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GALAXIES beamline
Research Contents > Beamlines > GALAXIES: IXS - HAXPES

The GALAXIES beamline is dedicated to inelastic x-ray scattering (IXS) and hard x-ray photoemission (HAXPES). These spectroscopic techniques are powerful probes to characterize the electronic properties of materials. The beamline is optimized to operate in the 2.3 et 12 keV energy range with high resolution and micro beam.

 
Workshop High-Pressure SOLEIL 2012  
  Le Workshop HP-SOLEIL 2012 "High Pressure Studies using Synchrotron Radiation: Present and Future" will be held at SOLEIL on January 16-17 2012 as a satellite of the next users meeting.
  		 
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First absorption spectrum obtained on the GALAXIES beamline  
  The first absorption spectrum has been measured at the Pt L3-edge on a Pt foil using an ionization chamber located after the premonochromator (DCM). These first results prefigure of the beamline quality in terms of flux and resolution.
  		 
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Beamline description

GALAXIES is an undulator beamline dedicated to hard x-ray spectroscopy. The main experimental techniques are:
- Inelastic x-ray scattering (IXS)
- Hard x-ray photoemission spectroscopy (HAXPES)
 
Technical data | Scientific opportinities | Contacts
Beamline News

All the news from the GALAXIES beamline installation, commissioning.
 
Commissioning | Installation
Research News

All the scientific news on the beamline
 
Highlights | Workshops

 Beamline scientific articles
 

Other News

April 2011: First monochromatic beam

July 2010: First beam

Delivery of the RIXS spectro

Start of construction

Preliminary Project

Notice

 Download diagram
of the energy ranges

Poster

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