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1 March 2010 Additional correction for energy transfer efficiency calculation in filter-based Förster resonance energy transfer microscopy for more accurate results
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Abstract
Förster resonance energy transfer (FRET) microscopy is commonly used to monitor protein interactions with filter-based imaging systems, which require spectral bleedthrough (or cross talk) correction to accurately measure energy transfer efficiency (E). The double-label (donor+acceptor) specimen is excited with the donor wavelength, the acceptor emission provided the uncorrected FRET signal and the donor emission (the donor channel) represents the quenched donor (qD), the basis for the E calculation. Our results indicate this is not the most accurate determination of the quenched donor signal as it fails to consider the donor spectral bleedthrough (DSBT) signals in the qD for the E calculation, which our new model addresses, leading to a more accurate E result. This refinement improves E comparisons made with lifetime and spectral FRET imaging microscopy as shown here using several genetic (FRET standard) constructs, where cerulean and venus fluorescent proteins are tethered by different amino acid linkers.

1.

Introduction

In Förster resonance energy transfer (FRET) microscopy, detection of the sensitized emission from the acceptor—the FRET signal—is obtained by exciting the specimen containing both the donor and acceptor with the donor excitation wavelength. Accurate quantification of FRET signals requires the removal of spectral bleedthrough (SBT) contaminations, which include the donor SBT (DSBT) resulting from the donor emission that is detected in the FRET channel, and the acceptor SBT (ASBT) caused by the direct excitation of the acceptor at the donor excitation wavelength. Algorithms have been developed for various microscopy techniques to identify and remove the SBT contaminations, allowing accurate measurements of the energy transfer efficiency (E) .1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12 In filter-based FRET microscopy, signals are measured in the donor and acceptor emission channels separated using bandpass filters. In contrast, spectral FRET microscopy uses a spectral detector to measure signals over a continuous emission spectrum. Comparing FRET measurements from cells expressing FRET-standard proteins obtained by filter-based or spectral methods suggested a source of error in the filter-based measurements. Our model, which includes the DSBT signals in the quenched donor (qD) for E calculation provides a more accurate measurement of E in filter-based FRET microscopy not previously considered in commonly used algorithms.1, 2, 3, 4, 5, 6, 7, 8 This source of error is not an issue in spectral FRET microscopy, since DSBT is included in the qD used for calculating E . The new model was tested with measurements from GHFT1 cells13 expressing several different genetic (FRET standard) constructs, including C5V, C17V, and C32V, where cerulean (C) and venus (V) are directly tethered by either a 5, 17, or 32 amino acid linker.14 Additionally, a CTV construct was used, where C and V are separated by a 229 amino acid linker encoding the tumor necrosis factor receptor-associated factor (TRAF) domain.9 The results are confirmed with both time-correlated single photon counting (TCSPC) and frequency-domain (FD) lifetime measurements.

2.

Methods

In our theoretical model, for a donor (D)-acceptor (A) FRET system, the energy transfer efficiency (E) is defined as the energy transfer rate (kT) divided by the sum of all deactivation rates of the excited state of D (kT+kD) , where kD is the sum of its deactivation rates other than FRET. At the D excitation wavelength, the decay profiles of the excited D [ DD(t) in Eq. 1] and the excited A [ AD(t) in Eq. 2] are presented, where kA is the sum of the rates for deactivation of the excited A, and D0 and A0 are the absorbed intensities of the D and A at t=0 , respectively.

Eq. 1

DD(t)=D0exp[(kD+kT)t],

Eq. 2

AD(t)=D0kT{exp[(kD+kT)t]exp(kAt)kA(kD+kT)} +A0exp(kAt).
Integrating DD(t) and AD(t) over time (0 to ∞) yields the absorbed intensities of D and A, which are then multiplied by their radiative rates ( kDr and kAr ) to obtain the emitted intensities of D [ IBDD in Eq. 3] and A [ IBDA in Eq. 4].

Eq. 3

IBDD=D0[kDr(kD+kT)]=QYDD0[1E],QYD=kDrkD,

Eq. 4

IBDA=D0(kTkD+kT)(kArkA)+A0(kArkA)=QYAD0E+QYAA0,QYA=kArkA.
Based on E=kT(kD+kT) , kD+kT is substituted by (1E)kD in Eq. 3, and kT(kD+kT) is substituted by E in Eq. 4. QYD and QYA are the respective natural quantum yields of D and A. IBDD refers to the signals emitted from the donor, which are called quenched donors (qD) . IBDA represents the signals emitted from the acceptor and is composed of the FRET (QYAD0E) and ASBT (QYAA0) signals (see Sec. 1).

In spectral microscopy imaging, the IBDD in Eq. 3 and IBDA in Eq. 4 can be directly measured using the combination of linear unmixing and ASBT correction to estimate E .9, 10, 11, 12 In our spectral FRET method known as sFRET,10 using the D (IDDS) and A (IAAS) reference spectra obtained from the respective single-label to unmix a double-label λ stack obtained under the donor excitation (IBDS) produces IBDD and IBDA images. Thus, E can be calculated by Eq. 5, which is derived from Eqs. 3, 4

Eq. 5

E=coefFRETcoefFRET+qD,FRET=IBDAASBT,qD=IBDD,coef=(ssDssA)(QYDQYA),
where a coefficient (coef) is introduced with SSD and SSA , which are the detector quantum efficiencies at the D and A peak emission wavelengths, respectively. The qD signals are quantified by the IBDD image. The FRET signals are measured by separating the ASBT signals from the IBDA image, and the ASBT signals are determined using the single-label acceptor specimens.10

In filter-based microscopy imaging, separate bandpass filters are usually used to measure the signals emitted close to D and A peak emission wavelengths. In our filter-based FRET method known as PFRET,7 at the D excitation wavelength, two images of the donor- and acceptor-labeled specimen are acquired IBDd in the D emission channel and IBDa in the A emission channel. In contrast to the IBDA image in spectral FRET, the IBDa image acquired using the filter-based method also contains the DSBT signals emitted from the donor, in addition to the FRET and ASBT signals emitted from the acceptor. The IBDd image is commonly used to measure the qD signals for the E calculation, as shown in Eq. 6.1, 2, 3, 4, 5, 6, 7, 8

Eq. 6

E=coefFRETcoefFRET+qD,FRET=IBDaASBTDSBT,qD=IBDd,
where coef has the same meaning as described in Eq. 5. FRET is measured by separating both DSBT and ASBT from the IBDa image, and the DSBT and ASBT are determined using the single-label donor and acceptor specimens.7 The DSBT signals appearing in the IBDa image in filter-based FRET are included in the qD (the IBDD image) for the spectral FRET E calculation [Eq. 5], but is not in the qD (the IBDd image) for the filter-based FRET E calculation [Eq. 6]. Significantly, DSBT is actually part of qD , so adding DSBT back to the IBDd image can provide a more accurate E measurement when using a filter-based FRET method, as shown in Eq. 7.

Eq. 7

E=coefFRETcoefFRET+qD,FRET=IBDaASBTDSBT,qD=IBDd+DSBT.

3.

Results and Discussions

The use of FRET-standard fusion proteins allowed direct comparison of the energy transfer efficiencies (E) measured in intensity- and lifetime-based FRET microscopy. The representative decays (TCSPC) and phasor plots15, 16 (FD) of the C-alone and FRET-standard constructs (Fig. 1 ) clearly demonstrate a shorter lifetime from C to CTV to C32V to C17V to C5V. In both TCSPC and FD FLIM measurements, the E of a FRET-standard construct was estimated from the donor (C) lifetimes determined in the absence ( τD as unquenched lifetime) and the presence ( τDA as quenched lifetime) of the acceptor (V) based on 1(τDAτD) :17 τDA was measured from the cells labeled with CTV, C17V, C32V or C5V; and the corresponding τD was determined from the cells labeled with C (for CTV), C32A (for C32V), C17A (C17V), or C5A (for C5V), where A (amber) is a nonfluorescent form of Venus.14

Fig. 1

FLIM-FRET data representation. Both TCSPC [Becker and Hickl (Bh, Berlin, Germany) SPC 150, Biorad Radiance 2100 Ex 820nm ]13 and FD [ISS (Champaign, Illinois) ALBA Ex 440 nm] FLIM-FRET measurements were carried out to verify the intensity-based FRET results. The lifetime results were obtained through TCSPC—fitting the decay data given an estimated instrument response function (IRF) in Bh SPCImage software; and FD—fitting the phase shifts and amplitude attenuations in ISS Vista Vision software. For all donor-alone controls and the CTV construct, a single exponential fitting was sufficient to yield good approximation of the raw data, while double exponential fitting had to be applied to the C32V, C17V, and C5V constructs. (a) TCSPC shows the estimated IRF and the representative decay profiles of the cerulean-alone (C) and FRET-standard constructs, clearly demonstrating a faster decay (a shorter lifetime) from C to CTV to C32V to C17V to C5V. (b) FD displays the representative phasor plots drawn from raw data measured at 20MHz [semicircle as the single lifetime curve; (1,0) zero lifetime; and (0,0) infinite lifetime],15, 16 clearly demonstrating a longer lifetime from C5V to C17V to C32V to CTV to C, and also showing the corresponding CTV, C17V, C32V, and C5V lifetime images. The distribution of C or CTV almost centers on the semicircle, indicating they both follow a monoexponential decay. The center of the distribution of C32V, C17V, or C5V falls inside the semicircle, conforming why they require double exponential fittings. (For both: objective-Nikon 60×1.2NA W; and emission filter 48030nm ).

020513_1_076002jbo1.jpg

In Fig. 2 , we summarized the results of the analysis of cells expressing the same FRET standard fusion proteins by the four FRET microscopy methods—spectral confocal FRET, filter-based confocal FRET with the E determined by Eq. 6 or 7 (see Sec. 2), TCSPC, and FD FLIM-FRET. For each construct, at least 12 cells were measured in each method and the E at each pixel of each cell. The E columns and inserted table represent the average E of all analyzed pixels in all cells. The coef (0.635) value involved in the E calculation in spectral or filter-based confocal FRET was determined empirically using the C5V E obtained by the TCSPC FLIM-FRET method as a reference. Both the columns and the numbers in Fig. 2 clearly demonstrate that the theoretically derived Eq. 7 produces an E for filter-based confocal microscopy that more closely matches the lifetime or spectral FRET measurements. Based on our PFRET results, the accuracy of E increases by including the DSBT in qD [Eq. 7]. The refinement of the E calculation presented here is of particular interest to those researchers who use multiple FRET methods, sometimes simultaneously, to achieve their research goals.

Fig. 2

FRET efficiency (E) comparison. The average Es of CTV, C32V, C17V, and C5V constructs measured in the four FRET microscopy methods are compared as columns and actual numbers in the inset ( n12 for each construct measured in each method; the bar on the top of each column indicates the standard deviation). Es in filter-based FRET were calculated using both Eqs. 6, 7 (see Sec. 2). For the C5V, C17V, or C32V construct, ANOVA analyses indicate conventional Eq. 6 results in a statistically different E of the same construct estimated by other methods (spectral, TCSPC, and FD) (p<0.05) . In contrast, Eq. 7 statistically matches the other methods (p> 0.05) . For the CTV construct, the intensity-based Es are found to be different than the FLIM-FRET Es based on ANOVA analysis, because the very low FRET signal level of the CTV construct results in a poor signal-to-noise ratio (SNR) in the intensity-based methods, and in turn affects the accuracies of their E estimations. However, it is still clearly shown that the average E obtained with Eq. 7 is closer to those obtained by other methods than the average E obtained with Eq. 6 within their small variations. [For filter based and spectral FRET: Zeiss 510 Meta; 63X/1.4NA Oil, Ex. 458 nm (donor), Ex. 415 nm (acceptor); filter-based: Em. 470~500 nm (donor) and Em. 535~590 nm (acceptor); spectral: Em. 458~561 nm.]

020513_1_076002jbo2.jpg

Acknowledgments

This work was supported by the University of Virginia and the National Center for Research Resources, NIH RR021202 (AP).

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©(2010) Society of Photo-Optical Instrumentation Engineers (SPIE)
Yuansheng Sun and Ammasi Periasamy "Additional correction for energy transfer efficiency calculation in filter-based Förster resonance energy transfer microscopy for more accurate results," Journal of Biomedical Optics 15(2), 020513 (1 March 2010). https://doi.org/10.1117/1.3407655
Published: 1 March 2010
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KEYWORDS
Fluorescence resonance energy transfer

Microscopy

Optical filters

Energy transfer

Image filtering

Resonance energy transfer

Energy efficiency

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