<p><b>Table 2.</b> Characterization of the Ti Kβ spectral profile. The profile is fully characterized on an absolute energy scale through a sum of component Lorentzians convolved with a Gaussian instrumental broadening. Integrated areas <em>A<sub>i</sub></em>, centroids <em>C<sub>i</sub></em> and FWHMs <em>W<sub>i</sub></em> of individual components were obtained from a fit of intensity against detector position. The detector position axis was transformed to an absolute energy scale via the calibration procedure. The Gaussian width σ = 1.244(41) eV. The background was <em>B</em> = 831(26) counts. The second and third components are dominant, contributing more than three quarters of the intensity of the spectrum while the fourth component is...
A high resolution study of Ti Kα X-ray spectra versus projectile Z has been performed. Energy shifts...
It is known that the peak of Uranium (U) Lα line (13.6 keV) overlaps with that of Rubidium (Rb) Kα l...
The financial support of the Swiss National Science Foundation (Grant No. 200020-146739) is acknowle...
<p><b>Table 4.</b> The full characterization of the V Kβ spectral profile on an absolute energy scal...
<p><strong>Figure 6.</strong> The peak energies of the fits of individual measured Ti Kβ spectra. Ea...
<p><b>Table 3.</b> Error budget for the peak energy of all the spectral profiles of Ti Kβ that go in...
<p><strong>Figure 1.</strong> Schematic diagram of experimental setup.</p> <p><strong>Abstract</stro...
<p><strong>Figure 5.</strong> Typical fit of a Ti Kβ spectrum. The crystal clinometer voltage was −1...
<p><strong>Figure 8.</strong> The peak energies of the fits of individual measured V Kβ spectra. Eac...
<p><strong>Figure 3.</strong> The energy shift from Bragg's law predicted by Mosplate, including pea...
<p><b>Table 1.</b> Characteristic radiation peak energy data from Chantler <em>et al</em> [<a href="...
In most high-accuracy x-ray experiments, characteristic radiation is used to determine calibration e...
Titanium spectra recorded in the infrared wavelength region with a Fourier Transform Spectrometer ha...
These spectra compare the Ti 2p core-level XPS line shape for atomically clean, stoichiometric sampl...
Titanium full Kα spectra have been measured using a vide-band crystal spectrometer in lover-hybrid c...
A high resolution study of Ti Kα X-ray spectra versus projectile Z has been performed. Energy shifts...
It is known that the peak of Uranium (U) Lα line (13.6 keV) overlaps with that of Rubidium (Rb) Kα l...
The financial support of the Swiss National Science Foundation (Grant No. 200020-146739) is acknowle...
<p><b>Table 4.</b> The full characterization of the V Kβ spectral profile on an absolute energy scal...
<p><strong>Figure 6.</strong> The peak energies of the fits of individual measured Ti Kβ spectra. Ea...
<p><b>Table 3.</b> Error budget for the peak energy of all the spectral profiles of Ti Kβ that go in...
<p><strong>Figure 1.</strong> Schematic diagram of experimental setup.</p> <p><strong>Abstract</stro...
<p><strong>Figure 5.</strong> Typical fit of a Ti Kβ spectrum. The crystal clinometer voltage was −1...
<p><strong>Figure 8.</strong> The peak energies of the fits of individual measured V Kβ spectra. Eac...
<p><strong>Figure 3.</strong> The energy shift from Bragg's law predicted by Mosplate, including pea...
<p><b>Table 1.</b> Characteristic radiation peak energy data from Chantler <em>et al</em> [<a href="...
In most high-accuracy x-ray experiments, characteristic radiation is used to determine calibration e...
Titanium spectra recorded in the infrared wavelength region with a Fourier Transform Spectrometer ha...
These spectra compare the Ti 2p core-level XPS line shape for atomically clean, stoichiometric sampl...
Titanium full Kα spectra have been measured using a vide-band crystal spectrometer in lover-hybrid c...
A high resolution study of Ti Kα X-ray spectra versus projectile Z has been performed. Energy shifts...
It is known that the peak of Uranium (U) Lα line (13.6 keV) overlaps with that of Rubidium (Rb) Kα l...
The financial support of the Swiss National Science Foundation (Grant No. 200020-146739) is acknowle...