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These peak periods are when solar arrays are producing the most excess power.
These peak positions depend mainly on the nature of metal incorporated in SBA-15.
These peak positions are well matched with the reported peaks for PPy [30].
These peak factors are also compared with those directly determined from time history simulations.
These peak shifts clearly indicate the absence of unreacted 1-pyrenebutyric acid and APiB-POSS.
These peak are labeled as AM are obviously related to the manganese impurity.
These peak tops were located around several tens of nanometer pore diameter.
These peak values are well below the accepted maximum trough concentration with parenteral dosing (2 μg/mL).
These peak positions agree with (220), (311), (400), (422), and (511) crystallographic planes of the spinel phase of Fe3O4 [25].
These peak shifts and intensity of extinction spectra for various P3HT/PMMA medium arrays are well described by the finite-difference time-domain (FDTD) simulation results.
These peak are indicated in figure S1A & B with an asterisk.
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