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MOONLANDER HHG

The Moonlander HHG is an efficient coherent EUV source for time-resolved spectroscopy such as ARPES. Driven by our high-power White Dwarf HE OPCPA, the Moonlander HHG-50 provides high photon flux at high repetition rates in a robust, reliable design.

  • 21-50 eV photon energy with optional filtering and focusing

  • full pump-probe suite available based on White Dwarf HE OPCPA
 
  • 100 kHz or more

  • designed for ARPES and CDI
Picture
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Ultrafast material science

2D Infrared spectroscopy (2DIR) / Multi-color pump-probe, Mid-IR and THz spectroscopy / Magneto-optical Kerr-effect (MOKE) microscopy / Raman spectroscopy (CARS, GAMERS)
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• Strong-field physics
• Relativistic plasma physics

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•  Cluster and gasphase dynamics
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• Carrier dynamics of
​solid materials
• Photosynthesis

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• Strong-field physics
​• Relativistic plasma physics

Time-resolved ARPES

OPCPA is a versatile tool which provides ultra-short pulses  from the UV to the mid-infrared.
Combined with our high flux, high repetition rate Moonlander HHG source, this makes OPCPA the ideal technology platform for time-resolved photoelectron spectroscopy.
Read about ARPES application

EUV and soft X-Ray science

Coherent diffractive imaging (CDI) / 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 Moonlander HHG-50 is a high flux coherent EUV source for time-resolved spectroscopy such as ARPES. Our White Dwarf HE OPCPA serves as an ultrashort driver at 400 nm or 800 nm with excellent temporal contrast and clean pulse profile to drive stable and efficiently higher harmonics. Hence, the Moonlander HHG-50 provides high photon flux at high repetition rates with long-term stable operation based on a robust, reliable design.

A second, synchronized optical output from UV to mid-IR can be provided with our White Dwarf HE OPCPA, hence offering a full pump-probe suite to take the next step in time-resolved photoelectron spectroscopy.
 
Moonlander HHG-50
Driver inclusive
White Dwarf HE OPCPA at 400 nm or 800 nm
Photon energy
21...50 eV
Wavelength
24...59 nm
Spectral bandwidth (FWHM)
ca 100 meV depending on driver
Photon flux at source
> 5x10^12 ph/sec @ 38 eV
Photon flux filtered (single-harmonic)
> 1x10^12 ph/sec @ 38 eV
Repetition rate
100 kHz, higher on request
Focusing and steering
on request
Full pump-probe suite
optionally based on White Dwarf HE OPCPA
User interface
motor control for target position and target camera, remote gas pressure control, diode for EUV flux measurement
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Normalized spectral intensity: Moonlander HHG-50 driven by White Dwarf HE OPCPA at 800 nm at 100 kHz.
Data sheet
Applications: Ultrafast science
Applications: EUV/ and soft x-ray technology
Get in contact with us about this product:
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Download data sheet
Get in contact with us about this product:
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CLASS 5 PHOTONICS GmbH
+49 40 22863165
+1   650 353 9700
info[at]class5photonics.com
Notkestr. 85 (Bldg. 200), 22607 Hamburg, Germany

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Korea - Wooyang Photonics

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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
    • Moonlander HHG
  • Applications
    • 3-photon microscopy
    • Ultrafast science
    • EUV/SXR technology
  • Technology
  • Company
  • Contact