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For our samples we found xs=0.45±0.05.
Average threshold value for our samples was around 40%.
In Fig. 4, the ESR spectra for our samples have been shown.
For our samples these values have been determined from Fig. 8.
The surface roughness for our samples is measured by AFM, which is shown in Figure 4.
For our samples used in this method, the repeatability is less than 47%.
The latter has been the case for our samples that were grown on flat microscope slides.
For our samples, as seen in Table 1, the QD diameter, aspect ratio, and volume increase with the QD height.
However, it has been shown that for our samples, this energy transfer is most efficient at high excitation energies.
The chemical shift of 31P has been found at −4.4 ppm for H3PMo12O40, a value close to those observed for our samples.
On the other hand, r0 measured for our samples is higher than that obtained for local star-forming galaxies selected according to some other star activity tracers.
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CEO of Professional Science Editing for Scientists @ prosciediting.com