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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.

 
GALAXIES
Superconductivity and nickelates
 
 

Cuprates (copper oxides) are currently used as highest temperature (-135° C) superconductors. Scientists are trying to find new candidates for which this temperature would be even higher. This involves understanding in detail the electronic mechanisms involved between the elements composing the superconductor. [Full story]


 
 
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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 | Staff | Partners

Beamline News

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

Research News

All the scientific news on the beamline
 
Highlights | Workshops

User guide

Everything you need to know about the beamline use and performances
 
Overview | References

 Beamline scientific articles
 

Other News

Characterization of the electronic properties of a functionalized oxides interface

Good reasons for using hard X-ray photoemission spectroscopy

July 2011: First XAS spectra

April 2011: First monochromatic beam

July 2010: First beam

Delivery of the RIXS spectro

Start of construction

All beamline news


Preliminary Project

Beamline description 

 Download diagram
of the energy ranges

Poster

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