometer
The ISTEQ Amplitude Grating Spectrometer (AGS) was specially developed for studying and characterizing the emission from short pulse laser experiments.
The absolute intensity and spectral calibration allows the determination of the UV photon number emitted by laser-based XUV-VUV sources, e.g. DPP and LPP sources and high-harmonic generation from plasma surfaces or in gaseous media. The grazing incidence amplitude grating (in comparison to a free standing transmission grating) is more reliable and robust, while also providing higher sensitivity down to soft X-ray.
Key Features:
- Wide spectral range from 6 to 200nm
- High quantum efficiency CCD
- Compact design
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Spectral range |
6-200nm |
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Resolution |
λ/Δλ = 50 |
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Grazing angle |
6° |
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Slit width |
80µm (default), other slit widths available on request |
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Grating |
TGZ-2 (NT-MDT), working area 3x3mm |
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Detector options |
1. CCD line Toshiba 1304AP, 3600 elements, pixels period 8µm, sensitive part 6µm, inorganic phosphor |
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2. CCD array Hamamatsu S7030/S7031 series 1024x122 pixels, 24um period |
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3. ANDOR DX440-BN camera, 2048x512, 13.5 um period |
XUV- VUV Spectrometer AGS Datasheet | Photo | Product | Price | |
|---|---|---|---|
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