The present invention relates generally to multi-species fluorescence microscopy techniques.
Confocal laser scanning microscopy (CLSM) with fluorescence is a widely used imaging tool for cell and molecular biology. This technique offers the possibility of three-dimensional imaging, deep imaging, live cell imaging, and quantitative imaging, all together and combined with current developments in fluorescence microscopy. At present, a wide variety of fluorescent dyes (e.g., synthetic dye molecules, fluorescent proteins, and inorganic nanoparticles) may be bound to biological targets with high specificity and through numerous coupling strategies, potentially providing a complete portrait of the observed sample. So-called multi-species (or multi-label) fluorescence imaging allows the detection of multiple targets, enabling the observation of interactions and relative spatial organization among different cellular structures with specific molecular contrast. In addition, the recent introduction of fast detector arrays (in the MHz range) has enabled a transparent and versatile implementation of image scanning microscopy (ISM), which has led CLSM to be counted among super-resolution techniques. In such an ISM implementation (described, for example, in WO 2019/145889 A1), a detector array—the projected size of which in the sample plane is 1-1.5 airy units (AU)—replaces the pinhole and single-element detector, typically used in CLSM, to provide an image of the fluorescent volume. This additional spatial information provided by the detector array may be used to reconstruct a super-resolved image with twice the resolution of conventional microscopy and a higher signal-to-noise ratio (SNR). Each element of the detector array acts as a single physical pinhole that produces a series of super-resolved but low SNR images. Since most of the fluorescence signal is acquired in parallel from the detector elements, a high SNR image may be obtained by combining all the images collected by pixel reassignment or multi-image deconvolution.
In conventional CLSM, simultaneous multi-species imaging is implemented by separating the different probes—or rather, the different fluorescent signals—on the basis of the photophysical properties of each probe. In particular, three different properties are typically used: the excitation spectrum, the emission spectrum, and the mean fluorescence lifetime (
The most widely used method for simultaneous multi-species CLSM imaging separates the signals of different probes by exploring the signatures of their emission spectra. All probes are simultaneously excited with one or more monochromatic laser beams (λexc). The fluorescent signal is then isolated from the excitation light and divided into a series of spectral windows (λdet, where λdet denotes the central value of the spectral band)—one for each probe—by a combination of filters, dichroic mirrors and/or adjustable acousto-optic filters. Finally, a detector for each spectral band, i.e., a probe, records the fluorescence signal. Said multi-detector spectral implementation has two major limitations: the number of detectors required increases with the number of probes, and the cross-talk between the emission spectra of different probes degrades the image.
The second problem may be partially solved by breaking the simultaneity of excitations to add information on the excitation spectra of the probes in the embodiment. In this case, the excitation laser beams are activated/modulated sequentially, and a series of images is recorded: one for each pair of values related to detector band and excitation beam wavelength (λexc, λdet). The image formed by the best corresponding excitation and emission wavelengths is selected for each probe. Then, the remaining cross-talk may be eliminated using linear unmixing algorithms. Because of the sequential activation of laser excitation beams, it is crucial to adopt fast modulation to effectively obtain simultaneous imaging. For example, a frame-by-frame or line-by-line modulation may be too slow to perform imaging of dynamic structures. Because fast biological processes occur with sub-millisecond time scales (changes in shapes of the proteins occur with much smaller scales, down to microseconds, but imaging is not an option for observing such processes in every case), and the typical dwell time of the pixel is in the range of tens of microseconds or less, the modulation of the laser beams on a pixel-by-pixel basis ensures simultaneous multi-species imaging.
Recently it has been proposed to modulate the excitation beams with a frequency greater than that given by the dwell time of the pixel (U.S. Pat. No. 9,231,575 B2). Said multi-species CLSM implementation multiplexes the excitation beams in the frequency domain. Accordingly, demodulation is achieved by filtering in the frequency domain. Moreover, said implementation uses a single detector without regard to the number of probes to be separated, thus greatly reducing implementation costs. In contrast, the use of a single detector precludes exploration of the excitation and emission spectra of the probes.
A multi-species CLSM that uses a single detector but explores the emission spectrum may be implemented using a linear detector array (US 20190361213 A1). Here, the fluorescence signal—induced by one or more excitation beams—is spectrally decomposed in space using a prism (or grating), and each wavelength is mapped to a specific position/element of the linear detector. The three-dimensional (x, y, λ) image, the so-called emission spectral image, is processed by a (blind) spectral unmixing algorithm to form the final multi-species image potentially free of artifacts due to the cross-talk of the signals. In this class of CLSM implementations, typically called hyper-spectral implementations, it is also possible to explore excitation spectra by modulating the excitation beams as described above. Hyper-spectral CLSM implementations could also be achieved by sequentially recording emission spectra; i.e., the fluorescence signal is spectrally dispersed in space, an adjustable double slit selectively filters only part of the spectrum, and a single-element sensor records the selected signal. Nevertheless, sequential recording of spectra prevents (by definition) simultaneous multi-species imaging.
All multi-species CLSM implementations described above use the emission signature and/or excitation signature to separate different probes. Another probe signature to be explored is the mean fluorescence lifetime and, more generally, the time decay distribution. Similar to the excitation and emission spectra, a probe may be characterized by a time spectrum f(t), which describes the probability that an excited molecule/probe will emit a spontaneous photon (fluorescent photon) at a given time t after the excitation event. The mean time the molecule spends in the excited state is called the mean fluorescence lifetime τ. In the case of a pure organic fluorophore, said distribution may be described by a single exponential ft∝exp(−t/τfl), but more convoluted models are needed in many practical cases. In CLSM, the mean lifetime decay distribution of a fluorescent probe is obtained by implementing a time-correlated single-photon count (TCSPC) experiment: a pulsed laser beam (typically with a pulse length of a few tens of picoseconds) excites the probe at a specific time (t=0); a single-photon detector with a low timing jitter (from tens of picoseconds up to a few hundred picoseconds) records the fluorescent photons emitted by the probes; a time-to-digital converter (TDC) or a high-frequency digitizer measures the time difference between the excitation and recording events. The histogram of the arrival time of the photons is measured by repeating experiments (typically, the pulsed laser has a repetition rate on the order of tens of MHZ). In a TCSPC-based CLSM, multi-species imaging may be implemented by recording the photon arrival histogram for each pixel and decomposing said histogram (according to the decay distribution of different probes) using different computation algorithms based on fitting, deconvolution, phasor decomposition, or linear unmixing. An interesting property of said implementation is the possibility of separating species with very similar excitation and emission spectra, thus using a single excitation beam and a single detection band, i.e., a single detector, which not only brings benefits in terms of complexity, but also allows imaging artifacts due to chromatic aberrations to be avoided. The same TCSPC-based CLSM system may be used to implement the above-described excitation laser modulation in a pulse-by-pulse mode, thus enabling exploration of the excitation spectral signature for multi-species imaging. The pulses from a series of monochromatic lasers are subjected to interleaving (with a delay longer than the mean fluorescence lifetime), and the histogram of the arrival time of the photons is used to implement time-gated detection and separate the signal associated with each probe. Said pulse interleaving approach may also be combined with emission spectral separation approaches to increase the number of probes to be separated, but more detectors are needed.
One of the most notable advantages of ISM implementation based on a fast detector array is its compatibility with many labeling methods, techniques, and protocols implemented in fluorescence CLSM, including many of the multi-species imaging techniques described above.
ISM is fully compatible with the spectral multi-detector approach, the modulated multi-excitation approach, and combinations thereof. Consequently, a person skilled in the art may easily integrate such simultaneous multi-species approaches into ISM. However, to date only slow frame-by-frame modulated multi-excitation ISM implementations have been demonstrated. In this case, different excitation wavelengths and spectral windows are alternated through motorized filter lenses using a single detector array; however, true simultaneous imaging such as that demonstrated in CLSM is precluded.
Conversely, hyper-spectral methods are not fully compatible with ISM. The basic principle of hyper-spectral methods is to decode spectral information in space, i.e., to decompose emission spectra spatially. Such spatial decomposition interferes with ISM because in ISM the spatial information channels are already used to transfer the image of the detection volume. Because spatial and spectral information are fused in the same channel and scale, their decomposition is non-trivial. For completeness, a hyper-spectral ISM implementation has been proposed and used to reconstruct two-species ISM images. However, for the same reasons described above, this implementation is subject to major artifacts in both spatial resolution and species separation.
The recent introduction of single-photon detector arrays (such as the single-photon avalanche diode array detector (SPAD)) also enables the implementation of multi-species imaging methods based on the mean fluorescence lifetime signature. In effect, the ability of the SPAD array-based ISM to implement TCSPC measurements has been fully demonstrated. However, in this case, no demonstration of multi-species ISM based on mean fluorescence lifetime has been reported.
Due to the introduction of asynchronous SPAD array detectors, many of the simultaneous multi-species imaging methods demonstrated in CLSM may in principle be extended to ISM, with some substantial limitations regarding hyper-spectral approaches. However, similar to CLSM, there is no single method able to explore, at the same time, the excitation spectrum, the emission spectrum, and the mean fluorescence lifetime signature. The constraints become even more important when only a single detector may be used in the implementation.
One object of the invention is to propose a new architecture for multi-species ISM imaging that provides simultaneous imaging, high scalability in terms of number of species, and low cost. Another object of the invention is to propose a new architecture that also offers similar benefits for CLSM, and more generally, for any fluorescence technique based on laser scanning microscopy (LSM), e.g., stimulated emission depletion microscopy (STED), two-photon excitation microscopy (TPE), and fluorescence fluctuation spectroscopy (FFS).
In light of these objects, the subject of the invention is a laser scanning microscope configured to illuminate a specimen with a plurality of pulsed excitation light beams comprising different spectral components, hereinafter excitation spectral components, said specimen containing a plurality of fluorescent species, wherein the microscope comprises:
Another subject of the invention is a method of laser scanning microscopy, comprising:
Single-photon detectors allow access to a wide range of time scales (with the only lower limit being the sub-nanosecond scale) due to their low photon timing jitter (when an element in the detector array receives a photon, it activates a signal with an accuracy of up to 200 ps), the reduced waiting time (up to 50 MHz, i.e., after a photon has been collected, the element remains blind for 20 ns), and the asynchronous readout (i.e., each detector array element is fully independent of the others).
While the mean fluorescence lifetime information is in the sub-nanosecond/nanosecond time scale, the fastest biological processes and the laser scanning process occur in the microsecond range. Thus, a simultaneous multi-species LSM would be feasible even with detectors covering only a time scale down to the microsecond, but the implementation of multi-species ISM based on the mean fluorescence lifetime of the probe would require access to the nanosecond time scale. In short, the time scale from tens of nanoseconds to microsecond is little used and may be adopted to transfer additional information (in practice, in LSM and used to improve the SNR).
Therefore, the idea behind the invention is to use this available band to transfer useful information to separate probes in the simultaneous multi-species ISM. Here, in particular, said available band is used to encode the excitation and emission spectral signatures of the probes. This idea translates into a TCSPC-based ISM measurement, where the photon arrival time histogram is used to encode: (i) the mean fluorescence lifetime signature of the probes, as in typical TCSPC experiments; (ii) the excitation spectral signature of the probes, by phase-multiplexing different excitation beams; and (iii) the emission spectral signature of the probes, by temporally separating the different spectral components of the fluorescent signal.
Note that hyper-spectral methods separate the spectral component of the fluorescent signal in space rather than time. Once the photon arrival time histogram has been recorded, well-established computational methods such as (blind) linear unmixing, phasor-based unmixing, fitting, deconvolution, or machine learning may be used to decode the probe signatures to obtain a multi-species ISM image. Since all encoding operations are performed using the time channel, the proposed approach may use a single detector. Moreover, because the encoding uses the sub-microsecond time scale, the simultaneous multi-species approach is ensured. Note that the same strategy may be applied for CLSM with a typical single-element, single-photon detector, but super-resolved images in this case are not obtainable.
The main advantages offered by the proposed solution over existing multi-species imaging approaches are:
Further features and advantages of the invention will be presented in the following detailed description, which refers to the attached drawings, provided only by way of non-limiting example, wherein:
Methods according to the invention may be implemented using, as the starting microscope architecture, a TCSPC-based ISM configuration (as described in M. Castello et al., “A robust and versatile platform for image scanning microscopy enabling super-resolution FLIM” [1]) or based on digital heterodyne.
In short, the starting microscope is a multi-beam pulsed laser fluorescence confocal microscope where the pinhole is fully open, and the conventional single-element detector typically used in CLSM is replaced with a single-photon detector array (e.g., a SPAD array detector), denoted as 40 in the figures. The different spectral components defined by the excitation beams are denoted as B1 and B2 in
Due to the two encoders and the pulse excitation scheme, each probe is characterized by a specific time signature, which will be called a color-time signature hereinafter. The single-photon detector array 40 records a linear combination of said signatures, the coefficients of which are proportional to probe concentrations. Therefore, the primary task of the decoder 70 is to computationally retrieve the coefficients of said linear combination (and possibly also the color-time signatures). In practice, the decoder 70 is implemented using spectral (blind) unmixing. (blind) deconvolution, phasor decomposition, fitting (if a signature model is provided), or machine learning algorithms. The (blind) spectral unmixing approach will be described in more detail hereinafter.
The most important property and condition to be fulfilled in practical embodiments of the proposed method is that the fluorescence signal generated by the time-resolved measurement fx(t) (i.e., the histogram of the photon arrival time) in the position x of the sample (i.e., the image pixel) and at the time t, is a linear composition of the color-time signatures sl(t) and the relative contributions/concentrations cl,x of the different probes:
where X is the number of spatial positions in the sample (image pixels), and L is the number of probes to be separated. The number of probes is typically known in any multi-species fluorescence imaging experiment. As indicated above, the color-time signature sl(t) is a function of the signature of the mean fluorescence lifetime τl(t), the excitation spectral signature el(λ), and the emission spectral signature ml(λ) of the probe. Two examples of a color-time signature sl(t) as a function of τl(t), el(λ) and ml(λ) are shown in
In order to implement multi-species blind imaging, the object of the decoder 70 is to estimate, for each position x of the sample, the concentrations cl,x and color-time signatures sl(t), starting from their “mixture” fx(t) (see
Considering the time-resolved measurement after the time discretization and the time sampling window t=t1, . . . , tT of the photon arrival time, Equation 1 may be written in vector notation as:
fx=[fx(t1), . . . , fx(tT)]T is the histogram of photon arrival time measured in the x-th pixel and sl=[sl(t1), . . . , sl(tT)]T is the color-time signature for the l-th species. Thus, switching to vector notation:
where S=[s1, . . . , sL] with S∈RT×L and cx=[c1,x, . . . , cL,x]. Finally, by incorporating all spatial samples (i.e., all pixels), the model of the mixture (equation 1) may be described by three matrices:
where F=[f1, . . . , fX] is the overall time-resolved measurement matrix, with F∈RT×X, and C=[c1, . . . , cX] is the concentration of each species at each available location in the sample, with C∈RL×X.
Given that in fluorescence microscopy the sample is typically artificially labeled, not only the number of species L is known, but also the color-time signatures sl(t) may be individually calibrated and estimated a priori. However, it should be kept in mind that calibrated signatures may sometimes be highly dependent on imaging conditions and labeling protocol (thus they may change from sample to sample).
Therefore, both the most arduous situation, where the color-time signatures sl(t) are not known, and the simplest case, where the color-time signatures sl(t) are known, are considered. If the color-time spectra S are known, C may be calculated from F by linear unmixing, otherwise the problem becomes a linear blind unmixing problem.
An example of how to solve the blind problem is now described. The non-blind problem is clearly a simplification of that more general problem and is typically solved sequentially (pixel-by-pixel) using equation 3 instead of equation 4. With the matrix notation of equation 4, the decoding operation, i.e., the unmixing problem, may be written as a problem of minimizing the difference between the measured “mixture” F and the modeled/predicted “mixture” SC. A different formulation of said minimization problem may be obtained on the basis of alternative assumptions, such as the probability distribution of the noise contaminating the measurements (e.g., Gaussian or Poissonian noise), and on other assumptions about color-time signatures and concentration values, typically introduced through regularization terms in the minimization problem. A formulation is given here where the Frobenius norm is used [2]:
Typical constraints to be introduced in the minimization problem are normalization and non-negativity of color-time signatures:
Furthermore, since in the blind problem the minimization is achieved by considering all sample locations together, it is common practice to impose an intensity normalization on the data measured at each sample location (image pixel), i.e., fxT1T=1∀x, which results in the following constraints on the coefficients:
The absolute intensity of each species l and each pixel x is obtained by multiplying the corresponding coefficient cl,x obtained by the total measured non-normalized initial intensity Σi=1Tfx(ti).
A typical solution to the linear blind unmixing problem is obtained by an inverse least squares procedure that minimizes the difference between the measured mixture and the modeled/predicted mixture [3]. Another example of how to transform the blind and non-blind unmixing problems by considering Poissonian noise in the measured mixture may be found in [4]. Note that the minimization approach described here is only one of several ways to transform the unmixing problem of equations 4 and 5. For example, the unmixing problem may be solved using other computational approaches such as phasor transformation, fitting, or machine learning. Note also that all of the above examples are used to solve the unmixing problem in the context of CLSM and only where typical hyper-spectral measurements or mean fluorescence lifetime histogram measurements are used.
The approach according to the invention measures a specially defined signature: the color-time signature, which encodes all the photophysical features of the fluorescent probes in the time-resolved measurement. Thus, conventional unmixing algorithms are used to calculate the probe coefficients/concentrations from the measured color-time signature.
Embodiment with a Discrete Emission Spectrum Encoder
As mentioned above, a first practical embodiment to effectively encode the excitation and emission spectra of the probes into the photon arrival time histogram will now be described. For the excitation spectrum encoder 50, a pulse interleaving is used to encode excitation spectra, i.e., a sequence of J excitation pulses at different wavelengths is implemented (λjexc with j=1, . . . , J), which is repeated periodically with a predetermined frequency (see
An effective implementation of pulse interleaving, which relies only on electronic components, may be achieved by using a set of triggerable pulsed diodes, the pulses of which may be electronically synchronized with each other with specific delays. The excitation beams are then focused on the sample, and the fluorescence signal is collected by an objective lens and supplied to the emission spectrum encoder 60. There, the fluorescence signal is split by a series of dichroic mirrors into spectral windows K([λjem, λj+1em] with j=1, . . . , K+1). Each window is capable of containing different portions of the probes' fluorescence according to their emission spectra (ml(λ) with (=l, . . . , L). Subsequently, the different components are guided through optical paths with different lengths (for example, an optical delay line) to introduce specific time delays. Finally, all components are recombined by a second set of dichroic mirrors and sent back onto the single-photon detector array 40 (a simplified example of that which is achieved by this process is shown in
where * denotes the convolution operator; τl(t) is the mean fluorescence lifetime signature for the l-th probe; tjexc is the delay of the i-th laser excitation beam; tkem is the delay of the k-th detection spectral window. In short, αl,j is the probability of exciting the l-th probe with the j-th laser beam, and βl,k is the probability that the emission from the l-th probe falls in the k-th time window. With some simple calculations, the following equation for the color-time signature is obtained:
In practice, the pulse sequence is repeated with a frequency 1/T, so T is the maximum value of the measured photon arrival time; tjexc<T, ∀j; tkem<T, ∀j. Moreover, to avoid overlapping signature copies of mean fluorescence lifetime, the excitation delay and emission delay should be separated by a time longer than the mean lifetime of all probes τlfl.
Note that the sequence of excitation pulses may be arranged to implement Hadamard coding to improve the SNR of the measurement, and here the delay tjexc may also be equal.
Embodiment with a Continuous Emission Spectrum Encoder
In this alternative practical embodiment, the encoder of the emission spectrum 60 changes while the encoder of the excitation spectrum 50 remains unchanged. In said continuous encoder, the emission spectrum is not separated into discrete windows, but is spatially separated by a prism, grating, or other similar device. Each component of the emission spectrum (continuous) follows a different path (with linearly increasing length) so as to introduce a different delay as a function of wavelength. Subsequently, all components are spatially recombined and sent to the single-photon detector array 40.
In this case, defining the coordinate variation m(t)=m(λ/a) that linearly delays the emission spectrum in time as a function of a time constant a, the color-time signature is given by:
With some simple calculations the following is obtained:
A prototype of the microscope (
The detection of a conventional confocal laser scanning microscope (CLSM) on an optical bench was modified. The traditional instrument is equipped with two excitation laser sources having respective wavelengths of 485 nm (LDH-P-C-485B, PicoQuant) and 560 nm (LDH-D-TA-560, PicoQuant).
A pulsed interleaving excitation scheme (excitation spectrum encoder 50) is implemented by commanding lasers with TTL signals from an FPGA control system (40 MHz repetition rate (laser period 25 ns), 12.5 ns delay between each pulse).
The sample is scanned by the laser beam through a pair of galvanometer mirrors (6215HM40B, CTI-Cambridge) and an objective lens (CFI Plan Apo VC60x oil, Nikon). Fluorescent photons are collected from the same objective lens, de-scanned and filtered by a multiband dichroic mirror (ZT-488-561-640-775, AHF Analysentechnik). The fluorescent signal is then sent to the emission spectrum encoder 60, which consists of a dichroic mirror (low-pass filter 575 nm, Edmund Optics) and four mirrors that define a delay line at 6.25 ns (corresponding to an optical path length of about 1.87 m) for fluorescence with wavelengths greater than 575 nm.
Finally, the beam is expanded and projected onto an array of SPAD detectors 40. The detector array has 25 elements arranged in a 5-by-5 array; it is mounted on a commercial stand with micrometer screws for fine alignment on three axes. The spatial and temporal performance of the detector array was evaluated, showing a temporal resolution of 200 ps and temporal jittering between 110 and 160 ps in the active area.
The detector array is controlled by a traditional dedicated operation board that provides power and performs electrical signal conditioning. The board provides 25 digital output channels (each related to the arrival of a photon on a specific element of the detector array), which are fed into a data acquisition system.
The data acquisition system was developed with a commercial FPGA development board (National Instruments USB-7856R), equipped with a Kintex7 FPGA processor and connected to a personal computer. The standard digital pixel/line/frame clock lines are used to synchronize the acquisition system with the microscope control system.
A digital heterodyne in the frequency domain is implemented in the FPGA control system to calculate the histogram of the photon arrival time.
Number | Date | Country | Kind |
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102021000017018 | Jun 2021 | IT | national |
Filing Document | Filing Date | Country | Kind |
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PCT/IB2022/056046 | 6/29/2022 | WO |