2018
DOI: 10.1080/08940886.2018.1483648
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HAXPES for Materials Science at the GALAXIES Beamline

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Cited by 19 publications
(16 citation statements)
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“…The SW-HAXPES measurements were performed at the beamline GALAXIES of SOLEIL. The details of this beamline can be found elsewhere [35,36]. The measurement was carried out at an excitation energy of 3000 eV and at room temperature.…”
Section: Resultsmentioning
confidence: 99%
“…The SW-HAXPES measurements were performed at the beamline GALAXIES of SOLEIL. The details of this beamline can be found elsewhere [35,36]. The measurement was carried out at an excitation energy of 3000 eV and at room temperature.…”
Section: Resultsmentioning
confidence: 99%
“…These have included the emergence of hard X-ray photoelectron spectroscopy (HAXPES). A variety of new HAXPES beamlines [113,114,115,116] have been constructed as new light sources are brought online, enabling XPS studies that are not limited by the surface sensitivity of lab sources. Performing XPS studies with X-ray photon energies >2 keV provides more bulk sensitivity and enables access to transition metal 1s core levels that cannot be examined in a conventional Al K α laboratory source.…”
Section: Future Directions For In Situ and Related Studiesmentioning
confidence: 99%
“…To maximize the overall photoelectron yield in HAXPES, quasi-normal emission detection is typically coupled with X-ray grazing incidence (α ≤ 5 • ) [44][45][46][47]. This has the advantage of minimizing the secondary (inelastic) electron background [46]; 5.…”
Section: Optimization Of the Ap-haxpes Experimental Conditionsmentioning
confidence: 99%