A new benchmark of soft X-ray transition energies of Ne, CO$_2$, and SF$_6$: paving a pathway towards ppm accuracy
J. Stierhof (1), S. K\"uhn (2), M. Winter (3,4), P. Micke (5), R., Steinbr\"ugge (6), C. Shah (7,2,8), N. Hell (8), M. Bissinger (1), M. Hirsch, (1), R. Ballhausen (1), M. Lang (1), C. Gr\"afe (1), S. Wipf (9), R. Cumbee, (7,10), G. L. Betancourt-Martinez (11), S. Park (12)

TL;DR
This study establishes a high-precision benchmark for soft X-ray transition energies in Ne, CO$_2$, and SF$_6$, aiming to achieve ppm accuracy for spectral interpretation by combining experimental measurements with ab initio calculations.
Contribution
It introduces a novel calibration approach for X-ray transition energies that improves accuracy and discusses the limitations and potential of reaching 1-10 meV uncertainty levels.
Findings
CO$_2$ results align with previous data
SF$_6$ spectrum shifted by ~0.5 eV from earlier results
Ne results differ significantly from past measurements
Abstract
A key requirement for the correct interpretation of high-resolution X-ray spectra is that transition energies are known with high accuracy and precision. We investigate the K-shell features of Ne, CO, and SF gases, by measuring their photo ion-yield spectra at the BESSY II synchrotron facility simultaneously with the 1s-np fluorescence emission of He-like ions produced in the Polar-X EBIT. Accurate ab initio calculations of transitions in these ions provide the basis of the calibration. While the CO result agrees well with previous measurements, the SF spectrum appears shifted by ~0.5 eV, about twice the uncertainty of the earlier results. Our result for Ne shows a large departure from earlier results, but may suffer from larger systematic effects than our other measurements. The molecular spectra agree well with our results of time-dependent density functional theory.…
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