HighPower MicroSpot® Focusing Objectives for VIS and NIR Lasers
 5X, 10X, 20X, or 50X Magnification
 532 nm, 850 nm, or 1064 nm Center Wavelength
 Better than 95% Transmission at Center Wavelength
 Damage Threshold ≥15 J/cm^{2}
LMH5X1064
5X Magnification,
980  1130 nm AR Coating
LMH50X850
50X Magnification,
790  910 nm AR Coating
LMH20X532
20X Magnification,
495  570 nm AR Coating
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Objective Lens Selection Guide 

Objectives 
Super Apochromatic Microscope Objectives Microscopy Objectives, Dry Microscopy Objectives, Oil Immersion Physiology Objectives, Water Dipping or Immersion Phase Contrast Objectives Long Working Distance Objectives Reflective Microscopy Objectives UV Focusing Objectives VIS and NIR Focusing Objectives 
Scan Lenses and Tube Lenses 
Scan Lenses FTheta Scan Lenses InfinityCorrected Tube Lenses 
Features
 Designed for HighPower Industrial Lasers
 532 nm Center Wavelength, 490  570 nm AR Coating
 850 nm Center Wavelength, 790  910 nm AR Coating
 1064 nm Center Wavelength, 980  1130 nm AR Coating
 All Fused Silica Lens Design
 RMSThreaded (0.800"36) Housing
 Damage Threshold of ≥15.0 J/cm^{2}(See the Damage Thresholds Tab for More Details)
Applications
 Laser Engraving
 Laser Cutting
 2D and 3D Photolithography
 3D Printing
 Stealth Dicing
 Laser Welding
Zemax Files 

Click on the red Document icon next to the item numbers below to access the Zemax file download. Our entire Zemax Catalog is also available. 
Click to Enlarge
This diagram illustrates the labels, working distance, and parfocal distance. The format of the engraved specifications will vary between objectives and manufacturers. (See the Objective Tutorial tab for more information about microscope objective types.)
Thorlabs' HighPower MicroSpot^{®} Focusing Objectives are designed to focus onaxis laser beams to a diffractionlimited spot. We offer center wavelengths of 532 nm, 850 nm, and 1064 nm, with AR coatings of 490  570 nm, 790  910 nm, and 980  1130 nm, respectively. These objectives can be used at common fiber laser wavelengths including 515 nm, 808 nm, 1030 nm, or 1070 nm. Objectives with a 532 nm or 1064 nm center wavelength are also ideal for use with Nd:YAG lasers; for additional optics for use with these lasers, see the Nd:YAG Optics tab. All of the focusing objectives below offer a damage threshold of ≥15 J/cm^{2} (see the Damage Thresholds tab for more details). The RMS threading on each of our MicroSpot objectives allows for easy integration into existing systems, and their robust housing and fused silica lens design is built to hold up to consistent industrial or laboratory use.
Focusing objectives can be used in a variety of applications where intense optical power is necessary, such as laser cutting or engraving. At lower powers, focused laser light can be used for wafer inspection or to activate special types of photoresist in photolithography. Because all the objectives on this page have a limited field of view, laser scanning should be performed by moving either the sample or the objective. When incorporating these objectives into a system, note that the labeled magnifications of these objectives are calculated assuming the objective is being use with a 200 mm focal length tube lens.
Each 50X objective is equipped with a cover glass correction collar with engraved graduations, in mm, for fused silica coverslip thicknesses from 0 to 1 mm. In addition, the 1064 nm variant is engraved with a scale for up to 1.2 mm thick silicon carbide coverslips. The scales span the majority of the objectives' circumferences, allowing for smooth, precise adjustment. Once the correct position is found, the collar can be locked in place by tightening the setscrew below it with the included 0.050" hex key. Custom graduations for specific cover glass materials including sapphire (Al_{2}O_{3}), silicon (Si), silicon carbide (SiC), gallium arsenide (GaAs), and gallium nitride (GaN) can be made on request; please contact Tech Support for more details.
These objectives are capable of producing a neardiffractionlimited spot size when used with a monochromatic source within the 450  2100 nm range that fills the entrance aperture, also known as the entrance pupil. However, if used at a wavelength other than the design wavelength, the effective focal length listed on the Specs tab will shift and the AR coating will no longer be optimized; see the Graphs tab for AR coating plots. Custom AR Coatings are available by contacting Tech Support to optimize the performance of these objectives at other wavelengths. When working with wavelengths outside of the visible, consider using some of Thorlabs' laser viewing cards to help locate and align your beam.
Our MicroSpot objectives are externally RMSthreaded (0.800"36), which allows them to be mounted directly to our fiber launch systems, DIY Cerna^{®} Microscope Systems, and microscope objective turrets; to convert RMS threads to M32 x 0.75 threads, we offer the M32RMSS brass thread adapter. Our 5X, 10X, and 20X objectives can be mounted to any of our flexure stages using an HCS013 RMS mount. An objective case (OC2RMS lid and OC22 canister) is included with our 50X objectives and an aluminum cap (RMSCP1) is available for purchase separately.
For wavelengths between 192 nm  500 nm, Thorlabs offers UV MicroSpot Laser Focusing Objectives in a number of magnifications; this range covers many excimer lasers which cure photoresist, such as KrF lasers (248 nm) and ArF lasers (193 nm).
Click Here for Raw Data
The shaded region of this graph identifies the specified wavelength range of the AR coating.
Click Here for Raw Data
This graph shows the reflectance per surface. The shaded region identifies the specified wavelength range of the AR coating.
AR Coating Specifications  

Wavelength Range  Average Reflectance per Surface  Max Reflectance per Surface  Damage Threshold 
495  570 nm  <0.2% (495  570 nm)  <0.7% (488  580 nm) <0.2% (503  553 nm) 
15 J/cm^{2} (532 nm, 20 Hz, 10 ns, Ø213 µm) 
Click Here for Raw Data
The shaded region of this graph identifies the specified wavelength range of the AR coating.
Click Here for Raw Data
This graph shows the reflectance per surface. The shaded region identifies the specified wavelength range of the AR coating.
AR Coating Specifications  

Wavelength Range  Average Reflectance per Surface  Max Reflectance per Surface  Damage Threshold 
790  910 nm  <0.2% (790  910 nm)  <0.7% (794  935 nm) <0.2% (833  855 nm) 
20 J/cm^{2} (850 nm, 10 Hz, 10 ns, Ø300 µm) 
Click Here for Raw Data
The shaded region of this graph identifies the specified wavelength range of the AR coating.
Click Here for Raw Data
This graph shows the reflectance per surface. The shaded region identifies the specified wavelength range of the AR coating.
AR Coating Specifications  

Wavelength Range  Average Reflectance per Surface  Max Reflectance per Surface  Damage Threshold 
980  1130 nm  <0.2% (980  1130 nm)  <0.7% (960  1160 nm) <0.2% (1000  1100 nm) 
20 J/cm^{2} (1064 nm, 20 Hz, 10 ns, Ø395 µm) 
Chromatic Aberration Correction per ISO Standard 190122  

Objective Class  Common Abbreviations  Axial Focal Shift Tolerances^{a} 
Achromat  ACH, ACHRO, ACHROMAT  δ_{C'}  δ_{F'} ≤ 2 x δ_{ob} 
Semiapochromat (or Fluorite) 
SEMIAPO, FL, FLU  δ_{C'}  δ_{F'} ≤ 2 x δ_{ob} δ_{F'}  δ_{e} ≤ 2.5 x δ_{ob} δ_{C'}  δ_{e} ≤ 2.5 x δ_{ob} 
Apochromat  APO  δ_{C'}  δ_{F'} ≤ 2 x δ_{ob} δ_{F'}  δ_{e} ≤ δ_{ob} δ_{C'}  δ_{e} ≤ δ_{ob} 
Super Apochromat  SAPO  See Footnote b 
Improved Visible Apochromat  VIS+  See Footnotes b and c 
Parts of a Microscope Objective
Click on each label for more details.
This microscope objective serves only as an example. The features noted above with an asterisk may not be present on all objectives; they may be added, relocated, or removed from objectives based on the part's needs and intended application space.
Objective Tutorial
This tutorial describes features and markings of objectives and what they tell users about an objective's performance.
Objective Class and Aberration Correction
Objectives are commonly divided by their class. An objective's class creates a shorthand for users to know how the objective is corrected for imaging aberrations. There are two types of aberration corrections that are specified by objective class: field curvature and chromatic aberration.
Field curvature (or Petzval curvature) describes the case where an objective's plane of focus is a curved spherical surface. This aberration makes widefield imaging or laser scanning difficult, as the corners of an image will fall out of focus when focusing on the center. If an objective's class begins with "Plan", it will be corrected to have a flat plane of focus.
Images can also exhibit chromatic aberrations, where colors originating from one point are not focused to a single point. To strike a balance between an objective's performance and the complexity of its design, some objectives are corrected for these aberrations at a finite number of target wavelengths.
Five objective classes are shown in the table to the right; only three common objective classes are defined under the International Organization for Standards ISO 190122: Microscopes  Designation of Microscope Objectives  Chromatic Correction. Due to the need for better performance, we have added two additional classes that are not defined in the ISO classes.
Immersion Methods
Click on each image for more details.
Objectives can be divided by what medium they are designed to image through. Dry objectives are used in air; whereas dipping and immersion objectives are designed to operate with a fluid between the objective and the front element of the sample.
Glossary of Terms  

Back Focal Length and Infinity Correction  The back focal length defines the location of the intermediate image plane. Most modern objectives will have this plane at infinity, known as infinity correction, and will signify this with an infinity symbol (∞). Infinitycorrected objectives are designed to be used with a tube lens between the objective and eyepiece. Along with increasing intercompatibility between microscope systems, having this infinitycorrected space between the objective and tube lens allows for additional modules (like beamsplitters, filters, or parfocal length extenders) to be placed in the beam path. Note that older objectives and some specialty objectives may have been designed with finite back focal lengths. In their inception, finite back focal length objectives were meant to interface directly with the objective's eyepiece. 
Entrance Pupil Diameter (EP)  The entrance pupil diameter (EP), sometimes referred to as the entrance aperture diameter, corresponds to the appropriate beam diameter one should use to allow the objective to function properly. EP = 2 × NA × Effective Focal Length 
Field Number (FN) and Field of View (FOV) 
The field number corresponds to the diameter of the field of view in object space (in millimeters) multiplied by the objective's magnification. Field Number = Field of View Diameter × Magnification 
Magnification (M)  The magnification (M) of an objective is the lens tube focal length (L) divided by the objective's effective focal length (F). Effective focal length is sometimes abbreviated EFL: M = L / EFL . The total magnification of the system is the magnification of the objective multiplied by the magnification of the eyepiece or camera tube. The specified magnification on the microscope objective housing is accurate as long as the objective is used with a compatible tube lens focal length. Objectives will have a colored ring around their body to signify their magnification. This is fairly consistent across manufacturers; see the Parts of a Microscope Objective section for more details. 
Numerical Aperture (NA)  Numerical aperture, a measure of the acceptance angle of an objective, is a dimensionless quantity. It is commonly expressed as: NA = n_{i} × sinθ_{a}where θ_{a} is the maximum 1/2 acceptance angle of the objective, and n_{i} is the index of refraction of the immersion medium. This medium is typically air, but may also be water, oil, or other substances. 
Working Distance (WD) 
The working distance, often abbreviated WD, is the distance between the front element of the objective and the top of the specimen (in the case of objectives that are intended to be used without a cover glass) or top of the cover glass, depending on the design of the objective. The cover glass thickness specification engraved on the objective designates whether a cover glass should be used. 
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.
Manufacturer  Tube Lens Focal Length 

Leica  f = 200 mm 
Mitutoyo  f = 200 mm 
Nikon  f = 200 mm 
Olympus  f = 180 mm 
Thorlabs  f = 200 mm 
Zeiss  f = 165 mm 
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' previousgeneration 1501MUSB 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.
Figure 1: A Gaussian intensity profile only asymptotically approaches zero, so the spot size is defined by convention as either the fullwidth at halfmaximum (FWHM) or 1/e^{2} value. We use the latter convention in this tutorial.
Spot Size Tutorial
The spot size achieved by focusing a laser beam with a lens or objective is an important parameter in many applications. This tutorial describes how the ratio of the initial beam diameter to the entrance pupil diameter, known as the truncation ratio, affects the focused spot size and provides expressions for calculating the spot size as a function of this ratio. Because the power transmitted by the focusing optic also depends upon the truncation ratio, the optimal balance between spot size and power transmission will depend upon the given application.
For each focusing objective that Thorlabs provides, we provide an estimate of the focused spot size when the incident Gaussian spot size (1/e^{2}) is the same as the diameter of the entrance pupil. With this choice, the focused spot size is given by:
s ≈ 1.83λN, or equivalently, s ≈ 1.83λ/(2*NA), where NA is the numerical aperture of the objective; and the transmitted power is 86% of that of the incident beam.
Gaussian Beam Profile
Laser beams typically have a tranverse intensity profile that may be approximated by a Gaussian function,
,
where w is the beam halfwidth or beam waist radius, conventionally defined as the radius (r) at which the intensity has decreased from its maximum axial value of I_{0} to I_{0}/e^{2} ≈ 0.14I_{0}. The spot size of a laser beam may be defined as twice the beam waist radius, and the corresponding circle with diameter equal to the spot size thus contains 86% of the beam's total intensity.
When a laser beam is focused by an objective, the resulting spot size (s) will depend upon the wavelength of the light (λ), the beam diameter as it enters the objective (S), the focal length of the objective (f), and the entrance pupil diameter of the objective (D). Dimensionless parameters are formed by taking the ratio of the focal length to the entrance pupil diameter and the ratio of the beam diameter to the entrance pupil diameter, which are known respectively as the fnumber (N = f/D) and the truncation ratio (T = S/D). The fnumber is fixed for a given objective, while the truncation ratio may be tuned by increasing or decreasing the incident beam diameter.
Spot Size vs. Truncation Ratio
The focused spot size is expressed in terms of the wavelength, truncation ratio, and fnumber as
where K(T) is called the spot size coefficient and is a function of the truncation ratio [1]. In Figure 2 below, numerically computed values for K, obtained by calculating the focused intensity profile and extracting the focused spot size for discrete values of T, are plotted as black squares. As discussed in detail below, the solidanddashed blue line represents the coefficient predicted by Gaussian beam theory, the gray line represents the value of K for an Airy disk intensity profile, and the red line is a polynomial fit to the numerical values for T ≥ 0.5.
Figure 2: The shaded blue region below T < 0.5 indicates where Gaussian beam theory provides an accurate estimate of the focused spot size; however, above this value the effects of truncation cannot be neglected and the actual spot size is larger. As T → ∞, the coefficient approaches the Airy disk value of 1.6449 as indicated by the solid gray line.
Figure 3: The power transmitted through an entrance aperture of diameter D by a Gaussian beam with spot size S as a function of the truncation ratio T = S/D. The shaded blue region corresponds to the region where truncation effects on the spot size are negligible.
In both the large (T → ∞) and small (T → 0) limits, K approaches wellknown theoretical results. For small T, which corresponds to an entrance pupil much larger than the Gaussian spot, K obeys the relation 1.27/T. This can be obtained from Gaussian beam propagation theory [2] which predicts that the minimum spot size a Gaussian beam can be focused to is s ≈ 1.27λf/S. By inserting factors of D to write this in terms of N and T, this expression can be cast into the same form as the spot size equation above, s = (1.27/T)λN, giving the result K = 1.27/T. As seen in Figure 2 above, this accurately predicts the focused spot size up to T ≈ 0.5, when the entrance pupil diameter D is twice as large as the spot size S. Above T = 0.5, it underestimates the value of K, as indicated by the deviation of the dashed blue line from the numerical results.
Figure 4: The spot size of an Airy disk profile is typically defined by the radius where the first intensity zero occurs. When the radius is expressed in units of λN, this corresponds to a radius of 1.22λN, or a spot size of 2.44λN. The 1/e^{2} radius for the same profile is 0.82245λN, or a spot size of 1.6449λN.
As T is increased, the illumination of the aperture becomes more and more uniform. The resulting intensity profile of the focused spot will therefore transition from a Gaussian profile to an Airy disk profile. In the large T limit, this is reflected in the value of K, which approaches a constant value of 1.6449 as T → ∞. This value corresponds to the 1/e^{2} spot size of an Airy disk instead of the betterknown 2.44λN value which is where the first intensity minimum occurs, as shown in Figure 4 [3].
For intermediate values of T, which is the range in which most applications will fall, there is no exact theoretical result for K. Instead, the red line above represents a twoterm polynomial fit to the numerical results, the coefficients of which are specified in the table below (the polynomial fit was performed using 1/T as the independent variable). This expression may be used to estimate K for T ≥ 0.5.
Spot Size Coefficient, K(T)  

Truncation Ratio  Equation 
T < 0.5 (Gaussian Regime) 

T ≥ 0.5 (Intermediate and Uniform/Airy Regimes) 
Power Transmission and Spot Size
The results presented above suggest that, in the intermediate T regime, a smaller spot size may be achieved by increasing T. This, however, comes at the cost of reducing the overall power transmitted through the entrance aperture, and reductions in spot size may not be worth the loss in power. The power transmitted through an entrance pupil of diameter D as a function of T is plotted above in Figure 3. Already at T = 1, when the Gaussian spot size has the same diameter as the entrance pupil, the transmitted power is 86% of the incident power. By increasing T from 1 to 2, the spot size is reduced by only ≈ 9%, while the transmitted power decreases from 86% to 40%.
The optimal balance between spot size and power transmission will depend upon the given application. For each focusing objective that Thorlabs offers, we provide an estimate of the spot size using T = 1, when the Gaussian spot size is the same as the diameter of the entrance pupil. With this choice, the spot size is given by: s ≈ 1.83λN, or equivalently, s ≈ 1.83λ/(2*NA), where NA is the numerical aperture of the objective.
References
[1] Hakan Urey, "Spot size, depthoffocus, and diffraction ring intensity formulas for truncated Gaussian beams," Appl. Opt. 43, 620625 (2004)
[2] Sidney A. Self, "Focusing of spherical Gaussian beams," Appl. Opt. 22, 658661 (1983)
[3] Eugene Hecht, "Optics," 4th Ed., AddisonWesley (2002)
Damage Threshold Specifications  

Item # Suffix  Damage Threshold 
532  15 J/cm^{2} (532 nm, 20 Hz, 10 ns, Ø213 µm) 
850  20 J/cm^{2} (850 nm, 10 Hz, 10 ns, Ø300 µm) 
1064  20 J/cm^{2} (1064 nm, 20 Hz, 10 ns, Ø395 µm) 
Damage Threshold Data for HighPower Focusing Objectives AR Coatings
The specifications to the right are measured data for the antireflective (AR) coatings deposited onto the optical surface of our high power focusing objectives. Damage threshold specifications are constant for a given coating type, regardless of the focal length or magnification.
Laser Induced Damage Threshold Tutorial
The following is a general overview of how laser induced damage thresholds are measured and how the values may be utilized in determining the appropriateness of an optic for a given application. When choosing optics, it is important to understand the Laser Induced Damage Threshold (LIDT) of the optics being used. The LIDT for an optic greatly depends on the type of laser you are using. Continuous wave (CW) lasers typically cause damage from thermal effects (absorption either in the coating or in the substrate). Pulsed lasers, on the other hand, often strip electrons from the lattice structure of an optic before causing thermal damage. Note that the guideline presented here assumes room temperature operation and optics in new condition (i.e., within scratchdig spec, surface free of contamination, etc.). Because dust or other particles on the surface of an optic can cause damage at lower thresholds, we recommend keeping surfaces clean and free of debris. For more information on cleaning optics, please see our Optics Cleaning tutorial.
Testing Method
Thorlabs' LIDT testing is done in compliance with ISO/DIS 11254 and ISO 21254 specifications.
First, a lowpower/energy beam is directed to the optic under test. The optic is exposed in 10 locations to this laser beam for 30 seconds (CW) or for a number of pulses (pulse repetition frequency specified). After exposure, the optic is examined by a microscope (~100X magnification) for any visible damage. The number of locations that are damaged at a particular power/energy level is recorded. Next, the power/energy is either increased or decreased and the optic is exposed at 10 new locations. This process is repeated until damage is observed. The damage threshold is then assigned to be the highest power/energy that the optic can withstand without causing damage. A histogram such as that below represents the testing of one BB1E02 mirror.
The photograph above is a protected aluminumcoated mirror after LIDT testing. In this particular test, it handled 0.43 J/cm^{2} (1064 nm, 10 ns pulse, 10 Hz, Ø1.000 mm) before damage.
Example Test Data  

Fluence  # of Tested Locations  Locations with Damage  Locations Without Damage 
1.50 J/cm^{2}  10  0  10 
1.75 J/cm^{2}  10  0  10 
2.00 J/cm^{2}  10  0  10 
2.25 J/cm^{2}  10  1  9 
3.00 J/cm^{2}  10  1  9 
5.00 J/cm^{2}  10  9  1 
According to the test, the damage threshold of the mirror was 2.00 J/cm^{2} (532 nm, 10 ns pulse, 10 Hz, Ø0.803 mm). Please keep in mind that these tests are performed on clean optics, as dirt and contamination can significantly lower the damage threshold of a component. While the test results are only representative of one coating run, Thorlabs specifies damage threshold values that account for coating variances.
Continuous Wave and LongPulse Lasers
When an optic is damaged by a continuous wave (CW) laser, it is usually due to the melting of the surface as a result of absorbing the laser's energy or damage to the optical coating (antireflection) [1]. Pulsed lasers with pulse lengths longer than 1 µs can be treated as CW lasers for LIDT discussions.
When pulse lengths are between 1 ns and 1 µs, laserinduced damage can occur either because of absorption or a dielectric breakdown (therefore, a user must check both CW and pulsed LIDT). Absorption is either due to an intrinsic property of the optic or due to surface irregularities; thus LIDT values are only valid for optics meeting or exceeding the surface quality specifications given by a manufacturer. While many optics can handle high power CW lasers, cemented (e.g., achromatic doublets) or highly absorptive (e.g., ND filters) optics tend to have lower CW damage thresholds. These lower thresholds are due to absorption or scattering in the cement or metal coating.
Pulsed lasers with high pulse repetition frequencies (PRF) may behave similarly to CW beams. Unfortunately, this is highly dependent on factors such as absorption and thermal diffusivity, so there is no reliable method for determining when a high PRF laser will damage an optic due to thermal effects. For beams with a high PRF both the average and peak powers must be compared to the equivalent CW power. Additionally, for highly transparent materials, there is little to no drop in the LIDT with increasing PRF.
In order to use the specified CW damage threshold of an optic, it is necessary to know the following:
 Wavelength of your laser
 Beam diameter of your beam (1/e^{2})
 Approximate intensity profile of your beam (e.g., Gaussian)
 Linear power density of your beam (total power divided by 1/e^{2} beam diameter)
Thorlabs expresses LIDT for CW lasers as a linear power density measured in W/cm. In this regime, the LIDT given as a linear power density can be applied to any beam diameter; one does not need to compute an adjusted LIDT to adjust for changes in spot size, as demonstrated by the graph to the right. Average linear power density can be calculated using the equation below.
The calculation above assumes a uniform beam intensity profile. You must now consider hotspots in the beam or other nonuniform intensity profiles and roughly calculate a maximum power density. For reference, a Gaussian beam typically has a maximum power density that is twice that of the uniform beam (see lower right).
Now compare the maximum power density to that which is specified as the LIDT for the optic. If the optic was tested at a wavelength other than your operating wavelength, the damage threshold must be scaled appropriately. A good rule of thumb is that the damage threshold has a linear relationship with wavelength such that as you move to shorter wavelengths, the damage threshold decreases (i.e., a LIDT of 10 W/cm at 1310 nm scales to 5 W/cm at 655 nm):
While this rule of thumb provides a general trend, it is not a quantitative analysis of LIDT vs wavelength. In CW applications, for instance, damage scales more strongly with absorption in the coating and substrate, which does not necessarily scale well with wavelength. While the above procedure provides a good rule of thumb for LIDT values, please contact Tech Support if your wavelength is different from the specified LIDT wavelength. If your power density is less than the adjusted LIDT of the optic, then the optic should work for your application.
Please note that we have a buffer built in between the specified damage thresholds online and the tests which we have done, which accommodates variation between batches. Upon request, we can provide individual test information and a testing certificate. The damage analysis will be carried out on a similar optic (customer's optic will not be damaged). Testing may result in additional costs or lead times. Contact Tech Support for more information.
Pulsed Lasers
As previously stated, pulsed lasers typically induce a different type of damage to the optic than CW lasers. Pulsed lasers often do not heat the optic enough to damage it; instead, pulsed lasers produce strong electric fields capable of inducing dielectric breakdown in the material. Unfortunately, it can be very difficult to compare the LIDT specification of an optic to your laser. There are multiple regimes in which a pulsed laser can damage an optic and this is based on the laser's pulse length. The highlighted columns in the table below outline the relevant pulse lengths for our specified LIDT values.
Pulses shorter than 10^{9} s cannot be compared to our specified LIDT values with much reliability. In this ultrashortpulse regime various mechanics, such as multiphotonavalanche ionization, take over as the predominate damage mechanism [2]. In contrast, pulses between 10^{7} s and 10^{4} s may cause damage to an optic either because of dielectric breakdown or thermal effects. This means that both CW and pulsed damage thresholds must be compared to the laser beam to determine whether the optic is suitable for your application.
Pulse Duration  t < 10^{9} s  10^{9} < t < 10^{7} s  10^{7} < t < 10^{4} s  t > 10^{4} s 

Damage Mechanism  Avalanche Ionization  Dielectric Breakdown  Dielectric Breakdown or Thermal  Thermal 
Relevant Damage Specification  No Comparison (See Above)  Pulsed  Pulsed and CW  CW 
When comparing an LIDT specified for a pulsed laser to your laser, it is essential to know the following:
 Wavelength of your laser
 Energy density of your beam (total energy divided by 1/e^{2} area)
 Pulse length of your laser
 Pulse repetition frequency (prf) of your laser
 Beam diameter of your laser (1/e^{2} )
 Approximate intensity profile of your beam (e.g., Gaussian)
The energy density of your beam should be calculated in terms of J/cm^{2}. The graph to the right shows why expressing the LIDT as an energy density provides the best metric for short pulse sources. In this regime, the LIDT given as an energy density can be applied to any beam diameter; one does not need to compute an adjusted LIDT to adjust for changes in spot size. This calculation assumes a uniform beam intensity profile. You must now adjust this energy density to account for hotspots or other nonuniform intensity profiles and roughly calculate a maximum energy density. For reference a Gaussian beam typically has a maximum energy density that is twice that of the 1/e^{2} beam.
Now compare the maximum energy density to that which is specified as the LIDT for the optic. If the optic was tested at a wavelength other than your operating wavelength, the damage threshold must be scaled appropriately [3]. A good rule of thumb is that the damage threshold has an inverse square root relationship with wavelength such that as you move to shorter wavelengths, the damage threshold decreases (i.e., a LIDT of 1 J/cm^{2} at 1064 nm scales to 0.7 J/cm^{2} at 532 nm):
You now have a wavelengthadjusted energy density, which you will use in the following step.
Beam diameter is also important to know when comparing damage thresholds. While the LIDT, when expressed in units of J/cm², scales independently of spot size; large beam sizes are more likely to illuminate a larger number of defects which can lead to greater variances in the LIDT [4]. For data presented here, a <1 mm beam size was used to measure the LIDT. For beams sizes greater than 5 mm, the LIDT (J/cm2) will not scale independently of beam diameter due to the larger size beam exposing more defects.
The pulse length must now be compensated for. The longer the pulse duration, the more energy the optic can handle. For pulse widths between 1  100 ns, an approximation is as follows:
Use this formula to calculate the Adjusted LIDT for an optic based on your pulse length. If your maximum energy density is less than this adjusted LIDT maximum energy density, then the optic should be suitable for your application. Keep in mind that this calculation is only used for pulses between 10^{9} s and 10^{7} s. For pulses between 10^{7} s and 10^{4} s, the CW LIDT must also be checked before deeming the optic appropriate for your application.
Please note that we have a buffer built in between the specified damage thresholds online and the tests which we have done, which accommodates variation between batches. Upon request, we can provide individual test information and a testing certificate. Contact Tech Support for more information.
[1] R. M. Wood, Optics and Laser Tech. 29, 517 (1998).
[2] Roger M. Wood, LaserInduced Damage of Optical Materials (Institute of Physics Publishing, Philadelphia, PA, 2003).
[3] C. W. Carr et al., Phys. Rev. Lett. 91, 127402 (2003).
[4] N. Bloembergen, Appl. Opt. 12, 661 (1973).
In order to illustrate the process of determining whether a given laser system will damage an optic, a number of example calculations of laser induced damage threshold are given below. For assistance with performing similar calculations, we provide a spreadsheet calculator that can be downloaded by clicking the button to the right. To use the calculator, enter the specified LIDT value of the optic under consideration and the relevant parameters of your laser system in the green boxes. The spreadsheet will then calculate a linear power density for CW and pulsed systems, as well as an energy density value for pulsed systems. These values are used to calculate adjusted, scaled LIDT values for the optics based on accepted scaling laws. This calculator assumes a Gaussian beam profile, so a correction factor must be introduced for other beam shapes (uniform, etc.). The LIDT scaling laws are determined from empirical relationships; their accuracy is not guaranteed. Remember that absorption by optics or coatings can significantly reduce LIDT in some spectral regions. These LIDT values are not valid for ultrashort pulses less than one nanosecond in duration.
A Gaussian beam profile has about twice the maximum intensity of a uniform beam profile.
CW Laser Example
Suppose that a CW laser system at 1319 nm produces a 0.5 W Gaussian beam that has a 1/e^{2} diameter of 10 mm. A naive calculation of the average linear power density of this beam would yield a value of 0.5 W/cm, given by the total power divided by the beam diameter:
However, the maximum power density of a Gaussian beam is about twice the maximum power density of a uniform beam, as shown in the graph to the right. Therefore, a more accurate determination of the maximum linear power density of the system is 1 W/cm.
An AC127030C achromatic doublet lens has a specified CW LIDT of 350 W/cm, as tested at 1550 nm. CW damage threshold values typically scale directly with the wavelength of the laser source, so this yields an adjusted LIDT value:
The adjusted LIDT value of 350 W/cm x (1319 nm / 1550 nm) = 298 W/cm is significantly higher than the calculated maximum linear power density of the laser system, so it would be safe to use this doublet lens for this application.
Pulsed Nanosecond Laser Example: Scaling for Different Pulse Durations
Suppose that a pulsed Nd:YAG laser system is frequency tripled to produce a 10 Hz output, consisting of 2 ns output pulses at 355 nm, each with 1 J of energy, in a Gaussian beam with a 1.9 cm beam diameter (1/e^{2}). The average energy density of each pulse is found by dividing the pulse energy by the beam area:
As described above, the maximum energy density of a Gaussian beam is about twice the average energy density. So, the maximum energy density of this beam is ~0.7 J/cm^{2}.
The energy density of the beam can be compared to the LIDT values of 1 J/cm^{2} and 3.5 J/cm^{2} for a BB1E01 broadband dielectric mirror and an NB1K08 Nd:YAG laser line mirror, respectively. Both of these LIDT values, while measured at 355 nm, were determined with a 10 ns pulsed laser at 10 Hz. Therefore, an adjustment must be applied for the shorter pulse duration of the system under consideration. As described on the previous tab, LIDT values in the nanosecond pulse regime scale with the square root of the laser pulse duration:
This adjustment factor results in LIDT values of 0.45 J/cm^{2} for the BB1E01 broadband mirror and 1.6 J/cm^{2} for the Nd:YAG laser line mirror, which are to be compared with the 0.7 J/cm^{2} maximum energy density of the beam. While the broadband mirror would likely be damaged by the laser, the more specialized laser line mirror is appropriate for use with this system.
Pulsed Nanosecond Laser Example: Scaling for Different Wavelengths
Suppose that a pulsed laser system emits 10 ns pulses at 2.5 Hz, each with 100 mJ of energy at 1064 nm in a 16 mm diameter beam (1/e^{2}) that must be attenuated with a neutral density filter. For a Gaussian output, these specifications result in a maximum energy density of 0.1 J/cm^{2}. The damage threshold of an NDUV10A Ø25 mm, OD 1.0, reflective neutral density filter is 0.05 J/cm^{2} for 10 ns pulses at 355 nm, while the damage threshold of the similar NE10A absorptive filter is 10 J/cm^{2} for 10 ns pulses at 532 nm. As described on the previous tab, the LIDT value of an optic scales with the square root of the wavelength in the nanosecond pulse regime:
This scaling gives adjusted LIDT values of 0.08 J/cm^{2} for the reflective filter and 14 J/cm^{2} for the absorptive filter. In this case, the absorptive filter is the best choice in order to avoid optical damage.
Pulsed Microsecond Laser Example
Consider a laser system that produces 1 µs pulses, each containing 150 µJ of energy at a repetition rate of 50 kHz, resulting in a relatively high duty cycle of 5%. This system falls somewhere between the regimes of CW and pulsed laser induced damage, and could potentially damage an optic by mechanisms associated with either regime. As a result, both CW and pulsed LIDT values must be compared to the properties of the laser system to ensure safe operation.
If this relatively longpulse laser emits a Gaussian 12.7 mm diameter beam (1/e^{2}) at 980 nm, then the resulting output has a linear power density of 5.9 W/cm and an energy density of 1.2 x 10^{4} J/cm^{2} per pulse. This can be compared to the LIDT values for a WPQ10E980 polymer zeroorder quarterwave plate, which are 5 W/cm for CW radiation at 810 nm and 5 J/cm^{2} for a 10 ns pulse at 810 nm. As before, the CW LIDT of the optic scales linearly with the laser wavelength, resulting in an adjusted CW value of 6 W/cm at 980 nm. On the other hand, the pulsed LIDT scales with the square root of the laser wavelength and the square root of the pulse duration, resulting in an adjusted value of 55 J/cm^{2} for a 1 µs pulse at 980 nm. The pulsed LIDT of the optic is significantly greater than the energy density of the laser pulse, so individual pulses will not damage the wave plate. However, the large average linear power density of the laser system may cause thermal damage to the optic, much like a highpower CW beam.
Laser Safety and Classification
Safe practices and proper usage of safety equipment should be taken into consideration when operating lasers. The eye is susceptible to injury, even from very low levels of laser light. Thorlabs offers a range of laser safety accessories that can be used to reduce the risk of accidents or injuries. Laser emission in the visible and near infrared spectral ranges has the greatest potential for retinal injury, as the cornea and lens are transparent to those wavelengths, and the lens can focus the laser energy onto the retina.
Safe Practices and Light Safety Accessories
 Laser safety eyewear must be worn whenever working with Class 3 or 4 lasers.
 Regardless of laser class, Thorlabs recommends the use of laser safety eyewear whenever working with laser beams with nonnegligible powers, since metallic tools such as screwdrivers can accidentally redirect a beam.
 Laser goggles designed for specific wavelengths should be clearly available near laser setups to protect the wearer from unintentional laser reflections.
 Goggles are marked with the wavelength range over which protection is afforded and the minimum optical density within that range.
 Laser Safety Curtains and Laser Safety Fabric shield other parts of the lab from high energy lasers.
 Blackout Materials can prevent direct or reflected light from leaving the experimental setup area.
 Thorlabs' Enclosure Systems can be used to contain optical setups to isolate or minimize laser hazards.
 A fiberpigtailed laser should always be turned off before connecting it to or disconnecting it from another fiber, especially when the laser is at power levels above 10 mW.
 All beams should be terminated at the edge of the table, and laboratory doors should be closed whenever a laser is in use.
 Do not place laser beams at eye level.
 Carry out experiments on an optical table such that all laser beams travel horizontally.
 Remove unnecessary reflective items such as reflective jewelry (e.g., rings, watches, etc.) while working near the beam path.
 Be aware that lenses and other optical devices may reflect a portion of the incident beam from the front or rear surface.
 Operate a laser at the minimum power necessary for any operation.
 If possible, reduce the output power of a laser during alignment procedures.
 Use beam shutters and filters to reduce the beam power.
 Post appropriate warning signs or labels near laser setups or rooms.
 Use a laser sign with a lightbox if operating Class 3R or 4 lasers (i.e., lasers requiring the use of a safety interlock).
 Do not use Laser Viewing Cards in place of a proper Beam Trap.
Laser Classification
Lasers are categorized into different classes according to their ability to cause eye and other damage. The International Electrotechnical Commission (IEC) is a global organization that prepares and publishes international standards for all electrical, electronic, and related technologies. The IEC document 608251 outlines the safety of laser products. A description of each class of laser is given below:
Class  Description  Warning Label 

1  This class of laser is safe under all conditions of normal use, including use with optical instruments for intrabeam viewing. Lasers in this class do not emit radiation at levels that may cause injury during normal operation, and therefore the maximum permissible exposure (MPE) cannot be exceeded. Class 1 lasers can also include enclosed, highpower lasers where exposure to the radiation is not possible without opening or shutting down the laser.  
1M  Class 1M lasers are safe except when used in conjunction with optical components such as telescopes and microscopes. Lasers belonging to this class emit largediameter or divergent beams, and the MPE cannot normally be exceeded unless focusing or imaging optics are used to narrow the beam. However, if the beam is refocused, the hazard may be increased and the class may be changed accordingly.  
2  Class 2 lasers, which are limited to 1 mW of visible continuouswave radiation, are safe because the blink reflex will limit the exposure in the eye to 0.25 seconds. This category only applies to visible radiation (400  700 nm).  
2M  Because of the blink reflex, this class of laser is classified as safe as long as the beam is not viewed through optical instruments. This laser class also applies to largerdiameter or diverging laser beams.  
3R  Class 3R lasers produce visible and invisible light that is hazardous under direct and specularreflection viewing conditions. Eye injuries may occur if you directly view the beam, especially when using optical instruments. Lasers in this class are considered safe as long as they are handled with restricted beam viewing. The MPE can be exceeded with this class of laser; however, this presents a low risk level to injury. Visible, continuouswave lasers in this class are limited to 5 mW of output power.  
3B  Class 3B lasers are hazardous to the eye if exposed directly. Diffuse reflections are usually not harmful, but may be when using higherpower Class 3B lasers. Safe handling of devices in this class includes wearing protective eyewear where direct viewing of the laser beam may occur. Lasers of this class must be equipped with a key switch and a safety interlock; moreover, laser safety signs should be used, such that the laser cannot be used without the safety light turning on. Laser products with power output near the upper range of Class 3B may also cause skin burns.  
4  This class of laser may cause damage to the skin, and also to the eye, even from the viewing of diffuse reflections. These hazards may also apply to indirect or nonspecular reflections of the beam, even from apparently matte surfaces. Great care must be taken when handling these lasers. They also represent a fire risk, because they may ignite combustible material. Class 4 lasers must be equipped with a key switch and a safety interlock.  
All class 2 lasers (and higher) must display, in addition to the corresponding sign above, this triangular warning sign. 
Thorlabs offers a wide selection of optics optimized for use with Nd:YAG lasers. Please see below for more information.
Nd:YAG Optics Selection  

Dielectric Mirrors  Ultrafast Mirrors  
Laser Line Mirrors, 1064 nm, 532 nm, 355 nm, 266 nm 
RightAngle Prism Mirrors, 1064 nm, 532 nm 
Cage CubeMounted Prism Mirrors, 1064 nm, 532 nm 
Low GDD Ultrafast Mirrors, 1064 nm or 532 nm 
Beamsplitters  Objectives  
Harmonic Beamsplitters, 1064 nm, 532 nm, 355 nm, 266 nm 
HighPower Polarizing Beamsplitter Cubes, 1064 nm, 532 nm: Unmounted or Mounted  NonPolarizing Plate Beamsplitters, 1064 nm, 532 nm  High Power Focusing Objectives, 1064 nm, 532 nm 
Lenses  Filters  
UVFS PlanoConvex Lenses: 532 nm/1064 nm: Unmounted or Mounted 532 nm: Unmounted 1064 nm: Unmounted 
AirSpaced Doublets, 1064 nm, 532 nm 
Laser Line Filters, 1064 nm: Standard or Premium 
Laser Line Filters, 532 nm: Standard or Premium 
Posted Comments:  
Manon Lallement
(posted 20231011 21:18:53.443) Hello,
Could you please share the reversed Zemax black box of LMH5X1064?
Best regards,
Manon Lallement srydberg
(posted 20231012 10:18:33.0) Hello, thank you for contacting Thorlabs! It is possible to reverse files containing black boxes in newer versions of Zemax. I have contacted you directly and sent you the requested file. Cristina Mendez
(posted 20190614 04:14:36.25) Good morning, we're using this objective both for a 1064nm laser and a 1038 nm fslaser; and we're interesting in how its focusing distance varies with the wavelength. Do you have any data on this matter? mdiekmann
(posted 20190619 09:45:45.0) Hello, thank you for contacting Thorlabs. We will contact you directly and will send the requested information. asalvador
(posted 20181114 13:40:43.497) Good afternoon, I'd like some advice to build a dicing system for Silicon wafers of 700 micron thickness, with internal micro cracking. We already have the sample XY scanning system and looking forward to buy a laser (need advice on models) and optics (focusing objectives, etc) YLohia
(posted 20181114 08:53:17.0) Hello, thank you for contacting Thorlabs. We will reach out to you directly to discuss your application. jaka.mur
(posted 20180425 12:04:06.603) I would like to know some details about the LMH5X1064 objective:
1) How was the "Diffractionlimited Spot Size" value calculated? I have tried using this: diameter = 4*lambda*EFL/pi/EA and it does not result in the same number.
2) What is the actual field of view with this objective?
3) Is there a measurement of CW damage threshold available?
Best regards,
Jaka nbayconich
(posted 20180426 03:19:35.0) Thank you for your feedback. The diffraction limited spot Size calculated for this objective will produce a spot size given by
Ø=C x λ x (f/A)
Where Ø is the 1/e2 beam diameter, λ is the wavelength of the laser, f is the effective focal length of the lens, and A is the entrance beam diameter. C is a constant that relates to the degree of pupil illumination and input truncation (for a Gaussian beam, C = 1.83 when the entrance beam is truncated at the 1/e2 diameter).
The field of view is the OFN/magnification = 2.4mm.
We do not have a certified damage threshold CW measurement at the moment, however we expect it to 1MW/cm². p.kleingarn
(posted 20171128 11:53:28.36) I've got a question regarding the LMH10x532nm Objective.
I'm working with the optical Breakdown in borosilikatglas and i'm wondering how the spherical Abberations would influence my results.
Can you give me any information about the wavefront abberation coefficient/transmitted wavefront error maybe?
This would be very appreciated, thanks !
besten regards
Philipp tfrisch
(posted 20180223 10:18:20.0) Hello, thank you for contacting Thorlabs. I can send you the Zemax files we have available if you need to do a rigorous analysis, but LMH10X532 has onaxis nominal a diffraction limited transmitted wavefront error for borosilicate glass up to 1mm when the coverglass is perpendicular to the objective axis. I will reach out to you to directly to discuss this. linlinchiayu
(posted 20170704 22:05:00.537) Can I receive the wavelength range information of LMH20X1064 and LMH10X1064? nbayconich
(posted 20170711 10:58:47.0) Thank you for contacting Thorlabs. I will reach out to you directly with more information on the transmission of LMH20X1064 and LMH10X1064. marin.vojkovic
(posted 20170627 10:46:21.98) Can you please tell me what coating is used for the objective and if it is suitable for working in the vacuum? If not, what would the price be for an objective suitable for vacuum?
By coating, I mean the whole objective, not just the lens.
Thank you in advance! tfrisch
(posted 20170803 11:31:47.0) Hello, thank you for contacting Thorlabs. We can offer a custom vacuum compatible version. I will reach out to you directly. jelke.wibbeke
(posted 20161010 09:57:25.37) We are using the LMH5X1064 on a femtosecond laser. It occours that we can find two more focus spots (with less intensity) symmetrically about 2mm to the left and the right of the actual focus spot. Any clue? jlow
(posted 20161010 11:13:42.0) Response from Jeremy at Thorlabs: We will contact you directly about troubleshooting this. erica.block
(posted 20160729 13:30:02.18) Could you make one of these high power MicroSpot focusing objectives with a 850nm AR coating? o.soroka
(posted 20151118 13:41:26.86) Can this objective be used in the UHV? besembeson
(posted 20151120 09:34:48.0) Response from Bweh at Thorlabs USA: The stock item like the LMH5X532 is not vacuum compatible as there are certain airpockets and anodized components inside that will outgas. We can provide a special vacuum compatible version that may be suitable for your application. I will contact you. andrefilipedrosa
(posted 20150714 19:58:24.633) Hello, is this objective lens able to be scanned? ty besembeson
(posted 20150923 12:03:35.0) Response from Bweh at Thorlabs USA: The design is not telecentric and the clear aperture may not be large enough so this will not be suitable for scanning applications. You can find several scanning objectives at the following link: http://www.thorlabs.com/NewGroupPage9.cfm?ObjectGroup_ID=2910 suwas.nikumb
(posted 20140210 09:37:53.92) Do you have microscope objectives at 532nm and 800nm with atleast 1215mm entrance aperture? besembeson
(posted 20140212 01:59:58.0) Response from Bweh E. at Thorlabs: Thanks for contacting Thorlabs. At this time, we do not carry such objectives that meet your requirements. We however have several other objectives at the following page: http://www.thorlabs.com/newgrouppage9.cfm?objectgroup_id=1044. lvtaohn
(posted 20130917 19:08:25.967) Do you have 40times or 60 times high power focusing objective 1064nm or 532nm? I need them in these days. Please let me know if you have them. Thank you! jlow
(posted 20130919 14:09:00.0) Response from Jeremy at Thorlabs: We do not currently have these short focal length objectives for high power application. I have logged this in our internal forum and we will look into whether we could make this. rpscott
(posted 20130529 17:06:42.537) Is the transmission for the 1064nm version of the objectives similar at 1037nm? tcohen
(posted 20130530 02:28:00.0) Response from Tim at Thorlabs: Yes. The number of surfaces in each objective is different and therefore deviation away from the design wavelength will have more of an impact on transmission for the 20X vs the 10X, for example. However, at your desired wavelength the total transmission for each is similar. tcohen
(posted 20120823 16:25:00.0) Response from Tim at Thorlabs: Thank you for contacting us. I’ve emailed you to go over this objective and supply some representative data. song31037
(posted 20120823 15:19:04.0) Can I receive the wavelength range information of LMH20X1064? tcohen
(posted 20120229 15:56:00.0) Response from Tim at Thorlabs: Thank you for your feedback on the LMH10X532. I am looking into the materials we use for this objective and will post an update soon. g.laliberte
(posted 20120229 10:13:58.0) I'm intersted in a microscope objective that would be made of non magnetic material. Do you have any data about the housing material of that lens?
THanks jjurado
(posted 20110708 08:58:00.0) Response from Javier at Thorlabs to last poster: Thank you very much for contacting us. For this objective, the absorption in the glass itself is almost negligible, and if we assume 3.5% loss at each surface we would end up with a total transmission in the neighborhood of 80%. However, keep in mind that the chromatic shift of roughly 0.2 mm will slightly affect the performance of this objective. Also, we do not currently have an objective specifically designed for operation at 980 and 1550 nm. Please contact us at techsupport@thorlabs.com if you would like to discuss your application a bit further. user
(posted 20110707 14:17:40.0) I am working with this objective (LMH10X1064), but I have beam at 1550nm. So I want to know the transmission spectrum of this objective especialy for 1550nm). Is there any particular objective design to work at 980nm and 1550nm? apalmentieri
(posted 20091231 17:12:33.0) A response from Adam at Thorlabs to Ilday: There was a server glitch and we are working to bring this page online. Please note that we do have stock on most of these objectives and they can be ordered direct through our sales department, sales@thorlabs.com or 9733003000, while these parts are not on the website. I will email you with more information. ilday
(posted 20091231 17:01:39.0) I wanted to purchase this product, which was available until yesterday, however it has disappeared from the webpage. Is that a server glitch or did you discontinue the product? 
Item #  AR Coating Range 
Transmission (Typical)^{a} 
M^{b}  WD  EFL  PFL  NA  EP^{c}  OFN  Spot Size^{d}  Design Tube Lens Focal Length^{e} 
Cover Glass Correction 
RMS Thread Depth 

LMH5X532  495  570 nm  >98%  5X  35 mm  40 mm  58.9 mm  0.13  9.9 mm  12  3.9 µm  200 mm    3.8 mm 
LMH10X532  >97%  10X  15 mm  20 mm  38.9 mm  0.25  9.9 mm  8  2.0 µm  
LMH20X532  >96%  20X  6 mm  10 mm  40.0 mm  0.40  8.0 mm  14  1.2 µm  
LMH50X532  >95%  50X  2.5 mm^{f}  4 mm  45.0 mm^{f}  0.60  5.0 mm  22  0.8 µm  0.0  1.0 mm of Fused Silica  4.5 mm 
Item #  AR Coating Range 
Transmission (Typical)^{a} 
M^{b}  WD  EFL  PFL  NA  EP^{c}  OFN  Spot Size^{d}  Design Tube Lens Focal Length^{e} 
Cover Glass Correction 
RMS Thread Depth 

LMH50X850  790  910 nm  >95%  50X  2.3 mm^{f}  4 mm  45.0 mm^{f}  0.65  5.3 mm  22  1.2 µm  200 mm  0.0  1.0 mm of Fused Silica  4.5 mm 
Item #  AR Coating Range 
Transmission (Typical)^{a} 
M^{b}  WD  EFL  PFL  NA  EP^{c}  OFN  Spot Size^{d}  Design Tube Lens Focal Length^{e} 
Cover Glass Correction 
RMS Thread Depth 

LMH5X1064  980  1130 nm  >98%  5X  35 mm  40 mm  58.9 mm  0.13  9.9 mm  12  7.9 µm  200 mm    3.8 mm 
LMH10X1064  >97%  10X  15 mm  20 mm  38.9 mm  0.25  9.9 mm  10  3.9 µm  
LMH20X1064  >96%  20X  6 mm  10 mm  40.0 mm  0.40  8.0 mm  14  2.4 µm  
LMH50X1064  >95%  50X  2.3 mm^{f}  4 mm  45.0 mm^{f}  0.65  5.3 mm  22  1.5 µm  0.0  1.0 mm of Fused Silica 0.0  1.2 mm of SiC 
4.5 mm 