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Principles of Fluorescence Spectroscopy

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PRINCIPLES OF FLUORESCENCE SPECTROSCOPY 173<br />

Figure 5.17. Emission spectra <strong>of</strong> 9,10-diphenylanthracene (DPA) in<br />

ethanol for excitation at 325 nm from a helium–cadmium laser. The<br />

solvent contained a small amount <strong>of</strong> Ludox colloidal silica as the scatterer.<br />

The dashed line is the transmission <strong>of</strong> the Corning 3-75 filter.<br />

Revised from [69].<br />

observed without an emission filter (solid) there is a large<br />

peak due to scattered light at the excitation wavelength <strong>of</strong><br />

325 nm. The presence <strong>of</strong> this scattered component would<br />

not be recognized without measurement <strong>of</strong> the emission<br />

spectrum, and would result in an incorrect intensity decay.<br />

Scattered light is typically rejected from the detector<br />

by using emission filters. In this case we used a Corning 3-<br />

75 filter, which transmits above 360 nm (dashed). As a control<br />

measurement one should always record the emission<br />

spectrum <strong>of</strong> the blank sample through the emission filter to<br />

ensure scattered light is rejected. Alternatively, one can<br />

measure the intensity <strong>of</strong> the blank through the filter to<br />

determine that the blank contribution is negligible. In such<br />

control measurements it is important that the blank scatters<br />

light to the same extent as the sample. Frequently, buffer<br />

blanks do not scatter as strongly as the sample containing<br />

the macromolecules because <strong>of</strong> the inner filter effect present<br />

in the sample.<br />

It is useful to understand how scattered light can corrupt<br />

the frequency-domain data. Frequency responses for<br />

the DPA solution are shown in Figure 5.18. For these measurements<br />

the excitation source was a helium-cadmium<br />

(HeCd) laser at 325 nm. The cw output <strong>of</strong> this laser was<br />

modulated with an electrooptic modulator, as shown in Figure<br />

5.8. The effect <strong>of</strong> scattered light is visually evident in<br />

the frequency-domain data. When measured without an<br />

emission filter, the phase angles (") are considerably smaller<br />

than expected for the single exponential decay <strong>of</strong> DPA<br />

(!). The phase angle error becomes larger at higher frequencies.<br />

It should be noted that the fractional intensity <strong>of</strong><br />

the background is only 15% (f B = 0.15), so that significant<br />

Figure 5.18. Frequency-domain intensity decay <strong>of</strong> 9,10-diphenylanthracene<br />

in ethanol with a scatterer. The sample was in equilibrium<br />

with dissolved oxygen. Data were measured without an emission filter<br />

(") and then corrected (!) for the scattered light using eqs.<br />

5.18–5.23. Bottom panels: deviations from the best single exponential<br />

fits for the data with ("), and corrected for (!) scattered light. Revised<br />

from [69].<br />

errors in phase angle are expected for even small amounts<br />

<strong>of</strong> scattered light.<br />

It is possible to correct for background from the sample.<br />

The solid dots represent the data corrected according to<br />

eqs. 5.18–5.23. The corrected data can be fit to a single<br />

decay time with τ = 6.01 ns. An alternative approach is to<br />

fit the data with scattered light to include a second component<br />

with a lifetime near zero. This also results in a good fit<br />

to the data, with a decay time near zero associated with f B =<br />

0.15. However, this procedure is only appropriate if the<br />

background is only due to scattered light. In general aut<strong>of</strong>luorescence<br />

will display nonzero lifetimes and nonzero<br />

phase angles.<br />

5.5. SIMPLE FREQUENCY-DOMAIN<br />

INSTRUMENTS<br />

A large fraction <strong>of</strong> the cost <strong>of</strong> a frequency-domain instrument<br />

is the light source and/or modulation optics. In<br />

TCSPC these expensive light sources are being replaced by<br />

LDs and LEDs. This substitution is also occurring with frequency-domain<br />

instruments. For most experiments the

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