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SUPERNOVA OPCPA | 100 W

  • highest average power OPCPA for demanding applications

  • pumped by kW-class Yb:YAG Innoslab amplifiers or thin-disk lasers

  • output power up to 100 W

  • pulse duration down to 9 fs

  • CEP stability available

  • add-ons EUV to MID-IR  
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EUV and soft X-ray science

High harmonic generation / Coherent diffractive imaging with atomic resolution / Time-resolved reaction microscopy (ARPES) / Coherent control / Attosecond streaking
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• Bioparticle imaging
• Nanoparticles
​​and clusters
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• Inspection in EUV
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• Attosecond dynamics
​in solids and gases
The Supernova OPCPA provides few-cycle, high-power pules at mid-infrared wavelengths, e.g. 2 μm, with mJ pulses for a new brilliant soft X-ray source at the Advanced Research Center for Nanolithography (ARCNL) in Amsterdam.
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Large research facilities

Pump-probe laser for material science and X-ray imaging / Photocathode laser, Seeding, heating, slicing of particle bunches / Femtosecond-synchronization to external clock (RF and Fiber Link)
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• Free-electron lasers
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• Particle accelerators
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• Laser user facilities
- Matthew K. R. Windeler et al, "100  W high-repetition-rate near-infrared optical parametric chirped pulse amplifier," Opt. Lett. 44, 4287-4290 (2019), https://www.osapublishing.org/ol/abstract.cfm?uri=ol-44-17-4287

- Katalin Mecseki et al, "High average power 88  W OPCPA system for high-repetition-rate experiments at the LCLS x-ray free-electron laser," Opt. Lett. 44, 1257-1260 (2019), https://www.osapublishing.org/ol/abstract.cfm?uri=ol-44-5-1257
The Supernova OPCPA is our award-winning flagship product with extremely short pulse durations and a high temporal contrast. Wavelength flexibility, options for multiple outputs and CEP stability allow tailoring it to custom multi-color experiments at highest average power. This allows leading scientists to push research to new limits.

The product is also available as high energy version (HE) with multimillijoule pulse energies, pumped by Yb:YAG thin-disk lasers.
 
SN-800
SN-1550
SN-2200
SN-3000
Central wavelength
800 nm
1550 nm
2200 nm
3000 nm
Tunability optional
700-950 nm
1400-1700 nm
-
-
Pulse duration (FWHM)
< 9 fs
< 35 fs
< 30 fs
< 50 fs
Average power
> 20 - 100 W
> 20 - 100 W
> 20 - 100 W
> 20 - 100 W
Pulse energy
> 1 mJ
> 1 mJ
> 1 mJ
> 1 mJ
Repetition rate
20 - 100 kHz
20 - 100 kHz
20 - 100 kHz
20 - 100 kHz
CEP stability
on request
on request
on request
on request
HHG extension
on request
on request
on request
on request
Pump Laser
300 W - 1 kW
300 W - 1 kW
300 W - 1 kW
300 W - 1 kW
Supernova HE at 1 kHz
on request
on request
on request
on request
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Long-term power stability measured with powermeter (averaged shots) over more than 5 hours: Pump laser Innoslab 300 W, 20 kHz repetition rate, Supernova OPCPA SN-800, 20.6 W average power and 0.3 % standard deviation.
Data sheet
News about ultrafast science
 News about EUX/SXR applications and technology
Any questions? You need more specifications? You want to inquire more information or get a quote?

Get in contact with us:

Submit
Download data sheet
Any questions? You need more specifications? You want to inquire more information or get a quote?

Get in contact with us:

Submit
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  • News/Events
  • Products
    • White Dwarf for 3-photon microscopy
    • White Dwarf for material science
    • White Dwarf for few-cycle pulses
    • White Dwarf HE
    • Supernova
  • Applications
    • 3-photon microscopy
    • Ultrafast science
    • EUV/SXR technology
  • Technology
  • Company
  • Contact