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The Apollo-T OPA has been developed to extend the tuning range of a kHz Ti:Sapphire amplifier from the UV to the Mid-IR. It is optimized to work with Ultrafast Systems’ spectrometers. High stability and high efficiency are achieved through two-step amplification of a white-light supercontinuum, and nonlinear crystal tuning, optical delay compensation, and wavelength separation are fully computer controlled.
The Apollo-T OPA has been developed to extend the tuning range of a kHz Ti:Sapphire amplifier from the UV to the Mid-IR. It is optimized to work with Ultrafast Systems’ spectrometers. High stability and high efficiency are achieved through two-step amplification of a white-light supercontinuum, and nonlinear crystal tuning, optical delay compensation, and wavelength separation are fully computer controlled.
| Mode | Wavelength range (nm) | Energy(ÎĽJ) at Peak* | Polarization |
|---|---|---|---|
| SH SF | 240 – 295 | > 15 | H |
| FH Signal | 300 – 400 | > 20 | V |
| FH Idler | 400 – 480 | > 10 | H |
| SF Signal | 480 – 540 | > 70 | V |
| SF Idler | 540 – 600 | > 40 | V |
| SH Signal | 600 – 800 | > 60 | H |
| SH Idler | 800 – 1150 | > 30 | V |
| Signal | 1150 – 1600 | > 120 | V |
| Idler | 1600 – 2600 | > 60 | H |
| DFG | 2400 – 10000 | > 10 | V, H |
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info@trokutsolutions.com
Our friendly team is here to help.
(+91) (022) 40124404
