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Abstract 


Reflection Interference Contrast Microscopy (RICM, also known as interference reflection microscopy) and related techniques have become of wide interest to the biophysical, soft matter and biochemistry communities owing to their exquisite sensitivity for characterising thin films or individual nanoscopic objects adsorbed onto surfaces, or for monitoring cell-substrate interactions. Over the recent years, striking progresses have been made to improve the sensitivity and the quantitative analysis of RICM. Its use in more complex environments, with spurious reflections stemming from a variety of structures in the sample, remains however challenging. In this paper, we demonstrate two methods for adding optical sectioning capabilities to a RICM setup: line confocal detection, and structured illumination microscopy. We characterise experimentally the axial resolution and demonstrate its use for the quantitative imaging of complex biological and biomimetic samples: cellular membranes, thin organic films, surface biofunctionalization. We then discuss the benefits of each method and provide guidelines to arbitrate between sectioning and signal-to-noise ratio. Finally, we provide a detailed description of our experimental setup and a home-written image acquisition and processing software that should allow the interested reader to duplicate such a setup on a home-built or commercial microscope.

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bioRxiv

PPRID: PPR864768
EMSID: EMS196815
bioRxiv preprint, version 1, posted 2024 June 10
https://doi.org/10.1101/2024.06.07.598038

Optical sectioning for reflection interference microscopy

Affiliations

  1. 1.Institut de Biologie de l’ENS (IBENS), Département de biologie, École normale supérieure, CNRS, INSERM, Université PSL, 75005Paris, France
  2. 2.Univ. Grenoble Alpes, CNRS, LIPhy, 38000Grenoble, France
  3. 3.Univ. Grenoble Alpes, CNRS, CERMAV, 38000Grenoble, France
  4. 4.IGF, Univ. Montpellier, CNRS, INSERM, Montpellier, France
  5. 5.School of Biomedical Sciences, Faculty of Biological Sciences, School of Physics and Astronomy, Faculty of Engineering and Physical Sciences, Astbury Centre for Structural Molecular Biology, and Bragg Centre for Materials Research, University of Leeds, LeedsLS2 9JT, United Kingdom

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Abstract

Reflection Interference Contrast Microscopy (RICM, also known as interference reflection microscopy) and related techniques have become of wide interest to the biophysical, soft matter and biochemistry communities owing to their exquisite sensitivity for characterising thin films or individual nanoscopic objects adsorbed onto surfaces, or for monitoring cell-substrate interactions. Over the recent years, striking progresses have been made to improve the sensitivity and the quantitative analysis of RICM. Its use in more complex environments, with spurious reflections stemming from a variety of structures in the sample, remains however challenging. In this paper, we demonstrate two methods for adding optical sectioning capabilities to a RICM setup: line confocal detection, and structured illumination microscopy. We characterise experimentally the axial resolution and demonstrate its use for the quantitative imaging of complex biological and biomimetic samples: cellular membranes, thin organic films, surface biofunctionalization. We then discuss the benefits of each method and provide guidelines to arbitrate between sectioning and signal-to-noise ratio. Finally, we provide a detailed description of our experimental setup and a home-written image acquisition and processing software that should allow the interested reader to duplicate such a setup on a home-built or commercial microscope.

Introduction

Reflection interference contrast microscopy (RICM), also known as interference reflection microscopy (IRM), has been used since the 1960s as a powerful method to image and quantify the interaction of cells with surfaces [1,2]. It has permitted numerous studies in soft matter and biophysics, ranging from wetting to membrane dynamics and cell adhesion. It has also found numerous applications for the study of thin films [3, 4], topology of objects near an interface [5, 6] and nano objects, a field in which the acronym iScat (“interference Scattering”) is used when optimizing for the efficient detection of light scattered by nanometric objects [79]. In short, RIC microscopy relies on the detection of the light reflected (or scattered for nanoobjects) by two or more interfaces (between regions of different optical properties) located within the coherence volume that create an interference pattern encoding information about the optical properties of, and relative distances between the interfaces.

RICM is thus a powerful technique to study thin films and object-substrate interactions, but as a wide field technique, it is sensitive to spurious reflexions outside of the volume of interest that may degrade the contrast of images and limit the sensitivity to small or weakly reflecting objects. While such background may be filtered out, physically through a phase/amplitude filter in the Fourier plane in the imaging path, or numerically at the processing stage, such approaches cannot be applied to a spatially inhomogeneous background such as created by a cell in the vicinity of the focal plane, or even the nucleus and organelles of a cell whose lower membrane is being imaged. Ideally, one would wish to detect signal stemming only from the vicinity of the coverslip - where interferences are located - similarly to the effect achieved in total internal reflection fluorescence (TIRF) microscopy compared to fluorescence confocal microscopy but accommodating lower numerical apertures (see below).

To this aim, we demonstrate the use of two optical sectioning techniques, structured illumination microscopy (SIM) [10] and line confocal (LC) [11] microscopy, applied to RICM. Optical sectioning permits to specifically detect the signal created around the focal plane, removing incoherent background to RICM images arising from out-of-focus structures. While these sectioning techniques have already been demonstrated and modelled at length for fluorescence imaging [1216] or to a lesser extend in reflection [10, 17], their application to RICM has to be adapted to accommodate for partially coherent imaging and peculiar numerical aperture conditions: In RICM, it is indeed critical to tune the coherence volume in accordance with the process under study, so that interferences occur over a limited axial depth around the focal plane where the structures of interest are located. This is achieved by a mix of spatial (numerical aperture modulation) and temporal (illumination spectral width control) coherence tuning [2]. This is in contrast with most uses of optical sectioning techniques, for which the best possible spatial resolution is sought. In particular, controlled (and generally low) illumination numerical aperture are used to facilitate the accurate retrieval of distances from the recorded interference patterns [5, 18]. Here, we therefore establish the use of sectioning techniques such as LC and SIM in the context of RICM at low illumination numerical aperture, and we detail their practical hardware and software implementations. We then present the principle of such combined techniques, and demonstrate the benefits of LC- or SI-RICM for soft matter and biophysics on three application examples: cell imaging in a crowded environment, topology of complex thin films, and monitoring of surface biofunctionalization. Finally, we discuss the benefits of optical sectioning for RICM in relation with existing alternatives.

Results

Principle and practical implementation

The proposed approaches are illustrated on Fig.1: compared to a wide-field RIC microscope, a digital micromirror device (DMD) is inserted in the optical path and is optically conjugated with the focal plane. By applying a black-and-white amplitude mask on the device, the amplitude of the incoming light is modulated at will at frequencies up to 20 kHz and a spatial sampling in the focal plane of 216 nm (for a 60× objective, as set by the camera pixel size and DMD-to-camera magnification factor). The resulting pattern is imaged on a camera and provides optical sectioning through a matching detection pattern or through post processing of the acquired image: in LC imaging (Fig.1, left), a line of controlled width is scanned across the field of view and the signal on the camera is acquired using a rolling shutter (i.e., signal acquisition starts one line after the other, instead of simultaneously for the whole camera) within a matching moving line of fixed width [19, 20]. In this case, similarly to laser scanning confocal microscopy (LSCM), optical sectioning is obtained through rejection of the defocussed reflections of the illumination line that fall mostly out of the detection line for a sufficiently large defocus [12, 16].

Fig 1
Open in new tabFig 1: RIC microscope with optical sectioning.

Center, a schematic view of a RIC microscope is presented, along with the illumination and detection schemes used for line confocal (LC, left) and structured illumination (SI, right) sectioning. The illumination path consists of an incoherent white light source illuminating a digital micromirror device (DMD). Its illumination cone must be large enough to fully neglect the subsequent diffraction and related chromaticism induced by the DMD. The DMD then is imaged onto the sample plane of the objective after spatial filtering through an aperture diaphragm (setting the illumination numerical aperture (INA) and hence the coherence volume within which RIC is observed [2]) and a field diaphragm (limiting the field of view). The field diaphragm is not strictly necessary as a virtual diaphragm can be set by the DMD by limiting the patterned area, but is useful for DMD alignment. The illumination beam is further filtered in polarisation using a polarising beamsplitter cube and a quarter wave plate (QWP) to separate illuminating from reflected light. The gray arrows show the polarisation of the beam at various positions in the beam path. Incoming and refected beams are drawn with an offset from the optical axis for the sake of clarity only, but are in reality incoming at the center of the objective back aperture. The reflected light is then imaged onto a sCMOS camera, either directly (not shown) or after passing through a slit and a beam splitting system to obtain simultaneously two RIC images at different wavelengths (the case of two colours is shown here as an example). Multicamera imaging is also possible to increase the number of simultaneously recorded images.

Alternatively in SIM, a series of illumination structures such as grids with varying orientations and phases are projected onto the focal plane (Fig.1, right) [21, 22], and the signal is reconstructed by calculating the standard deviation of the resulting image stack [10]. More complex algorithms can be used to improve the signal-to-noise ratio and the resolution of the reconstructions, but they all rely on the combination of at least two [23] and up to several tens of images [24], thereby reducing by the same factor the frame rate of the sectioned image acquisition [25]. The most common implementation, used in this paper, uses 3 images of a 1D sinusoidal pattern shifted between each image by one third of a period (I1, I2 and I3). While more efficient algorithms may be used to minimise the image noise and improve its resolution [26], we have restricted ourselves here to the canonical standard deviation calculation approach that has the benefit of simplicity and permits real time video-rate image reconstruction on a recent computer: ISIM=(I1I2)2+(I2I3)2+(I3I1)2(1)

Using the same three images, a widefield image can also be reconstructed using the formula: IWF=I1+I2+I3(2)

LC and SIM are complementary and can be implemented using the same experimental setup, and we detail their relative advantages and limitations in the Discussion section. Complete experimental details on their practical implementation can be found in the Methods section and S3 Fig, and should allow the reader to set up an equivalent sectioning module on their microscope. Briefly, hardware TTL signals are used to synchronize the display of preloaded black and white patterns on the DMD, the acquisition of images on one or several sCMOS cameras, and if needed the motorised displacement of the sample (to acquire several fields of view or adjusting the focus, for example). For SIM, a full image is acquired on the camera with simultaneous exposure of all pixels, while LC uses progressive scan on the camera at a speed synchronised with that of the illumination line movement on the DMD. Conversely, LC images are directly displayed and recorded, while SIM images require further postprocessing to cancel the illumination patterns and obtain a sectioned image (e.g. equ. 1). A home-written LabView software is described in S4 Fig that permits real-time visualisation of SIM sectioned images.

To assess the sectioning ability achieved with either of these methods, we have recorded the signal reflected by a test sample composed of a glass coverslip onto which a nanometric layer of gold has been deposited that provides the optical contrast, and which is covered with immersion oil of refractive index matching that of the glass. This permits neglecting all aberrations introduced upon changes in refractive index at the interface. Here, it should be noted that quantitative image analysis in RICM usually relies on the use of small illumination numerical apertures (INA) so that illumination can be considered quasi-parallel. INA is defined as n sin(αill), with n the refractive index of the sample and aill the maximum angle of the incoming illumination. A low INA also permits optimising the visibility of interferences within the focal volume, and allows visualizing objects up to ≈ 10 μm above the reference surface (together with the appropriate tuning of the temporal coherence) [18]. As a result, the width of the patterns p that can be projected onto the focal volume for optical sectioning is larger than the diffraction limit of the imaging objective (typically pminλ2INA>λ2NA, with NA the full numerical aperture of the objective). This, in turn, limits the performance of optical sectioning thickness to a minimum of δnpminINAnλINA2. Note tat or a given value of p, axial sectioning does not depend on the wavelength, facilitating multicolour SI-RICM. A full description of the image formation process in optically sectioned RICM is beyond the scope of this paper and is the topic of another manuscript in preparation by the authors. Considering that INA in RICM is often limited to 0.3-0.5, one gets a shortest axial sectioning in the range 2-10 μm.

While this is far from the sectioning obtained in TIRF microscopy (a widely-used option for imaging samples close to the coverslip surface), the proposed approaches are more easily compatible with quantitative interference imaging, are easily implemented in the conventional microscope and provide a larger field of view (typically ≈ 10× larger when using a 20× objective, at the expense of a lateral resolution ≈ 1.5 — 2x larger). To demonstrate their usefulness, we provide below three case studies where optical sectioning permits the quantitative analysis of complex samples.

Application example 1 : cell imaging in a complex environment

RICM has widely been used for marker-free quantification of cell adhesion or membrane fluctuations [2729]. While a powerful tool, in its classical configuration its lack of sectioning ability has hampered its use in complex environments such as in the presence of several layers of cells in which quantitative interpretation of images is challenging. In such cases, incoherent background subtraction cannot remove the spurious spatially-heterogenous, time-dependent incoherent signals arising from outside of the coherence volume.

As a proof-of-principle demonstration of optical sectioning with LC, RICM images of red blood cells in PBS sedimented on a glass slide, with and without LC sectioning, are shown on Fig.3. The lower membranes of red blood cells produce well-contrasted fringes that can be used to reconstruct their height profile. As expected, the widefield image exhibits a much higher background intensity due to incoherent parasite reflections, such as stemming from the liquid/air interface at the top of the sample. However, even when subtracting the constant offset from the images, incoherent reflections from area of cells outside the focal volume are visible in the image. In some cases, a second cell resting on a sedimented one modifies the contrast of the fringes, rendering the quantitative analysis of the latter challenging (arrows on Fig.3b). This is representative of typical physiological conditions, where the density of cells within a microvessel can reach 30-40% volume fraction [30]. Studying cell-wall interactions at such high density would thus induce massive out-of-focus heterogeneous reflections from blood cells inside the channel.

Fig 3
Open in new tabFig 3: Red blood cell imaging in a crowded environment

RICM images of red blood cells sedimenting on a glass surface without (a-b) and with (c) LC sectioning. (a) Raw wide field image. (b) Same image with background removed. Outlines of cells stemming from incoherent reflections are still visible in the images (red arrowhead) and can superimpose with the interference pattern (yellow arrowhead). This results in a variable intensity of the interference fringes, as demonstrated in (d) where the profile along the green line is plotted with and without LC sectioning. Scale bar, 10 μm.

In contrast, the same image acquired using LC-RICM yields a much clearer image of the cell structures in the vicinity of the coverslip that provide interferential contrast. Note that the images with and without LC sectioning were acquired sequentially, so that a slight sedimentation and differences in membrane fluctuations are visible in between the two images.

Application example 2 : quantifying the topology of complex surfaces

RICM can also be used as a non-invasive probe of the topology of surfaces decorated with organic material, including wet samples that cannot be dried without altering their structure. Compared to its derived counterpart biolayer interferometry (BLI) [31], it can provide sub-micron resolution in the imaging plane that permits assessing not only the average layer thickness but also the thickness distribution. This is usually performed using multicolour RICM, providing unambiguous information on the layer thickness up to about 1 μm [3, 4]. Quantitative analysis of the RICM signal is however often hampered by the spurious reflections from other interfaces. In particular, it is often convenient to use air objectives for intermediate characterisation steps, so that further functionalization can be performed without cleaning of the lower face of the coverslip, and without sample contamination with immersion oil. This leads to a strong reflection from the non-functionalized side of the coverslip which for samples immersed in water is typically one order of magnitude larger than the signal from the interface of interest itself. In this context, optical sectioning greatly improves the quantification of the surface topology.

As a demonstration, we have imaged a multilayer sample of alternating cellulose nanocrystals (CNCs) and xyloglucan (XG) particles adsorbed on a polyethileneimine (PEI) layer. XGs are the major hemicelluloses in the primary cell wall of dicotyledonous plants, while CNCs in plant cell walls combine with other biomolecules to form supramolecular assemblies reinforcing its structure. The strong interaction between CNCs and XGs permits building biomimetic nano composite films reminiscent of plant cell walls, whose thickness is controlled by the number of (CNC/XG) layers [32]. While such layers can be characterised by AFM at small scale (typical a few μm2), or by neutron reflectivity (with lateral averaging over typically several cm2) [32], multicolour RICM with optical sectioning provides a fast, sub-micrometric, large field-of-view characterization of the film height that can be performed as a quality control at different stages of film deposition. We demonstrate how with a 20×, air objective, line confocal RICM permits monitoring the thickness of a PEI(CNC/XG)5 CNC film over a 200 ×500 μm2 field of view in ≈ 1s with a ≈ 500nm lateral resolution using 3 visible wavelengths (453, 532 and 632 nm) that allow reconstructing pseudo-colour images (Fig.4a). Comparison between widefield and optically sectioned images reveals a striking improvement in contrast and an increased visibility of small structures, as well as a lower sensitivity to out-of-focus impurities (Fig.4a, red arrowheads). Even after FFT filtering to remove the slowly varying background, the visibility of small structures is still hampered by noise and residual background in wide field RICM images compared to line confocal images (Fig.4b, yellow arrowheads).

Fig 4
Open in new tabFig 4: Topology of a biomimetic multilayer film.

(a) A PEI(CNC/XG)5 CNC film immersed in water obtained by layer-by-layer deposition is visualised without (top) and with (bottom) line confocal sectioning in 3-colour RICM, yielding a false colour RGB image that informs on the topology of the film. In the absence of sectioning, a large incoherent background reduces the contrast of the signal of interest. Scale bar, 50 μm. (b) Zoom on the green rectangle in (a), with a Fourier filtering the wide field image (top). This preserves the RICM contrast only if assuming a zero low frequency component in the signal of interest (an assumption that fails in the case of samples thinner than about 100 nm). Even with this filtering, the contrast is still poor compared to the corresponding sectioned image (bottom). Scale bar, 10 μm. (c) Computed hue corresponding to a given height assuming a layer refractive index of 1.4. (d,e) Reconstruction of the height profile based on the 3-colour RICM signal, on the full image (d) and on the green inset (e). The two images share the same colour scale. (f) Histogram of heights measured on each pixel from the full RICM image.

Furthermore, sectioned images can be used to quantitatively reconstruct the topology of the film using simple assumptions for its optical properties: assuming a homogeneous, isotropic refractive index (a reasonable assumption for a disordered film of polysaccharides) ranging from 1.47 (fully dehydrated) to 1.4 (partly hydrated, polysaccharide content 50%) we can reconstruct the variations of hue expected as a function of film thickness (Fig.4c and methods). Interestingly, the colour scale is only weakly affected by the large change in refractive index that we have considered, yielding only a ≈ 5% systematic change in the estimated thickness between these two strongly different hydration assumptions. Based on this hue scale, machine learning is used to map the 3-colour RICM image onto a series of height probability images using 20-nm steps [33]. These images are subsequently combined to obtain a quantitative thickness image over the whole field of view (Fig.4d and 4e, see Methods). These maps provide a wealth of information such as the average film thickness (here ≈ 121 ± 5nm), roughness (here ≈ 24 ± 2nm, see methods for the definition of roughness) and characteristic lateral size of height variations (here ≈ 0.65 μm, close to the resolution limit ≈ 0.5 μm hinting that smaller features are present but less visible or poorly resolved, in agreement with AFM images [32]), as well as a full height histogram (Fig.4f). Previous AFM characterizations have shown that the thickness of hydrated PEI(CNC/XG)5 CNC films was 124 ± 21nm [34], a value with which our height measurement through confocal RICM is in excellent agreement, demonstrating the robustness of our optical measurement experimental setup and processing pipeline.

Application example 3: probing surface biofunctionalization quantitatively

In addition to being non invasive, spatially-resolved and compatible with wet samples, RICM also permits rapid measurements which allow monitoring of sample formation or changes in situ. Here, we imaged the functionalization of a glass interface with a molecular platform permitting controlled presentation of biomolecules at a solid/liquid interface. The platform is composed of a supported lipid bilayer (SLB) incorporating biotinylated lipids (see Methods) that provide anchor points for tetrameric traptavidin molecules (TAv), a variant of streptavidin (SAv) with a larger binding energy [35]. Because only two to three of the four biotin-binding sites are bound to the SLB [36], this platform provides a way to graft a variety of biotinylated molecules at a controlled orientation and surface density, forming well-controlled biomimetic surfaces widely used for in vitro studies of ligand-receptor, or interactions of cells or viruses with model cell surfaces [3739]. The method relies on the fact that the biotin-SAv bond is one of the strongest non-covalent bond known in nature, which is even strengthened in the synthetic variant TAv (35 kT/bond). However, while the SLB-SAv platform has been already widely used and characterised, and in particular the ability of mobile SAv molecules to form 2D crystals above a critical surface concentration [40], its synthetic variant TAv has not been characterized so far for this type of application.

Here, we take advantage of the enhanced sensitivity of SI-RICM to monitor the adsorption of TAv to a biotinylated SLB during TAv incubation. Contrary to spectral ellipsometry, which provide a laterally-averaged quantification of the adsorbed amount of protein, SI-RICM does not straightforwardly inform on the adsorbed surface density of proteins in the regime of a fraction of a single monolayer, but provides a direct readout of the homogeneity of the functionalized surfaces. Interestingly, this sub-micron resolution shows that in incubation conditions that provide homogeneous and mobile SAv layers, TAv forms regions of higher densities (appearing darker in RICM) surrounded by lower density areas (Fig.5). Real-time monitoring shows that this process occurs quasi-simultaneously in the whole field of view and is initiated on sub-resolution defects (lateral resolution ≈ 250 nm, using a 60×, 1.35NA oil objective) in the bilayer (see S1 Video). By analogy with SAv, for which literature extensively documents the formation of 2D crystals on lipid layers [4043], and since when labelled (see below), dense areas display an anisotropic in-plane response and an absence of mobility despite the fluidity of the LSB (confocal imaging and FRAP, not shown), we similarly attribute the dense phase to the formation of 2D crystals.

Fig 5
Open in new tabFig 5: In situ, non-invasive monitoring of TAv adsorption to a biotinylated surface.

(a) 532-nm SI (left) and widefield (right) RICM images of a biotinylated SLB incubated with TAv. Crystals start to form on the surface after ≈ 17 min incubation, with a contrast that remains constant over the whole incubation phase. Scale bars, 20 μm. (b) Relative change in intensity in the crystalline phase compared to the mobile phase with (SIM) and without (WF) SI sectioning, illustrating the gain in contrast thanks to optical sectioning. Error bars are standard deviations on n=24 independent measurements on different crystals of the same sample. (c) Computed concentration of TAv in the mobile phase compared to the crystalline phase using fluorescence confocal microscopy (Fluo), SI and widefield (WF) RICM. SI-RICM is in good agreement with confocal measurements, while widefield RICM underestimates the difference in surface concentration between the two phases. Error bars are standard deviations on n=16 (confocal) or n=24 (RICM) independent measurements on different crystals of the same sample, represented as blue dots. The same sample was measured in RICM and fluorescence to allow direct comparison of the measured densities.

This application highlights the extreme sensitivity of SI-RICM to minute variations of the surface reflectivity which is modulated here by only 0.6%. Importantly, optical sectioning permits analyzing the changes in reflectivity to extract quantitative information about the sample. Here, we observe first that the contrast between the high- and low-density phases is constant over time, indicating that once a sufficient surface density is reached, additional binding of TAv does not increase further the density of the mobile phase, but instead induces growth of the crystalline phase. Furthermore, modelling the optical properties of the SLB-TAv platform and assuming that the TAv crystalline phase density is identical to that of SAv (34 nm2/molecule, or 4.9 pmol/cm2, for crystallization conditions similar to ours [41,42]), we can estimate the density of TAv in the disordered phase (see Methods). We find that the mobile phase is about 30-35% less dense than the crystalline phase (corresponding to 3.3±0.1 pmol/cm2), while analyzing widefield images provides a relative difference of only 13% (corresponding to 4.3±0.05 pmol/cm2). This stems from the lesser contrast of the crystals in the presence of an unknown incoherent background.

To validate the value obtained by SI-RICM, we incubated the platform further with biotinylated-FITC and imaged the sample using fluorescence confocal microscopy: comparing the relative fluorescence intensities in the crystalline and mobile regions confirms a relative change of ≈ 30%, highlighting the benefits of optical sectioning for the quantitative analysis of RICM images. Note that while fluorescent tagging provides a more straightforward measure of TAv surface density, it can only be used after the end of incubation, and prevents further functionalization by biotinylated molecules of interest. This highlights the benefits of SI-RICM for investigating surface functionalization.

Discussion

In this paper, we have demonstrated two complementary methods for obtaining optical sectioning in a RIC microscope through patterning of the illumination light. We have also illustrated the use of these methods for the quantitative monitoring of soft matter samples with high temporal and spatial resolution. Both methods improve the sensitivity of wide-field RICM at the expense of a moderate increase in the imaging system complexity, and require the use of a light patterning device, and of a light source powerful enough to afford the loss of ≈ 50% of the illumination power upon patterning (due to reflection losses on the DMD). However, while reaching optimal axial sectioning requires particular care in the design and alignment of the optical system, the small INAs classically used in RICM minimize issues of chromatic aberrations and field aplanetism compared to, e.g., TIRF microscopy. This makes such a system particular simple to install, and we estimate that a student with experience in optics can setup an equivalent system in about two weeks. To this aim, we provide detailed information about the setup (Fig.1) and its control and synchronization (S3 Fig), to help the interested reader implement a similar sectioning method on their microscope.

In addition, line confocal sectioning requires the patterning device to operate at high speed (typically several kHz to tens of kHz, setting the line rate of image acquisition), and a sCMOS camera with a successive line detection scheme that can be synchronized with the patterning device. This increases the cost of the optical system significantly, and requires particular alignment care when multicolour imaging is sought. In this approach, the illuminating beam is confined along a single, instead of two, spatial dimensions compared to point-scanning confocal imaging and the resulting signal decays relatively slowly with the distance to the focal plane [12, 44]. Its efficiency to cut out the signal reflected from a very bright interface close to the focal plane is thus more limited than that of SIM (see Fig.2b and 2c). In addition, the sectioning in LC decreases is obtained at the expense of a dramatic reduction of the integration time per pixel (typically by a factor Nill/Ntot, with Ntot the total number of DMD lines imaged on the camera, and Nill the number of DMD lines simultaneously illuminating the sample), and hence of the brightness of images. As a result, the benefit of optical sectioning to remove out-of-focus noise may be offsetted by the increased photon noise on the resulting image, unless long integration times and hence low frame rates are used. This limits its acquisition speed benefit compared to SIM, unless the power of the illumination light source can be increased by a factor Ntot/Nill. It should be noted, however, that the decrease in integration time corresponds to an equivalent decrease in sample exposure, so that further integration or intensity increase would not induce additional light-induced detrimental effects. An alternative is to use the physical scanning of the image of the light source focussed onto a thin line, but this approach makes synchronization between illumination and detection scans challenging and only partially mitigates the light loss for an incoherent, high-NA light source as mostly used in widefield RICM.

Fig 2
Open in new tabFig 2: Optical sectioning in RICM.

(a) Test sample used to measure the axial response of the microscope. The gold layer acts as a partially reflective layer between two semi-inifinite regions with similar refractive indices. (b) Axial response in line confocal RICM, obtained with a 20×, 0.85NA oil immersion objective and a 0.46 illumination NA (INA). For a projected line width p ≈ 1 μm (black), δLC ≈ 7.5 μm. For a projected line width p ≈ 2 μm (gray), δLC ≈ 14 μm. (c) Axial response in SI-RICM at three different visible wavelengths, illustrating the possibility to acquire multicolour sectioned RICM images. Profiles were acquired with a 20×, 0.75NA air objective and INA=0.46, using a pattern with period p ≈ 1μm. δSIM ≈ 2 μm.

The advantage of LC, however, is that if the reduction in illumination power does not limit the dynamic range of signal acquisition on the camera, or is the illumination intensity can be increased, the imaging frame rate is unaffected compared to WF imaging and sectioning is obtained through a single image. As a result, fast processes are imaged without loss of temporal dynamics, and without reconstruction artefacts.

In contrast, SIM is compatible with most cameras and patterning devices provided that image acquisition can be synchronized with light patterning at the frame rate (instead of the line rate). This also permits the use of slower, less expensive patterning devices. In addition, sectioning is improved with SIM compared to LC: SIM sectioning can be compared to point-scanning confocal, with intensity dropping sharply outside of the focal volume. In contrast, LC relies on confinement in one spatial dimension only and the intensity therefore decreases more slowly as 1/z (with z the distance from the focal plane), producing a further-reaching tail in the axial intensity distribution (Fig.1). The main drawback of SIM, though, is that contrary to LC it yields raw images with a very strong modulation that prevents observing the sample in real time, unless quasi-real-time processing is performed to display a sectioned image. In S4 Fig, we provide the interested reader with a guide on how to set up such real-time processing, which permits mitigating this limitation.

Another limitation of SIM is that the nonlinear processing used to retrieve the sectioned image also results in an increase of the residual photon noise in the sectioned image, both from the coherent signal and from the incoherent background (compare e.g. the SI- and WF-RICM images in Fig.5a). While the noise is generally low for the large signals achieved in reflection imaging (in contrast to fluorescence imaging), a consequence is that removing a known background through background subtraction, as is used e.g. in iScat, proves more efficient than sectioning. Background subtraction, however, requires that it is possible to accurately record a background image, which is most often difficult to distinguish from the homogeneous reflexion of the coverslip (and hence biases quantitative reflection variation measurements, see Application 3) or might change over time (see Application 1).

It follows that both LC and SIM are particular relevant when background subtraction is not possible (changing or unknown background, complex incoherent reflections from upper parts of the object under investigation) or would bias quantitative measurements. They are also particularly useful for achieving well-contrasted imaging of the sample in real time when exploring a sample in which the background changes with the position and cannot be efficiently subtracted: microfluidic channel, well with a curved upper free surface for the liquid, etc. Table 1 summarizes the comparative benefits of each background removal method.

Table 1. Summary of background removal options for widefield RICM.
Background subtractionLine confocalStructured illumination
Known background requiredYesNoNo
Frame ratemaxmaxmax/3
Illumination powerstandard≈ x100≈ x2
Image brightnessstandardor ≈ /100or ≈ /2
Background noiseIbackground023Ibackground
Movement artifact--+

We underline here that both proposed approaches are compatible with fluorescence imaging, that would also benefit from the same optical sectioning. Since the approach does not impose any constraint on the illumination wavelength, any fluorophore can be used for combined RICM/fluorescence imaging. We also point out that LC- and SI-RICM do not impose any constraint on the type of sample under investigation beyond that of classical RICM (i.e., having a reference surface providing one of the reflected light waves creating the interference pattern): inorganic (gold, silica, anti-reflective or reflection-enhancing coatings) or organic (e.g. surface biofunctionalization, thin Comparative benefits of the different methods for background removal. Frame rate refers to the case where processing is performed offsline,except for line confocal. Image brightness considers identical acquisition time per image and illumination power, and can be mitigated through adjustment of the illumination power (line above). Signal to noise ratio is given for a comparable illumination power and acquisition time for the three methods, and can be reduced by increased exposure, averaging or illumination power. Movement artifacts refer to artifacts induced by the background removal operation. Additionally, distortions or blurring can occur for movements faster than the pixel exposure time.

adhesive or anti-adhesive coatings) deposits can be used without affecting the axial sectioning. In addition, the sample can be included in more complex environments such as microfluidic devices, well plates, etc. Together, these points make the proposed approaches versatile for imaging soft matter or biological samples.

Other approaches have aimed at improving the contrast of RICM images. Interferometric scattering (iScat) provides unprecedented contrast on point-like objects such as individual proteins through a combination of spatial and temporal filtering of the signal [8]. While this method is orders of magnitude more efficient for picking out unlabelled nanometric objects down to the single macromolecule, it is not the best suited to quantify extended structures for which only edges would be detected with a signal that is difficult to relate quantitatively to the sample properties (refractive index, thickness). Similarly, label-free evanescent reflection imaging (epi-EM) [45], which uses an optical configuration similar to TIRF, relies on spatial filtering of the small-angle component of the illumination and detection light. While it permits accurate quantification of the height of relatively well-known objects above a substrate, the use of TIRF objectives limits its field of view and the reconstruction of height profile is quite sensitive to the assumptions on refractive indices in the sample. Both iScat and epi-EM can thus be seen as complementary methods to investigate fine details of relatively well-known samples, while LC- or SI-RICM provides a wide field-of-view mapping of less well-known samples that supports quantitative analysis.

An alternative to increase the contrast of interest is the combination of RICM with custom-designed coverslip coated with multiple layers of transparent material which, upon illumination at the right angle and wavelength, provide a quantitative, dark field image of material deposited at the interface [46]. This methods yields highly contrasted images of thin deposits of material at the coverslip surface, and has been demonstrated e.g. for mapping bacterial trails without staining [47] or monitoring surface functionalization with supported lipid bilayers [48]. It relies on the use of specific coverslips that considerably increase the cost of experiments and can also limit flexibility in sample preparation (e.g., surface biofunctionalization with thiols requiring addition of a gold layer on the coverslip), and impose some constrains on the optical system (INA, illumination wavelength). High-contrast images are however obtained without the need for further image processing. Again, both approaches can be seen as complementary, depending on the sample under investigation.

Conclusion

In this paper, we have demonstrated the use of two optical sectioning methods, line confocal and structured illumination, to provide widefield RICM with axial sectioning, thereby improving the contrast of structures of interest in a crowded environment or in the presence of a strong, unknown incoherent background. Both methods are demonstrated on application examples relevant for biophysical and soft matter studies, and quantification of the optically-sectioned RICM images is demonstrated. The flexibility of these methods should make them useful in a number of experimental situations, and we provide the readers with a detailed guide on how to setup such sectioning methods to make it widely accessible to non-specialists.

Materials and methods

Optical setup

Our optical setup, apart from the DMD, is described in details elsewhere [49]. Briefly, it is based on a modified IX71 Olympus inverted widefield microscope, with the optical turret replaced with a home-built system separating illuminating from reflected light based on polarisation. It consists of a polarisation beamsplitter cube (Thorlabs) and a custom-made optically flat achromatic quarter waveplate (Fichou, France). Illumination is provided by an incoherent plasma light source (HPLS345, Thorlabs) that is spectrally and spatially filtered using dichroic filters (FF01-457/530/628-25, or FF01-530/43-25, Semrock) and graduated diaphragms (SM1D12C, Thorlabs). Before filtering, illumination light is reflected off a high-speed DMD (V-9601, Vialux, Germany) conjugated with the image plane of the microscope objective (depending on the experiment and as mentionned in the text: UPLSAPO60XO, UPLSAPO20XO, and UPLSAPO20X Olympus, Japan). Detection is achieved on one (single colour imaging) or two (3-colour imaging) sCMOS cameras (ORCA-Flash4.0 V2 and V3, Hamamatsu, Japan). For efficient transfer of images to the acquisition computer, the two cameras are connected using dedicated boards (CameraLink pack for Flash4, Hamamatsu). For LC imaging the DMD and the sCMOS are synchronized using a pulse generator (4052 waveform generator, BK precision). For green and blue imaging, a home-built beamsplitting system is used to project the two images on two halves of one of the camera sensors [49]. Each colour image is 2048×1024 pixels. The magnification between the DMD and camera planes is chosen such that one DMD pixel (10.8 μm) is projected onto two camera pixels (2 × 6.5 = 13 μm, corresponding to M=1.2).

Sample preparation

All coverslips (no 1.5, VWR) were cleaned in piranha solution and stored in ultrapure water before use.

Red blood cells were obtained from a healthy donor through the French Blood Bank, diluted in PBS and let to sediment on a clean coverslip. Images were acquired within a few minutes after sample preparation.

CNC/XG multilayer samples were prepared using layer-by-layer deposition of in-house-prepared CNCs from cotton linters and of XG purchased from Dainnipon (Osaka, Japan). PEI (Mw ∼25 000) was purchased from Sigma. A full description of the sample preparation and characterization can be found in [34].

SLB-TAv platform preparation is described in detail in [50]. Briefly, pre-cleaned coverslips were dried, plasma treated for 3 min in water vapour and glued to a home-made teflon holder using two-component silicon glue (Twinsil-speed, Picodent, Germany). After 10 min curing, small unilamellar vesicles (SUVs, 100 μg/mL) in HEPES buffer (HEPES, pH 7.4, 150 mM NaCl in ultrapure water, all from Sigma) were incubated on the coverslip for 30 min and then thoroughly rinsed with HEPES buffer. SUVs were prepared using tip sonication of a HEPES solution of 5 mol % DOPE-cap-B and 95 % DOPC (both Avanti Polar Lipids, USA). At the start of the RICM image acquisition, TAv was added at 40 μg/mL. TAv was expressed and purified from E. coli as described previously [40] and kindly provided by Mark Howarth (University of Cambridge. UK). For subsequent fluorescence staining, TAv was thoroughly rinsed with HEPES, and biotinylated-FITC (10 μg/mL, Thermo Scientific) was incubated for 30 minutes before thorough rinsing with HEPES.

Image acquisition

In SI-RICM, acquisition time was set between 3 and 10ms to avoid saturation of the cameras, and three successive images were taken at 10ms time difference, resulting in a total acquisition time of 30ms. In case of real-time image processing, the frame rate was limited to 20Hz (for a single camera) or 10Hz (for two cameras). For LC-RICM, the acquisition time was set by the line rate (25 μs per line) and the number of simultaneous illuminated lines, ranging from 6 to 20 depending on the illumination line width. As a result, the acquisition time for each pixel was between 150 and 500 μs. For comparison of fluorescence labelling quantification with RICM measurements of TAv density (Application example 3), fluorescence confocal microscopy was performed on a TCS SP8 (Leica, Germany) with a 40×, 1.30NA oil objective and a built-in autofocus. Fluorescence was excited at 488 nm with a power on the sample in the range of ≈ 2μW and detected in the wavelength range of 491–629 nm with a pixel dwell time of 1.2 μs and a sampling of 0.284 μm/pixel. Since labelled TAv crystals produce an anisotropic signal as a function of polarization, we rotated the sample in the imaging plane and acquired 7 images over a range of 180°, and considered the maximum intensity value for each crystal.

Image analysis

Real-time SIM images reconstruction was performed using a home-written software using LabView 11.0 (National Instrument) described in the Supplementary Materials. All other image analysis was performed using the ImageJ bundle FIJI, and reflected intensity numerical calculations were performed using Mathematica.

Reconstructed SIM images often present a small residual modulation at the pattern spatial frequency or a higher harmonic, due to slight deviations from a perfect sine pattern or to illumination fluctuations. This residual modulation is filtered out by FFT filtering centered on the pattern spatial frequency and its harmonics.

For monitoring of TAv crystal formation, prior to TAv incubation, three reference images with shifted illumination patterns were acquired and sectioned and widefield reference images were computed. 3 RICM images with shifted patterned illumination were then acquired every minute after adding TAv to the solution, and the sectioned and widefield images were computed and normalized by their reference counterparts.

For 3-colour analysis of multilayer film height (Application example 2), the contrast of each of the RICM images was adjusted between its minimum and maximum value before the three images were merged into a RGB pseudo-colour image. The corresponding colour scale was built using the formula: Iλ,h=|nfilmnglassnfilm+nglass+nwaternfilmnwater+nfilmexp(4πnfilmλh)|2,(3)

where λ is the wavelength, h is the thickness of the film, and nflim, nglass and nwater are the refractive indices of the multilayer film (assumed to be homogenous), coverslip and water, respectively. The curves for the 3 wavelengths (453, 532 and 632 nm) were then scaled between 0 and 1 and used to create the colour scale shown on Fig.4c. The refractive index of the film depends on its hydration, which is not a priori known. In S1 Figa, we show the scales obtained for a protein content of 50% (n=1.4) and 100% (n=1.47). The weak change in the colour scale illustrates the limited sensitivity to the uncertainty in the exact hydration level. In the analysis, we have then used n=1.4 (50% water content), in agreement with previous estimates of the hydration of these layers when immersed in water [34]. Using this colour scale as a reference, the FIJI plugin Weka Trainable Segmentation [33] is then used to classify the image as the function of pixel hue: classes of heights with 20-30 nm widths are used, and training is achieved by manually referencing pixels to each of the classes based on its hue. Manual inspection found a highest value in the image in the range 460-480nm, while the lowest values were in the range 70-80nm, setting the number of classes used for the full segmentation (16). The output of the Weka classifier is then a series of 16 probability maps for the height of each pixel (see S2 Fig), which were combined to estimate the height through a weighted average of the 3 classes nearest to the one with the highest probability.

To quantify the roughness of the CNC/XG multilayer film, we used the widely-used arithmetic average roughness Ra=1Ni=1Nzi,, where summation is over all the N pixels of the 2D image, and zi is the estimated local thickness.

For estimating the surface density of TAv (Application example 3), the ratio between the intensities of adjacent regions within and outside of the crystalline region is computed at different positions on the sample. To relate this ratio to the local density of TAv, we use a model for the sample that includes a thin layer of medium (n=1.335, thickness 1 nm) [51, 52] above the coverslip (n=1.5196), below a lipid bilayer (n=1.4554, thickness 4.9nm) [52], onto which a TAv layer (thickness 5 nm, in agreement with measured values for SAv [53]) has a density varying between 0 and 100% of the crystalline density (estimated to 268 ng/cm2 [42]). We assume that this corresponds to a linear variation of the refractive index between 1.334 and 1.455 [54]. Coherent addition of the reflections from these different interfaces yields a TAv-concentration-dependant signal which is well described by a parabola in the range 50-100% of the crystal density (S2 Fig). Inverting this function permits converting the experimentally measured ratio of non-crystalline-to-crystalline intensities in ratios of TAv surface densities.

Supplementary Material

Acknowledgments

The authors thank Gwennou Coupier for help with the red blood cell experiment and Mark Howarth for the kind provision of the traptavidin. This work was supported by ANR grant HiTrac (ANR-19-CE42-0010), CNRS MITI grant TOC-SRIM and UGA IRGA grant SRIM-FAST to D.D., the LabEx Tec2l (Investissements d’Avenir, ANR-11-LABX-0030), and the BBSRC (Partnering Award BB/W018500/1; to R.P.R.).

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References

History

  • Posted June 10, 2024.

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Biotechnology and Biological Sciences Research Council (1)