ThorImage^®LS Software

ThorImageLS is an open-source image acquisition program that controls Thorlabs' microscopes, as well as supplementary external hardware. From prepared-slice multiphoton Z-stacks to simultaneous in vivo photoactivation and imaging, ThorImageLS provides an integrated, modular workspace tailored to the individual needs of the scientist. Its workflow-oriented interface supports single image, Z-stacks, time series, and image streaming acquisition, visualization, and analysis. See the video to the lower right for a real-time view of data acquisition and analysis with ThorImageLS.

ThorImageLS is included with a Thorlabs microscope purchase and open source, allowing full customization of software features and performance. ThorImageLS also includes Thorlabs’ customer support and regular software updates to continually meet the imaging demands of the scientific community.

For additional details, see the full web presentation.

New Functionality: Version 4.0 - October 15, 2019 (Click to Expand for More Details)

Please contact ImagingTechSupport@thorlabs.com to obtain the latest ThorImageLS version compatible with your microscope. Because ThorImageLS 4.0 adds significant new features over 3.x, 2.x and 1.x versions, it may not be compatible with older microscopes. We continue to support older software versions for customers with older hardware. See the full web presentation for functionality of previous versions.

New Hardware Support

• Added Support for Windows^® 10 OS
• Added Support for CS895MU and CS505MU Monochrome Cameras (Requires ThorCAM 3.2)
  • Allows for Hot Pixel Correction
• Added Support for CSN210 Motorized Dual-Objective Nosepiece
  • Allows for Improved Objective Setup and Control
• Added Support for Secondary Three Channel Controller
• Added Support for Second LED of the DC2200 LED Driver
• Added Support for New Version of  Thorlabs' Tiberius^® Femtosecond Ti:Sapphire Laser 
  (Up to 1060 nm)
• Added Support for Second Channel for GGNI (Allows for Sequential Imaging with 2 Channels)
• Added Support for Controlling Up to 6 Digital Shutters (ThorShutterDig)
• Added Support for Resonant-Galvo-Galvo Scan-Head (Galvo-Resonant or Gavlo-Galvo Scan Modes Only)
• Added Support for Coherent^® Discovery with AOM Support (Requires Coherent^® Discovery GUI Version 1.8.3 and 3rd Party Virtual Serial Port Software)

User Interface (UI) Improvements

• Renamed “Bleaching” to “Stimulation”
• Added Scale Bar in Image
• Added Help Menu Features
  • Allows User to Check for Updates
  • Allows User to View Log File for Trouble-Shooting
• Added Shortcuts to Hardware Settings and Application Settings in Hardware Connections Window and Edit Under Settings Menu
• Changed Capture Preview of Image to Show Averaged if Cumulative Mode is Used
• Added Control Digital Switches within Script
• Updated Digital Switch Configuration to be Saved in Experiment Settings and Viewable in Experiment Settings Browser
• Updated Extend Filing Numbering Index Out to 6 Digits

New Features

• Added Ability to Save Experiment Data in Multi-Page TIFF Format (OME TIFF)
• Added Rapid Image Update for Galvo-Galvo Scanner
  • Updates Image Every 16 Scan Lines During Acquisition
• Added Galvo-Galvo External Trigger Sync (Minimum 1 MHz) (GGNI Not Supported)
• Added Improved Galvo-Galvo and Galvo-Resonant Triggering Times
• Added Ability to Read Resonant Frequency Probe
• Added Configurable Trigger Output (Signal Generator) Based on Time or Other Digital Events
• Added Auto Update for Histograms
• Added Dedicated Bleach Shutter Control for Galvo-Galvo and GGNI
• Added Stimulation Epoch Control
• Added Additional Stimulation Features (Pre Idle, Post Idle) and Control Lines (Active, Cycle Output, Epoch)
• Added SLM Multiple Epoch Control (Random Epoch)
• Added Ability to Invert Z Control’s Plus and Minus Buttons (Supports Both Primary and Secondary Z Controllers)
• Added Ability to Display X and Y Positions in Microns or Millimeters
• Added BCM-PA Slider Step Size
  • Allows for Setting Slide Step Size When Using Slider Plus and Minus Buttons for Power Adjustment.
• Added Auto Saving of Changed Fine Alignment Values
• Added Ability to Save Image Location and Zoom Level When Switching Image Modalities
• Added ThorSync Changes
  • Stack Panel Option
  • Virtual Channel

Supported Imaging Platforms
Bergamo® II Multiphoton Microscopes		DIY Multiphoton Microscope Kits
Veneto™ Inverted Microscopes	Confocal Imaging Systems	Hyperspectral Imaging System

Introduction

The goal of any microscope is to generate high-contrast, high-resolution images. In much the same way that a telescope allows scientists to discern the finest details of the universe, a microscope allows us to observe biological functioning at the nanometer scale. Modern laser scanning microscopes are capable of generating multidimensional data (X, Y, Z, τ, λ), leading to a plethora of high-resolution imaging capabilities that further the understanding of underlying biological processes.

In conventional widefield microscopy (Figure 1, below left), high-quality images can only be obtained when using thin specimens (on the order of one to two cell layers thick). However, many applications require imaging of thick samples, where volume datasets or selection of data from within a specific focal plane is desired. Conventional widefield microscopes are unable to address these needs.

LSM, in particular confocal LSM and multiphoton LSM, allows for the visualization of thin planes from within a thick bulk sample, a technique known as optical sectioning. In confocal LSM, signals generated by the sample outside of the optical focus are physically blocked by an aperture, preventing their detection. Multiphoton LSM, as we will discuss later, does not generate any appreciable signal outside of the focal plane. By combining optical sectioning with incremented changes in focus (Figure 2, below right), laser scanning microscopy techniques can recreate 3D representations of thick specimen.

Contrast Mechanisms in LSM

Biological samples typically do not have very good contrast, which leads to difficulty in observing the boundaries between adjacent structures. A common method for improving contrast in laser scanning microscopes is through the use of fluorescence.

In fluorescence, a light-emitting molecule is used to distinguish the constituent of interest from the background or neighboring structure. This molecule can already exist within the specimen (endogenous or auto-fluorescence), be applied externally and attached to the constituent (chemically or through antibody binding), or transfected (fluorescent proteins) into the cell.

In order for the molecule to emit light (fluoresce) it must first absorb light (a photon) with the appropriate amount of energy to promote the molecule from the ground state to the excited state, as seen in Figure 3A below. Light is emitted when the molecule returns back down to the ground state. The amount of fluorescence is proportional to the intensity (I) of the incident laser, and so confocal LSM is often referred to as a linear imaging technique. Natural losses within this relaxation process require that the emitted photon have lower energy—that is, a longer wavelength—than the absorbed photon.

Multiphoton excitation (Figure 3B, below) of the molecule occurs when two (or more) photons, whose sum energy satisfies the transition energy, arrive simultaneously. Consequently, the two arriving photons will be of lower energy than the emitted fluorescence photon.

There are also multiphoton contrast mechanisms, such as harmonic generation and sum frequency generation, that use non-absorptive processes. Under conditions in which harmonic generation is allowed, the incident photons are simultaneously annihilated and a new photon of the summed energy is created, as illustrated in Figure 3C below.

Further constituent discrimination can be obtained by observing the physical order of the harmonic generation. In the case of second harmonic generation (SHG), signal is only generated in constituents that are highly ordered and lacking inversion symmetry. Third harmonic generation (THG) is observed at boundary interfaces where there is a refractive index change. Two-photon excitation and SHG are nonlinear processes and the signal generated is dependent on the square of the intensity (I²).

The nonlinear nature of signal generation in multiphoton microscopy means that high photon densities are required to observe SHG and THG. In order to accomplish this while maintaining relatively low average power on the sample, mode-locked femtosecond pulsed lasers, particularly Ti:Sapphire lasers, have become the standard.

Another consideration to be made in nonlinear microscopy is the excitation wavelength for a particular fluorophore. One might think that the ideal excitation wavelength is twice that of the one-photon absorption peak. However, for most fluorophores, the excited state selection rules are different for one- and two-photon absorption.

This leads to two-photon absorption spectra that are quite different from their one-photon counterparts. Two-photon absorption spectra are often significantly broader (can be >100 nm) and do not follow smooth semi-Gaussian curves. The broad two-photon absorption spectrum of many fluorophores facilitates excitation of several fluorescent molecules with a single laser, allowing the observation of several constituents of interest simultaneously.

All of the fluorophores being excited do not have to have the same excitation peak, but should overlap each other and have a common excitation range. Multiple fluorophore excitation is typically accomplished by choosing a compromising wavelength that excites all fluorophores with acceptable levels of efficiency.

Figure 3 Signal Generation in Laser Scanning Microscopy Click to Enlarge Absorptive Process (A, B): The absorption of one or more excitation photons (λEX) promotes the molecule from the ground state (S0) to the excited state (S1). Fluorescence (λEM) is emitted when the molecule returns to the ground state. Non-Absorptive Process (C): The excitation photons (λEX) simultaneously convert into a single photon (λSHG,THG) of the sum energy and half (for SHG) or one-third (for THG) the wavelength.

Image Formation

In a point-scanning LSM, the single-plane image is created by a point illumination source imaged to a diffraction-limited spot at the sample, which is then imaged to a point detector. Two-dimensional en face images are created by scanning the diffraction-limited spot across the specimen, point by point, to form a line, then line by line in a raster fashion.

The illuminated volume emits a signal which is imaged to a single-element detector. The most common single-element detector used is a photomultiplier tube (PMT), although in certain cases, avalanche photodiodes (APDs) can be used. CCD cameras are not typically used in point-scanning microscopes, though are the detector of choice in multifocal (i.e. spinning disk confocal) applications.

The signal from the detector is then passed to a computer which constructs a two-dimensional image as an array of intensities for each spot scanned across the sample. Because no true image is formed, LSM is referred to as a digital imaging technique. A clear advantage of single-point scanning and single-point detection is that the displayed image resolution, optical resolution, and scan field can be set to match a particular experimental requirement and are not predefined by the imaging optics of the system.

Confocal LSM

In confocal LSM, point illumination, typically from a single mode, optical-fiber-coupled CW laser, is the critical feature that allows optical sectioning. The light emitted from the core of the single mode optical fiber is collimated and used as the illumination beam for scanning. The scan system is then imaged to the back aperture of the objective lens which focuses the scanned beam to a diffraction-limited spot on the sample. The signal generated by the focused illumination beam is collected back through the objective and passed through the scan system.

After the scan system, the signal is separated from the illumination beam by a dichroic mirror and brought to a focus. The confocal pinhole is located at this focus. In this configuration, signals that are generated above or below the focal plane are blocked from passing through the pinhole, creating the optically sectioned image (Figure 2, above). The detector is placed after the confocal pinhole, as illustrated in Figure 4 to the right. It can be inferred that the size of the pinhole has direct consequences on the imaging capabilities (particularly, contrast, resolution and optical section thickness) of the confocal microscope.

The lateral resolution of a confocal microscope is determined by the ability of the system to create a diffraction-limited spot at the sample. Forming a diffraction-limited spot depends on the quality of the laser beam as well as that of the scan optics and objective lens.

The beam quality is typically ensured by using a single mode optical fiber to deliver the excitation laser light as a Gaussian point source, which is then collimated and focused into a diffraction-limited beam. In an aberration-free imaging system, obtained by using the highest quality optical elements, the size of this focus spot, assuming uniform illumination, is a function of excitation wavelength (λ_EX) and numerical aperture (NA) of the objective lens, as seen in Equation 1.

Equation 1 Spot Size

In actuality, the beam isn't focused to a true point, but rather to a bullseye-like shape. The spot size is the distance between the zeros of the Airy disk (diameter across the middle of the first ring around the center of the bullseye) and is termed one Airy Unit (AU). This will become important again later when we discuss pinhole sizes.

The lateral resolution of the imaging system is defined as the minimum distance between two points for them to be observed as two distinct entities. In confocal (and multiphoton) LSM, it is common and experimentally convenient to define the lateral resolution according to the full width at half maximum (FWHM) of the individual points that are observed.

Using the FWHM definition, in confocal LSM, the lateral resolution (R_{lateral,confocal}) is:

Equation 2 Lateral Resolution, Confocal LSM

and the axial resolution (R_{axial,confocal}) is:

Equation 3 Axial Resolution, Confocal LSM

where n is the refractive index of the immersion medium.

It is interesting to note that in a confocal microscope, the lateral resolution is solely determined by the excitation wavelength. This is in contrast to widefield microscopy, where lateral resolution is determined only by emission wavelength.

To determine the appropriate size of the confocal pinhole, we multiply the excitation spot size by the total magnification of the microscope:

Equation 4 Pinhole Diameter

As an example, the appropriate size pinhole for a 60X objective with NA = 1.0 for λ_EX = 488 nm (M_{scan head} = 1.07 for the Thorlabs Confocal Scan Head) would be 38.2 μm and is termed a pinhole of 1 AU diameter. If we used the same objective parameters but changed the magnification to 40X, the appropriate pinhole size would be 25.5 μm and would also be termed a pinhole of 1 AU diameter. Therefore, defining a pinhole diameter in terms of AU is a means of normalizing pinhole diameter, even though one would have to change the pinhole selection for the two different objectives.

Theoretically, the total resolution of a confocal microscope is a function of the excitation illumination spot size and the detection pinhole size. This means that the resolution of the optical system can be improved by reducing the size of the pinhole. Practically speaking, as we restrict the pinhole diameter, we improve resolution and confocality, but we also reduce the amount of signal reaching the detector. A pinhole of 1 AU is a good balance between signal strength, resolution, and confocality.

Multiphoton LSM

In multiphoton LSM, a short pulsed free-space laser supplies the collimated illumination beam that passes through the scanning system and is focused by the objective. The very low probability of a multiphoton absorption event occurring, due to the I² dependence of the signal on incident power, ensures signal is confined to the focal plane of the objective lens. Therefore, very little signal is generated from the regions above and below the focal plane. This effective elimination of out-of-focus signal provides inherent optical sectioning capabilities (Figure 2, above) without the need for a confocal pinhole. As a result of this configuration, the collected signal does not have to go back through the scanning system, allowing the detector to be placed as close to the objective as possible to maximize collection efficiency, as illustrated in Figure 5 to the right. A detector that collects signal before it travels back through the scan system is referred to as a non-descanned detector.

Again using the FWHM defintion, in multiphoton LSM, the lateral resolution (R_{lateral,multiphoton}) is:

Equation 5 Lateral Resolution, Multiphoton LSM

and the axial resolution (R_{axial,multiphoton}) is:

Equation 6 Axial Resolution, Multiphoton LSM

These equations assume an objective NA > 0.7, which is true of virtually all multiphoton objectives.

The longer wavelength used for multiphoton excitation would lead one to believe (from Equation 5) that the resolution in multiphoton LSM, compared to confocal LSM, would be reduced roughly by a factor of two. For an ideal point object (i.e. a sub-resolution size fluorescent bead) the I² signal dependence reduces the effective focal volume, more than offsetting the 2X increase in the focused illumination spot size.

We should note that the lateral and axial resolutions display a dependence on intensity. As laser power is increased, there is a corresponding increase in the probability of signal being generated within the diffraction-limited focal volume. In practice, the lateral resolution in a multiphoton microscope is limited by how tightly the illumination beam can be focused and is well approximated by Equation 5 at moderate intensities. Axial resolution will continue to degrade as excitation power is increased.

Image Display

Although we are not directly rendering an image, it is still important to consider the size of the image field, the number of pixels in which we are displaying our image (capture resolution) on the screen, and the lateral resolution of the imaging system. We use the lateral resolution because we are rendering an en face image. In order to faithfully display the finest features the optical system is capable of resolving, we must appropriately match resolution (capture and lateral) with the scan field. Our capture resolution must, therefore, appropriately sample the optical resolution.

In LSM, we typically rely on Nyquist sampling rules, which state that the pixel size should be the lateral resolution divided by 2.3. This means that if we take our 60X objective from earlier, the lateral resolution is 249 nm (Equation 2) and the pixel size in the displayed image should be 108 nm. Therefore, for a 1024 x 1024 pixel capture resolution, the scan field on the specimen would be ~111 μm x 111 μm. It should be noted that the 40X objective from our previous example would yield the exact same scan field (both objectives have the same NA) in the sample. The only difference between the two images is the angle at which we tilt our scanners to acquire the image.

It may not always be necessary to render images with such high resolution. We can always make the trade-off of image resolution, scan field, and capture resolution to create a balance of signal, sample longevity, and resolution in our images.

Considerations in Live Cell Imaging

One of LSM's greatest attributes is its ability to image living cells and tissues. Unfortunately, some of the by-products of fluorescence can be cytotoxic. As such, there is a delicate balancing act between generating high-quality images and keeping cells alive.

One important consideration is fluorophore saturation. Saturation occurs when increasing the laser power does not provide the expected concurrent increase in the fluorescence signal. This can occur when as few as 10% of the fluorophores are in the excited state.

The reason behind saturation is the amount of time a fluorophore requires to relax back down to the ground state once excited. While the fluorescence pathways are relatively fast (hundreds of ps to a few ns), this represents only one relaxation mechanism. Triplet state conversion and nonradiative decay require significantly longer relaxation times. Furthermore, re-exciting a fluorophore before it has relaxed back down to the ground state can lead to irreversible bleaching of the fluorophore. Cells have their own intrinsic mechanisms for dealing with the cytotoxicity associated with fluorescence, so long as excitation occurs slowly.

One method to reduce photobleaching and the associated cytotoxicity is through fast scanning. While reducing the amount of time the laser spends on a single point in the image will proportionally decrease the amount of detected signal, it also reduces some of the bleaching mechanisms by allowing the fluorophore to completely relax back to the ground state before the laser is scanned back to that point. If the utmost in speed is not a critical issue, one can average several lines or complete frames and build up the signal lost from the shorter integration time.

The longer excitation wavelength and non-descanned detection ability of multiphoton LSM give the ability to image deeper within biological tissues. Longer wavelengths are less susceptible to scattering by the sample because of the inverse fourth power dependence (I^-4) of scattering on wavelength. Typical penetration depths for multiphoton LSM are 250 - 500 μm, although imaging as deep as 1 mm has been reported in the literature, compared to ~100 μm for confocal LSM.

When viewing an image with a camera, the system magnification is the product of the objective and camera tube magnifications. When viewing an image with trinoculars, the system magnification is the product of the objective and eyepiece magnifications.

Magnification and Sample Area Calculations

Magnification

The magnification of a system is the multiplicative product of the magnification of each optical element in the system. Optical elements that produce magnification include objectives, camera tubes, and trinocular eyepieces, as shown in the drawing to the right. It is important to note that the magnification quoted in these products' specifications is usually only valid when all optical elements are made by the same manufacturer. If this is not the case, then the magnification of the system can still be calculated, but an effective objective magnification should be calculated first, as described below.

To adapt the examples shown here to your own microscope, please use our Magnification and FOV Calculator, which is available for download by clicking on the red button above. Note the calculator is an Excel spreadsheet that uses macros. In order to use the calculator, macros must be enabled. To enable macros, click the "Enable Content" button in the yellow message bar upon opening the file.

Example 1: Camera Magnification
When imaging a sample with a camera, the image is magnified by the objective and the camera tube. If using a 20X Nikon objective and a 0.75X Nikon camera tube, then the image at the camera has 20X × 0.75X = 15X magnification.

Example 2: Trinocular Magnification
When imaging a sample through trinoculars, the image is magnified by the objective and the eyepieces in the trinoculars. If using a 20X Nikon objective and Nikon trinoculars with 10X eyepieces, then the image at the eyepieces has 20X × 10X = 200X magnification. Note that the image at the eyepieces does not pass through the camera tube, as shown by the drawing to the right.

Using an Objective with a Microscope from a Different Manufacturer

Magnification is not a fundamental value: it is a derived value, calculated by assuming a specific tube lens focal length. Each microscope manufacturer has adopted a different focal length for their tube lens, as shown by the table to the right. Hence, when combining optical elements from different manufacturers, it is necessary to calculate an effective magnification for the objective, which is then used to calculate the magnification of the system.

The effective magnification of an objective is given by Equation 1:

(Eq. 1)

Here, the Design Magnification is the magnification printed on the objective, f_{Tube Lens in Microscope} is the focal length of the tube lens in the microscope you are using, and f_{Design Tube Lens of Objective} is the tube lens focal length that the objective manufacturer used to calculate the Design Magnification. These focal lengths are given by the table to the right.

Note that Leica, Mitutoyo, Nikon, and Thorlabs use the same tube lens focal length; if combining elements from any of these manufacturers, no conversion is needed. Once the effective objective magnification is calculated, the magnification of the system can be calculated as before.

Example 3: Trinocular Magnification (Different Manufacturers)
When imaging a sample through trinoculars, the image is magnified by the objective and the eyepieces in the trinoculars. This example will use a 20X Olympus objective and Nikon trinoculars with 10X eyepieces.

Following Equation 1 and the table to the right, we calculate the effective magnification of an Olympus objective in a Nikon microscope:

The effective magnification of the Olympus objective is 22.2X and the trinoculars have 10X eyepieces, so the image at the eyepieces has 22.2X × 10X = 222X magnification.

Sample Area When Imaged on a Camera

When imaging a sample with a camera, the dimensions of the sample area are determined by the dimensions of the camera sensor and the system magnification, as shown by Equation 2.

(Eq. 2)

The camera sensor dimensions can be obtained from the manufacturer, while the system magnification is the multiplicative product of the objective magnification and the camera tube magnification (see Example 1). If needed, the objective magnification can be adjusted as shown in Example 3.

As the magnification increases, the resolution improves, but the field of view also decreases. The dependence of the field of view on magnification is shown in the schematic to the right.

Example 4: Sample Area
The dimensions of the camera sensor in Thorlabs' 1501M-USB Scientific Camera are 8.98 mm × 6.71 mm. If this camera is used with the Nikon objective and trinoculars from Example 1, which have a system magnification of 15X, then the image area is:

Sample Area Examples

The images of a mouse kidney below were all acquired using the same objective and the same camera. However, the camera tubes used were different. Read from left to right, they demonstrate that decreasing the camera tube magnification enlarges the field of view at the expense of the size of the details in the image.

Click to Enlarge
Acquired with 1X Camera Tube (Item # WFA4100)

Click to Enlarge
Acquired with 0.75X Camera Tube (Item # WFA4101)

Click to Enlarge
Acquired with 0.5X Camera Tube (Item # WFA4102)

To schedule an in-person or virtual demo appointment, please email ImagingSales@thorlabs.com.

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China Demo Room

Try Our Microscopes In Person or Virtually

Thorlabs' sales engineers and field service staff are based out of eight offices across four continents. We look forward to helping you determine the best imaging system to meet your specific experimental needs. Our customers are attempting to solve biology's most important problems; these endeavors require matching systems that drive industry standards for ease of use, reliability, and raw capability.

Thorlabs' worldwide network allows us to operate demo rooms in a number of locations where you can see our systems in action. We welcome the opportunity to work with you in person or virtually. A demo can be scheduled at any of our showrooms or virtually by contacting ImagingSales@thorlabs.com.

Customer Support Sites
(Click Each Location for More Details)

Newton, New Jersey, USA

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Thorlabs HQ

56 Sparta Avenue
Newton, NJ 07860

Customer Support

• Phone: (973) 300-3000
• E-mail: techsupport@thorlabs.com

Ely, United Kingdom

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Thorlabs Ltd.

1 Saint Thomas Place, Ely
Ely CB7 4EX

Customer Support

• Phone: +44 (0)1353-654440
• E-mail: techsupport.uk@thorlabs.com

Bergkirchen, Germany

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Thorlabs GmbH

Münchner Weg 1
85232 Bergkirchen

Customer Support

• Phone: +49 (0) 8131-5956-0
• E-mail: europe@thorlabs.com

Maisons-Laffitte, France

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Thorlabs SAS

109, rue des Cotes
Maisons-Laffitte 78600

Customer Support

• Phone: +33 (0)970 440 844
• E-mail: techsupport.fr@thorlabs.com

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Thorlabs Vendas de Fotônicos Ltda.

Rua Rosalino Bellini, 175
Jardim Santa Paula
São Carlos, SP, 13564-050

Customer Support

• Phone: +55-16-3413 7062
• E-mail: brasil@thorlabs.com

Demo Rooms and Customer Support Sites
(Click Each Location for More Details)

Sterling, Virginia, USA

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Thorlabs Imaging Systems HQ

108 Powers Court
Sterling, VA 20166

Customer Support

• Phone: (703) 651-1700
• E-mail: ImagingTechSupport@thorlabs.com

Demo Rooms

• Bergamo^® II Series Multiphoton Microscopes
• Veneto™ Inverted Microscopes
• Single- and Multi-Channel Cerna^®-Based Confocal Microscopes
• Confocal Upgrade for Existing Systems
• Cerna Hyperspectral Imaging System
• Multiphoton Mesoscope
• Birefringence Imaging System
• OCT Systems: Telesto^® and Ganymede™

Lübeck, Germany

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Thorlabs GmbH

Maria-Goeppert-Straße 9
23562 Lübeck

Customer Support

• Phone: +49 (0) 8131-5956-40840
• Email: oct@thorlabs.com

Demo Rooms

• Ganymede™ Series SD-OCT Systems
• Telesto^® Series SD-OCT Systems
• Telesto^® Series PS-OCT Systems
• Atria^® Series SS-OCT Systems
• Vega™ Series SS-OCT Systems

Nerima-ku, Tokyo, Japan

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Thorlabs Japan, Inc.

3-6-3 Kitamachi
Nerima-ku, Tokyo 179-0081

Customer Support

• Phone: +81-3-6915-7701
• Email: sales@thorlabs.jp

Demo Rooms

• Four-Channel Cerna^®-Based Confocal Systems
• Cerna^® Modular Brightfield Microscopes
• OCT Systems: Ganymede™

Shanghai, China

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Thorlabs China

Room A101, No. 100, Lane 2891, South Qilianshan Road
Shanghai 200331

Customer Support

• Phone: +86 (0)21-60561122
• Email: techsupport-cn@thorlabs.com

Demo Rooms

• Bergamo^® II Series Multiphoton Microscopes
• Single-Channel Cerna^®-Based Confocal Microscopes
• Galvo-Galvo or Galvo-Resonant Confocal Upgrade for Existing Systems
• OCT Systems: Telesto^® and Ganymede™

Standard Mechanical Interfaces on DIY Cerna^® Components

The table below gives the dovetail, optical component threads, and cage system interfaces that are present on each DIY Cerna component. If a DIY Cerna component does not have one of the standard interfaces in the table, it is not listed here. Please note that mechanical compatibility does not ensure optical compatibility. Information on optical compatibility is available from Thorlabs' web presentations.