1. Field of the Invention
This invention relates generally to cytometry tools, and more particularly, to cell sorters and counters used in biotechnological applications such as stem cell research, cancer research, blood analysis, and general clinical studies.
2. Description of the Related Art
Cytometry is a set of techniques designed for counting, imaging, measuring specific cellular parameters and phenotypes. Cytometry provides the ability to analyze and identify individual cells in a large population of heterogeneous cells. The cells are imaged either on slides, micro-titer plates or as they flow through a channel suspended in a focused stream of isotonic media. The latter technique is known as flow cytometry and enables the sorting and purification of large numbers of a specific cell type. All flow cytometers consist of a light source, usually a laser, a channel in which suspended column of cells flow rapidly past an imaging port containing an opto-electrical detector. Cells are primarily analyzed with respect to their light scattering properties and fluorescent signatures. Flow cytometry is widely used in basic and translational biological research as well as clinically. Examples include counting and sorting blood cells, analyzing DNA content, detecting cells in precise stages of the cell cycle and cells undergoing apoptosis. Flow cytometry is routinely used to identify, sort and purify hematopoietic stem cells.
A key element of flow cytometry is the flow chamber. Through the use of a distinct fluid stream, the suspended cells are focused into the center of the fluid stream as they pass through the flow chamber. This enables all cells to be individually exposed to a beam of light. At this position, the cells are at the appropriate focal plane for emitted light to be collected by the optical system and captured by detectors. Typically detectors are positioned both perpendicular and directly in line with the excitation beam. The in-line detector detects light that is forward scattered at a low angle and thus provides information regarding cell size. The perpendicular detector detects high angle scatter, which is caused by highly refractive organelles in the cell such as a nucleus or large vesicles. Finally there is a second perpendicularly positioned detector dedicated for fluorescence detection. Due to a wealth of highly specific fluorescent probes, fluorescent-based flow cytometry has proven particularly powerful in identifying specific cell types. Specific cell types can be identified through highly specific antibodies to cell surface markers. This strategy has proven particularly effective in isolating hematopoietic stem cells. These antibodies can be directly tagged with a fluorophore or indirectly tagged using fluorescently-tagged secondary antibodies. Alternately there is a rapidly growing list of fluorescent small molecule probes that can be used to define cellular phenotypes.
While sorting cells through their forward and side scattering light properties is not as definitive as fluorescent-based cell sorting for identifying specific cell populations, it does have the advantage that it does not require labeling or any modification to the population of cells being analyzed and sorted. This non-invasive feature is particularly important if the cells will be used for in vivo studies. For example, stem cell-based therapies will require that the sorted cells be injected into the patient. For this reason, there is a tremendous need for a more sophisticated method of identifying specific cell types that does not rely on fluorescent labeling, yet can effectively analyze and classify unperturbed unlabeled cells.
In accordance with the present invention, an optical system for label-free, non-invasive analysis of mammalian cells includes a light source, a cell positioner, an optical imager, a Shack-Hartmann optical wavefront sensor and a computer. The light source produces an illuminating beam of spatially coherent radiation. The cell positioner comprised of a sample of multiple cells and a mechanical stage or flow channel precisely positions a single cell within the sample into a sub-aperture region of the illumination beam. The cell perturbs the wavefront of the illumination beam according to the structure of the cell. The optical imager relays a magnified image of the sub-aperture region containing the single cell to an image plane. At the image plane the lenslet array of a Shack-Hartmann wavefront sensor is positioned. Within the pupil of the wavefront sensor the local tilts of the wavefront in the sub-aperture region are measured and sent to a computer. Software produces a set of Zernike coefficients corresponding to the aberrations induced by the morphology of each cell. Cells can then be sorted in a label-free fashion by their Zernike signature.
In a preferred embodiment, the light source comprises a fiber coupled semiconductor diode laser that emits radiation at a wavelength of 635 nm. The fiber output is connected to a lens that produces a collimated illumination beam that is directed into a conventional biological inverted microscope. The laser light is directed through the condenser lens of the microscope. The condenser lens focuses the laser beam to a spot on a microscope slide placed upon an XY translation stage mounted to the microscope body. The microscope slide comprises a sample of multiple mammalian cells distributed randomly. A single isolated cell is manipulated by the XY stage such that it is centered in a sub-aperture region of the laser illumination beam. The laser beam propagates through the cell and into an infinity-corrected objective lens. The objective lens in concert with the tube lens of the microscope provides a lateral magnification of 40×. The magnified image of the cell in the sub-aperture region is exited through an output port of the microscope and further relayed through an afocal beam-expanding telescope that provides an additional magnification of 3×, thereby producing an overall image magnification of 120×. At the plane of the image relayed by the telescope the lenslet array of a Shack-Hartmann wavefront sensor is positioned. The Shack-Hartmann wavefront sensor measures the wavefront tilts caused by the perturbation of the wavefront of the laser beam passing through the single cell on the slide. Using the wavefront tilt information a computer program calculates the Zernike coefficients of the wave aberrated by the cell. These Zernike coefficients provide a signature for the various cell types that are of interest to the biological researcher.
In further accordance with the present invention, a method for analyzing mammalian cells includes producing an illuminating beam of spatially coherent radiation then sequentially moving a single cell from a sample population of multiple cells to within a sub-aperture region of the illuminating beam of coherent radiation. Images of the single cells are magnified and the wavefront tilts of the illuminating beam of coherent radiation are measured. The Zernike coefficients associated with the wavefront distortion imparted on the illuminating beam of coherent radiation by each single cell are calculated and the cells in the sample population are classified according to their Zernike coefficient signatures.
Referring now to the block diagram of
Referring now to the flow chart of
System 100 and the method of
Referring now to the schematic of
System 300 operates as follows. The light source 110 produces an illumination beam 130 that is collimated to a diameter of approximately 400 microns. Laser 310 has a wavelength that lies in the visible region of the electromagnetic spectrum, specifically at 635 nanometers (nm) in this particular embodiment. Condenser lens 380 focuses the illumination beam 130 into the cell positioner 120 to a spot diameter of about 100 microns. Cell positioner 120 sequentially moves single cells 122 into the analysis region represented by sub-aperture region 125. XY stage 325 bi-directionally translates, transverse to the propagating illumination beam 130, the microscope slide 320 such that a single cell 122, with a typical diameter of 10 microns, is centered within the sub-aperture 125. The sub-aperture 125 has a nominal diameter of 25 microns and is roughly defined as the center of the focused illumination beam 130. Optical imager 140 magnifies and relays the image of the single cell 122 in the sub-aperture region 125. Beam splitter 343 is placed in the tube section behind objective lens 342 to allow a portion of the illumination beam 130 to be transmitted towards the CCD camera 390 and a portion to be reflected towards Shack-Hartmann wavefront sensor 160. Objective lens 342 is focused to form an image at 40 × magnification of the object of the single cell 122 at the plane of the image sensor of CCD camera 390. This image is formed in concert with tube lens 112385 and is used for observation, image recording and stage control. Objective lens 342 simultaneously works in concert with tube lens TL1347 and telescope 348 to place a 120 × magnified image of the single cell 122 at the plane of a lenslet array 150, included in the Shack-Hartmann wavefront sensor 160. This image is parfocal with the observation image at the CCD camera 390. The Shack-Hartmann wavefront sensor 160 processes this image and measures the wavefront tilts of the wavefront aberrated by the single cell 122. The computer 170 receives the wavefront tilt measurements from the Shack-Hartmann wavefront sensor 160 and its software calculates the Zernike coefficients related to the aberrations imparted onto the illumination beam 130 by the single cell 122. The single cell 122 can then be classified by its Zernike coefficients which are unique for specific cell structures (e.g.
In more detail, semiconductor diode laser 310 in light source 110 is a Thor Labs Model S1FC635 Fabry-Perot laser that produces up to 2.5 milliwatts of average power at 635 nm. The fiber 312 is a Thor Labs P1-630A-FC-2 which is 2 meters long and is coupled via an FC/PC connector to the laser 310. The fiber 312 is a single mode type which produces an illumination beam 130 with a high spatial coherence (single transverse mode). This spatial coherence aspect of the laser 310 beam quality is important in deriving reliable wavefront tilt information. The collimating lens 314 is a Thor Labs CFC-2X-B aspheric lens with a 2 mm focal length and it also couples to the fiber 312 with an FC/PC connector. The focusing of this collimating lens 314 is adjustable to optimize the collimation of the diverging light emanating from the fiber 312 which has a mode field diameter of about 4.5 microns. The resulting collimated illumination beam 130 has an approximate diameter of 400 microns. The illumination beam is fed into the cell positioner 120 via condenser lens 380 directly or it can be directed via turning mirrors as is customary in laser optical systems.
A standard Olympus IX-71 brightfield inverted microscope is used as the mechanical structure in this system embodiment, although any commercial biological microscope or custom made microscope can be utilized as a system platform for optical system 300. The microscope provides the following components of optical system 300 shown in
The telescope 348 is a CVI Melles-Griot model CWBX-7.0-3X-633 laser beam expander which is anti-reflection coated at 635 nm and provides an additional magnification of 3×, for an overall image magnification of 120×. Telescope 348 is mounted external to the microscope on a stable table surface. The image of the 10-micron diameter cell 122 is thus magnified to 1.2 mm at the intermediate image plane coinciding with the lenslet array 150 of the Shack Hartmann sensor 160. The 25 micron-diameter sub-aperture region 125 is likewise magnified to 3 mm at the lenslet array 150.
Cell positioner 120 in this particular embodiment comprises an automated XY stage 325 that is retrofitted to the Olympus IX-71 stand and a microscope slide 320 of the standard laboratory variety that includes a sample population of cells 122 placed under a cover slip about one millimeter thick. The XY stage 325 is a Prior Scientific H117 ProScan automated stage with 1 micron repeatability and a stage speed of 60 mm/s. Single cells 122 are sequentially positioned by the XY stage 325 into the sub-aperture region, either manually by the operator or under control of computer 170 using standard machine vision software that uses the imagery on camera 390 in concert with XY stage 325 motion control software.
We now give a brief explanation on the workings of the Shack-Ha rtmann wavefront sensor 160 and on Zernike coefficients:
For wavefront analysis it is useful to write the two-dimensional function W(x,y) as a finite series of orthogonal polynomials, where, the Zj(x,y) are Zernike polynomials and the Zernike coefficients cj are weighting factors. The Zernike coefficients describe the wavefront in a concise way which connects to classical aberration theory. In the context of cell 122 sorting, the Zernike coefficients are valuable because they are related to the morphology of an object that perturbs an incident plane wave illumination beam 130. For instance, a subset of the Zernike polynomials is invariant with respect to a coordinate rotation about the z-axis. For a rotationally symmetric perturber, such as a spherical cell 122 (
Real-time data for the Zernike coefficients of an aberrated plane wave can be acquired with a Shack-Hartmann wavefront sensor 160. This device, which is in widespread use in adaptive optics applications, uses a lenslet array 150 and CCD sensor to directly measure the tilts of the wavefront, that is δW/δx and δW/δy , on a grid of x and y values. An array of identical microlenses is positioned one focal length from a CCD array, with the pitch of the lenslet array being larger by some factor (typically 4-10) than that of the CCD, so that the spot of light focused by each lenslet falls within a group of CCD pixels. According to the principles of Fourier optics, each lenslet performs a Fourier transform operation that maps the wavevector k=(kx, ky) of the incident beam (averaged over the lenslet aperture) to a spatial coordinate r=(rx, ry) on the CCD array. The focal length and numerical aperture of the lenslet array 150 and the size of the CCD pixels are chosen so that the diffraction limited spot on the CCD extends over several pixels, which allows the centroid of the spot to be determined to sub-pixel accuracy. From the measured centroid positions and the known focal length of the lenslets one deduces the wave vector components kx and ky, which are proportional to δW/δx and δW/δy . One can “integrate” the partial derivatives to reconstruct the wavefront W(x, y), or use least-squares fitting to find the set of Zernike coefficients that best describes the measured wavefront tilts.
The Shack-Hartmann wavefront sensor 160 used in the preferred embodiment is a Thor Labs model WFS300-14AR which has a lenslet array 150 consisting of 15 by 19 micro-lenses and a CCD with 1280 by 1024 pixels each measuring 4.65 by 4.65 microns. The specified wavefront sensitivity at 633 nm is 1/150 of a wavelength. The pupil area (analysis region) is set by software in computer 170 at 3 mm to equal the diameter of the magnified sub-aperture region 125 containing cell 122 (25 microns multiplied by the 120× image magnification). The cell 122 thus extends over a 1.2 mm region within the pupil. This is an optimum ratio for the Shack-Hartmann wavefront sensor 160 to operate.
The computer 170 is a standard Intel microprocessor based PC loaded with the Thor Labs software to run the WFS300-14AR Shack-Hartmann wavefront sensor 160. The wavefront tilts are processed as described above and the Zernike coefficients are calculated as shown in the examples of
U.S. Pat. No. 7,804,794 9/2010 Vacca et al. 356/337 U.S. Pat. No. 5,017,497 5/1991 De Grooth et al. This application claims the benefit of U.S. Provisional Patent Application Ser. No. 61/306,830, “Cellular Analysis Using Optical Wavefront Sensing”, by John Hoffnagle and James Jacob, filed on Feb. 22, 2010, and of which subjects matter are incorporated herein by reference.