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The yield of 3D in M202HL is reported to be very low (Vrieze, J.; Schenck, C. C.; Hoff, A. J. Biochim. Biophys. Acta 1996, 7276, 229-238), and we confirmed that the absorption of D is not bleached on the 10 /
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33645911001
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note
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When the slow or fast component comprises a relatively small percentage of the total rise amplitude (<30%), the fit values for this component will be less accurate and will deviate from the values of 'B decay measured at 850 nm for direct excitation of B at 795 nm. In general, the slow component appears slower and the fast component appears faster and the values may lie outside the standard deviations reported for 'B decay. We note that such discrepancies are disguised in global analyses (common in the RC literature) where similar rate constants at different wavelengths are forced to converge upon a single value. Energy transfer to the highenergy feature or blue edge of D is likely following ultrafast relaxation (~100 fs) prior to emission (see Discussion and ref 24). For excitation in the B bands, where there is underlying absorption of D, direct excitation of D is unavoidable. Since we would not be able to resolve a 50-100 fs rise (relaxation of the initially excited state prior to emission) along with an ~190 fs rise ('B -D), the fit returns an intermediate value, depending on the relative populations of BM and D excited. This could explain why the rise of 'D in M202HL/M182HL for excitation at 802 nm appears faster than for excitation at 793 nm and why the rise of 'D is faster in general for excitation at the red edge of B compared with the blue edge.
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25
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33645929866
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This result is reminiscent of what was observed in the M214LH ()6 and the M182HL (O)7 mutants, where changing the absorption band of the accessory chromophores (and presumably the spectral overlap of these bands with P) had little effect on the energy transfer rate as measured by the rise of 'P emission
-
This result is reminiscent of what was observed in the M214LH ()6 and the M182HL (O)7 mutants, where changing the absorption band of the accessory chromophores (and presumably the spectral overlap of these bands with P) had little effect on the energy transfer rate as measured by the rise of 'P emission.
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39
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33645904971
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Differences in the kinetics between the QA-reduced and QA-depleted heterodimer RCs are seen in the ratios of the amplitudes of the slow and fast components of 'B emission. Essentially identical ratios between QAreduced and QA-depleted RCs when measuring the rise of 'D at 1040 nm indicates that there are not significant differences in the relative absorption of L and M side chromophores at the excitation wavelengths. One explanation of the amplitude differences in 'B emission is that subtle changes occur in the BL and/or BM emission bands between QA-reduced and QAdepleted RCs
-
Differences in the kinetics between the QA-reduced and QA-depleted heterodimer RCs are seen in the ratios of the amplitudes of the slow and fast components of 'B emission. Essentially identical ratios between QAreduced and QA-depleted RCs when measuring the rise of 'D at 1040 nm indicates that there are not significant differences in the relative absorption of L and M side chromophores at the excitation wavelengths. One explanation of the amplitude differences in 'B emission is that subtle changes occur in the BL and/or BM emission bands between QA-reduced and QAdepleted RCs.
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