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High-Precision Determination of Oxygen Kα Transition Energy Excludes Incongruent Motion of Interstellar Oxygen
- Leutenegger, MA;
- Kühn, S;
- Micke, P;
- Steinbrügge, R;
- Stierhof, J;
- Shah, C;
- Hell, N;
- Bissinger, M;
- Hirsch, M;
- Ballhausen, R;
- Lang, M;
- Gräfe, C;
- Wipf, S;
- Cumbee, R;
- Betancourt-Martinez, GL;
- Park, S;
- Yerokhin, VA;
- Surzhykov, A;
- Stolte, WC;
- Niskanen, J;
- Chung, M;
- Porter, FS;
- Stöhlker, T;
- Pfeifer, T;
- Wilms, J;
- Brown, GV;
- López-Urrutia, JR Crespo;
- Bernitt, S
- et al.
Published Web Location
https://doi.org/10.1103/physrevlett.125.243001Abstract
We demonstrate a widely applicable technique to absolutely calibrate the energy scale of x-ray spectra with experimentally well-known and accurately calculable transitions of highly charged ions, allowing us to measure the K-shell Rydberg spectrum of molecular O_{2} with 8 meV uncertainty. We reveal a systematic ∼450 meV shift from previous literature values, and settle an extraordinary discrepancy between astrophysical and laboratory measurements of neutral atomic oxygen, the latter being calibrated against the aforementioned O_{2} literature values. Because of the widespread use of such, now deprecated, references, our method impacts on many branches of x-ray absorption spectroscopy. Moreover, it potentially reduces absolute uncertainties there to below the meV level.
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