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The APOLLO-Y Optical Parametric Amplifier has been developed to extend the tuning range of an ultrafast Ytterbium amplifier from the UV to the NIR. It is optimized to work with Ultrafast Systems’ spectrometers – Helios, Eos, Halcyone, etc. High stability and high efficiency are achieved through three-step amplification of a white-light supercontinuum, and all nonlinear crystal tuning, optical delay compensation, and wavelength separation is fully computer controlled.
The APOLLO-Y Optical Parametric Amplifier has been developed to extend the tuning range of an ultrafast Ytterbium amplifier from the UV to the NIR. It is optimized to work with Ultrafast Systems’ spectrometers – Helios, Eos, Halcyone, etc. High stability and high efficiency are achieved through three-step amplification of a white-light supercontinuum, and all nonlinear crystal tuning, optical delay compensation, and wavelength separation is fully computer controlled.
| Max. pulse energy | 500 µJ |
|---|---|
| Max. average output power | 6 W and 10 W |
| Pulse duration | < 290 fs |
| Center wavelength | 1040 ± 10 nm (fixed) |
| Repetition rate (user adjustable) | Single shot – 200 kHz |
| Power stability | < 0.5 % rms over 48 h |
| Polarization | Linear, vertical |
| Beam quality | TEM00, M² < 1.3 |
| Beam ellipticity | < 0.2 |
| Beam pointing stability | < 25 µrad/°C |
Our friendly team is here to help.
info@trokutsolutions.com
Our friendly team is here to help.
(+91) (022) 40124404
