A Reassessment of Absolute Energies of the X-ray L Lines of Lanthanide Metals
arXiv:1702.00507 · doi:10.1088/1681-7575/aa722f
Abstract
We introduce a new technique for determining x-ray fluorescence line energies and widths, and we present measurements made with this technique of 22 x-ray L lines from lanthanide-series elements. The technique uses arrays of transition-edge sensors, microcalorimeters with high energy-resolving power that simultaneously observe both calibrated x-ray standards and the x-ray emission lines under study. The uncertainty in absolute line energies is generally less than 0.4 eV in the energy range of 4.5 keV to 7.5 keV. Of the seventeen line energies of neodymium, samarium, and holmium, thirteen are found to be consistent with the available x-ray reference data measured after 1990; only two of the four lines for which reference data predate 1980, however, are consistent with our results. Five lines of terbium are measured with uncertainties that improve on those of existing data by factors of two or more. These results eliminate a significant discrepancy between measured and calculated x-ray line energies for the terbium Ll line (5.551 keV). The line widths are also measured, with uncertainties of 0.6 eV or less on the full-width at half-maximum in most cases. These measurements were made with an array of approximately one hundred superconducting x- ray microcalorimeters, each sensitive to an energy band from 1 keV to 8 keV. No energy-dispersive spectrometer has previously been used for absolute-energy estimation at this level of accuracy. Future spectrometers, with superior linearity and energy resolution, will allow us to improve on these results and expand the measurements to more elements and a wider range of line energies.
arXiv commentThis version is the one accepted for publication in Metrologia
References in corpus (7)
- The Quiescent Intracluster Medium in the Core of the Perseus Cluster
- The ASTRO-H X-ray Observatory
- The Practice of Pulse Processing
- Fe XVII X-ray Line Ratios for Accurate Astrophysical Plasma Diagnostics
- Recent studies of kaonic atoms and nuclear clusters
- Microcalorimeter Spectroscopy at High Pulse Rates: a Multi-Pulse Fitting Technique
- Maximum-likelihood fits to histograms for improved parameter estimation
Cited by in corpus (15)
- Energy of the Th Nuclear Clock Isomer Determined by Absolute -ray Energy Difference
- Eliminating the non-Gaussian spectral response of X-ray absorbers for transition-edge sensors
- A Transition-edge Sensor-based X-ray Spectrometer for the Study of Highly Charged Ions at the National Institute of Standards and Technology Electron Beam Ion Trap
- Testing Quantum Electrodynamics with Exotic Atoms
- L-Edge Spectroscopy of Dilute, Radiation-Sensitive Systems Using a Transition-Edge-Sensor Array
- Absolute energies and emission line shapes of the L x-ray transitions of lanthanide metals
- A Model for Excess Johnson Noise in Superconducting Transition-edge Sensors
- Approaches to the Optimal Nonlinear Analysis of Microcalorimeter Pulses
- Experimental determination of line energies, line widths and relative transition probabilities of the Gadolinium L X-ray emission spectrum
- Resonant soft x-ray scattering from stripe-ordered LaBaCuO detected by a transition edge sensor array detector
- Energy calibration of nonlinear microcalorimeters with uncertainty estimates from Gaussian process regression
- A robust principal component analysis for outlier identification in messy microcalorimeter data
- A Highly Linear Calibration Metric for TES X-ray Microcalorimeters
- Absolute Energy Measurements with Superconducting Transition-Edge Sensors for Muonic X-ray Spectroscopy at 44 keV
- Controlled Shifts of X-ray Emission Lines Measured with Transition Edge Sensors at the Advanced Photon Source