
iHR Series Spectrographs
Simply the Best Imaging Spectrometer with No Compromise
HORIBA’s most popular and iconic spectrometers, the iHR series build on decades of experience in spectroscopy and represent the highest quality, performance and versatility of any spectrometer in this class. The iHR 320 and iHR 550 spectrometers are immediately recognizable around the world by their unique shape, the result of a superior optical design. These spectrometers benefit from the highest quality of gratings, also designed and manufactured by HORIBA.
Two spectrometers to choose from

320 mm focal length f/4.1
550 mm focal length f/6.4
Best in class performance
- Widest range of applications
- Widest selection of options
- No re-diffracted light
- Fully automated
- Best in class resolution
- Best in class image quality
- Dual entrance & exit ports
Overview
- Unique optical design
Not all Czerny-Turner spectrometers are built the same
No one has more experience in designing and manufacturing spectrometers than HORIBA Scientific. When we designed the iHR we made a quantum leap forward in the traditional Czerny-Turner design and developed an asymmetrical spectrometer that is patented and immediately recognizable by its distinctive shape and design. With zero re-diffracted light, correction for optical aberrations, multi-track image capabilities and more options than any competitor, the iHR series offers best in class performance and flexibility.
For more details on the outstanding performance characteristics of this unique spectrometer, refer to our technical note, titled “Not all Czerny-Turner spectrometers are made the same”.
Inherent Benefits
iHR Series | Competition | iHR Benefits | ||
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Housing manufacture | Single Casting | Panels | Better stray light rejection | |
Size of entrance & exit swing away mirrors | Exit greater than entrance | Exit the same as entrance | No vignetting and homogeneous illumination of CCD | |
Non-crossed Czerny-Turner asymmetric optics | Yes | No | No re-diffracted light to present spurious signals | |
On-axis grating rotation with single motor triple grating turret | Yes | No | Patented design ensures uniform illumination | |
Dual entrance port | Yes | No | Flexibility | |
Dual exit port | Yes | No | Flexibility, no vignetting | |
Up to 4 single channel detectors or 2 single channel and one array | Yes | No | Flexibility and broad spectral coverage |
Hardware
The iHR series of spectrometers stand out in the field of standard Czerny-Turner spectrometers. They are manufactured from a single solid casting to eliminate light leaks and provide the strongest, most stable possible housing for the instrument. The computer optimized asymmetric optical path and patented on-axis grating drive improve image quality, while eliminating re-diffracted light and maximizing optical throughput. In addition, the use of toroidal mirrors corrects for astigmatism at the center of the focal plane, providing flexibility to work in either an imaging or resolution optimized configuration.
The iHR series spectrometers are fully automated; all motors are computer controlled including slits, gratings, turret rotation, and swing mirrors. There are four optional ports, two entrance and two exit, that can be utilized in any combination of two inputs and two outputs. The two optional output ports can be configured with either slits or array flanges for use with multichannel detectors.
Slits
The monochromator slits are adjustable automated slits with two available options; 0 to 2 mm opening with 2.25 micron step size and 0 to 7 mm opening with 6.25 micron step size. A manually adjustable height limiter allows the user to quickly shut or open the light path to 1 mm and 15 mm heights.
You can add accessories to the HR series spectrometers to obtain optimum results for a variety of applications. To attach the accessories to the iHR, use the two tapped holes on the body of the slit. These holes are also useful for connecting the iHR with your experiments and equipment. When connecting with the iHR, it is important to know the distance from the mounting face of the slit’s body to the slits.
Note that some custom accessories require removal of the height-limiter assembly in order to be attached to the iHR chassis. To remove the height-limiter assembly, remove the four screws holding the assembly onto the chassis.
Gratings
World Class Diffraction Gratings Manufactured by HORIBA
A Proud Tradition of Excellence
With the acquisition by HORIBA of Jobin Yvon, a spectroscopy company founded in 1819, HORIBA Scientific continues to define the leading edge of the Optics of Spectroscopy.
For the last 40 years HORIBA Scientific has taken a leading position in the design, development and manufacture of master and replica diffraction gratings. HORIBA Scientific diffraction gratings are found in both high volume OEM instruments and in world class cutting edge scientific applications. Our pattern of leadership in optics has been hallmarked by the continuing development of both classically ruled and holographic diffraction grating technologies. This led to the introduction in 1967 of the aberration corrected holographic grating and subsequently ion etched and blazed concave and plane holographic gratings.
The iHR series of spectrometers take full advantage of the highest quality of gratings that HORIBA designs and manufactures.
A Vast Array of Choices
There is a wide selection of gratings to choose from depending on optical requirements. Gratings are 68 x 68 mm for the iHR320 and 76 x 76 mm for the iHR550. There are three different types of gratings available; classically ruled, holographic, and blazed holographic.
Ruled gratings | Select for applications where high throughput or low groove density is required, or when working in the infrared. Typically, they have high throughput at the cost of higher stray light. |
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Holographic gratings | Available in higher groove densities for finer resolution requirements and are excellent choices for experiments with laser excitation such as Raman or laser induced photoluminescence. They provide the lowest possible stray light possible, sometimes at the cost of lower throughput. |
Blazed holographic gratings | These gratings have the same advantages as holographic gratings with better throughput. |
Groove Density
Ruled gratings and blazed holographic gratings have two fundamental parameters to choose from; the groove density, expressed in grooves (or lines) per millimeter, and the blaze angle which nominally refers to the peak reflectance wavelength expressed in nanometers.
The groove density of the selected grating affects the resolution and mechanical scanning range of the monochromator. Below is a reference chart showing the affect groove density has on the mechanical scanning range of the monochromator as well as the reciprocal linear dispersion of the slits.
Groove Density | Mechanical Scanning Range (nm)* | Reciprocal Linear Dispersion (nm/mm) | |
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iHR320 | iHR550 | ||
2,400 g/mm | 0 to 750 nm | 0.87 nm/mm | 0.53 nm/mm |
1,200 g/mm | 0 to 1,500 nm | 2.29 nm/mm | 1.34 nm/mm |
600 g/mm | 0 to 3,000 nm | 4.91 nm/mm | 2.83 nm/mm |
300 g/mm | 0 to 6,000 nm | 10.06 nm/mm | 5.75 nm/mm |
150 g/mm | 0 to 12,000 nm | 20.30 nm/mm | 11.58 nm/mm |
*High grating efficiency can be attained at up to 80% of the maximum mechanical scanning range, after which the grating efficiency decreases.
The triple grating turret that comes standard with the iHR series allows you to select three different gratings, to optimize throughput in different wavelength ranges and provide multiple options for different resolution requirements. The gratings are positioned in a patented on-axis turret design to provide the maximum possible mechanical tuning range while preventing beam walk-off. For even greater flexibility, the entire triple grating turret assembly can be easily and very quickly replaced with a different triple grating turret assembly, and the patented turret design assures proper alignment and on axis grating rotation.
Below is a comprehensive list of available gratings for the iHR series of spectrometers. Other gratings are also available upon request.
Ruled Gratings
Groove Density L/mm | Blaze Wavelength | Recommended Spectral Range | Blaze Angle | Part Numbers | |
---|---|---|---|---|---|
iHR320 68x68 mm | iHR550 76x76 mm | ||||
300 nm | 150-600 nm | 17°27' | 510 01 120 | 510 01 141 | |
500 nm | 250-850 nm | 26°45' | 510-02-120 | 510 02 141 | |
630 nm | 350-850 nm | 34°32' | 510 03 120 | Not Available | |
250 nm | 150-500 nm | 8°38' | 510-04-120 | 510-04-141 | |
330 nm | 200-700 nm | 11°25' | 510-05-120 | 510-05-141 | |
400 nm | 200-800 nm | 13°53' | 510-06-120 | 510-06-141 | |
500 nm | 250-950 nm | 17°27' | 510-07-120 | 510-07-141 | |
750 nm | 400-1200 nm | 26°45' | 510-09-120 | 510-09-141 | |
1µm | 500-1200 nm | 36°52' | 510-10-120 | 510-10-141 | |
350 nm | 200-700 nm | 9°00' | 510 91 120 | 510 91 141 | |
550 nm | 250-1100 nm | 14°30' | 510-93-120 | 510-93-141 | |
1.5 µm | 600-1700 nm | 42°27' | 510-97-120 | 510-97-141 | |
300 nm | 200-600 nm | 5°10' | 510-11-120 | 510-11-141 | |
400 nm | 250-800 nm | 6°54' | 510-12-120 | 510-12-141 | |
500 nm | 250-1000 nm | 8°38' | 510-13-120 | 510-13-141 | |
750 nm | 400-1500 nm | 13°00' | 510-14-120 | 510-14-141 | |
1µm | 500-1700 nm | 17°27' | 510-15-120 | 510-15-141 | |
1.5 µm | 750-2400 nm | 26°45' | 510-16-120 | 510-16-141 | |
2 µm | 1000-2400 nm | 36°52' | 510-17-120 | 510-17-141 | |
300 | 250 nm | 150-500 nm | 2°09' | 510-50-120 | 510-50-141 |
500 nm | 300-950 nm | 4°18' | 510-18-120 | 510-18-141 | |
600 nm | 350-1300 nm | 5°10' | 510-19-120 | 510-19-141 | |
1 µm | 700-2000 nm | 8°38' | 510-20-120 | 510-20-141 | |
2 µm | 1100-4500 nm | 17°27' | 510-21-120 | 510-21-141 | |
3 µm | 1700-5000 nm | 26°45' | 510-22-120 | 510-22-141 | |
4 µm | 2000-5000 nm | 36°52' | 510-23-120 | 510-23-141 | |
500 nm | 250-950 nm | 2°09' | 510-49-120 | 510-49-141 | |
1.2 µm | 800-2300 nm | 5°10' | 510-24-120 | 510-24-141 | |
2 µm | 1200-4000 nm | 8°38' | 510-25-120 | 510-25-141 | |
4 µm | 2.2 - 9 um | 17°27' | 510-26-120 | 510-26-141 | |
5 µm | 3.5 - 10 um | 22°01' | 510-27-120 | 510-27-141 | |
150 | 6 µm | 4 - 10 um | 26°45' | 510 28 120 | 510 28 141 |
150 | 8 µm | 5 - 10 um | 36°52' | 510 29 120 | 510 29 141 |
120 | 2-5 µm | 1.7 - 4.5 um | 8°39' | 510-30-120 | 510-30-141 |
5 µm | 3 - 10 um | 17°27' | 510-31-120 | 510 31 141 | |
7-5 µm | 4.5 - 12 um | 26°45' | 510-32-120 | 510-32-141 | |
450 nm | 250-950 nm | 1°17' | 510-48-120 | 510-48-141 | |
3 µm | 1.7 - 6 um | 8°38' | 510 33 120 | 510 33 141 | |
6 µm | 3 - 13 um | 17°27' | 510 34 120 | 510 34 141 | |
9 µm | 5 - 14.5 um | 26°45' | 510 35 120 | 510 35 141 | |
75 | 4 µm | 2 - 8 um | 8°38' | 510-36-120 | 510-36-141 |
8 µm | 5.5 - 17 um | 17°27' | 510 37 120 | 510 37 141 | |
12 µm | 8 - 19 um | 26°45' | 510-38-120 | 510-38-141 | |
10 µm | 7.5 - 13 um | 17°27' | 510 39 120 | 510 39 141 | |
15 µm | 9 - 24 um | 26°45' | 510 40 120 | 510 40 141 | |
50 | 6 µm | 3 - 12 um | 8°38' | 510-41-120 | 510-41-141 |
50 | 12 µm | 8 - 22 um | 17°27' | 510-42-120 | 510-42-141 |
50 | 18 µm | 11 - 28 um | 26°45' | 510-43-120 | 510-43-141 |
50 | 24 µm | 15 - 30 um | 36°52' | 510-44-120 | 510-44-141 |
40 | 22-5 µm | 14 - 30 um | 26°45' | 510 45 120 | 510 45 141 |
30 | 30 µm | N/A | 26°45' | 510 46 120 | 510 46 141 |
20 | 45 µm | N/A | 26°45' | 510 47 120 | Not Available |
Holographic Gratings
Groove Density L/mm | Recommended Spectral Range | Part Numbers | |
---|---|---|---|
iHR320 | iHR550 | ||
150-400 nm | 520-07-120 | 520-07-141 | |
3000 | 250-450 nm | 520-09-120 | 520-09-141 |
300-600 nm | 520-12-120 | 520-12-141 | |
170-500 nm | 520-13-120 | 520-13-141 | |
100-300 nm | 520 14 120 | 520 14 141 | |
450-650 nm | 520 15 120 | 520 15 141 | |
190-650 nm | 520 16 120 | 520 16 141 | |
150-450 nm | 520 17 120 | 520 17 141 | |
2000 | 100-300 nm | 520 18 120 | 520 18 141 |
450-850 nm | 520 -19 -120 | 520 -19 -141 | |
190-700 nm | 520 -20 -120 | 520 -20 -141 | |
150-450 nm | 520 21 120 | 520 21 141 | |
1800 | 100-300 nm | 520 22 120 | 520 22 141 |
400-1200 nm | 520 -24 -120 | 520 -24 -141 | |
190-700 nm | 520 -25 -120 | 520 -25 -141 | |
150-450 nm | 520 -26 -120 | 520 -26 -141 | |
400-1300 nm | 520 -29 -120 | 520 -29 -141 | |
150-450 nm | 520 30 120 | 520 30 141 | |
250-800 nm | 520 32 120 | 520 32 141 | |
400-1200 nm | 520 33 120 | 520 33 141 |
Blazed Holographic Gratings
Groove Density L/mm | Blaze Wavelength | Recommended Spectral Range | Part Numbers | |
---|---|---|---|---|
iHR320 | iHR550 | |||
250 nm | 190-600 nm | 530-13-120 | 530-13-141 | |
330 nm | 200-600 nm | 530-11-120 | 530-11-141 | |
400 nm | 300-600 nm | 530-15-120 | 530-15-141 | |
1800 | 500 nm | 450-850 nm | 530 19 120 | 530 19 141 |
250 nm | 180-650 nm | 530-20-120 | 530-20-141 | |
400 nm | 250-850 nm | 530-18-120 | 530-18-141 | |
250 nm | 190-450 nm | 530-25-120 | 530-25-141 | |
330 nm | 240-800 nm | 530-22-120 | 530-22-141 | |
500 nm | 300-1000 nm | 530-24-120 | 530-24-141 | |
630 nm | 400-1200 nm | 530-27-120 | 530-27-141 | |
750 nm | 500-1200 nm | 530-28-120 | 530-28-141 | |
900 nm | 600-1200 nm | 530-50-120 | 530-50-141 | |
900 nm | 700-1700 nm | 530-60-120 | 530-60-141 | |
850 nm | 700-1700 nm | 530-66-120 | 530-66-141 | |
500 nm | 300-1000 nm | 530-29-120 | 530-29-141 | |
1000 nm | 700-1750 nm | 530-34-120 | 530-34-141 |
Diffraction Grating Calculator
The Diffraction Grating Calculator below can be used to determine the various optical performance specifications of HORIBA spectrometers when used in conjunction with selected spectroscopy cameras, point detectors and various grating alternatives. It is a very useful tool with pull down selections of all of our current spectrometers, cameras and gratings.
Computer Control
All monochromator controls are fully automated including slit widths, turret position, wavelength, and swing mirror position. Slit widths may be set in step sizes of 2.25 micron for the 0 – 2 mm slit option and 6.25 micron steps for the 0 – 7 mm slit option. The turret position may be changed to switch from one grating to another and the wavelength may be tuned for the grating currently selected. The swing mirror position on either the entrance or exit of the monochromator can be adjusted to axial or lateral ports to switch between different entrance or exit front or side ports.
There are multiple software platforms to choose from for spectrometer control and acquisition.
HORIBA’s world renowned software platform, LabSpec is ideal for most Raman and photoluminescence applications. It offers advanced capabilities, with expert functionality, control and flexibility. LabSpec is the first choice for most spectrometer customers. | |
SynerJY™ | SynerJY™ software is a fully integrated data acquisition and data analysis program for spectroscopic systems. It is selected for custom spectroscopy configurations not suitable for LabSpec. |
LabVIEW™ | LabVIEW VI’s are now available for the complete line of instrumentation from the Optical Spectroscopy Division, allowing users to work with the LabVIEW™ development package from National Instruments. This option requires proficiency with LabVIEW™ programing. |
SDK | Software Development Kits (SDK’s) are available for programmers who wish to write their own software control of HORIBA spectrometers. This option absolutely requires proficiency with programing |
Schematics
iHR320, Top View
iHR320, Front View
iHR550, Top View
iHR550, Front View
Accessories
Compatible Optical Building Blocks
The iHR series spectrograph is one of many inter-connectible Optical Building Blocks available from HORIBA Scientific. These Optical Building Blocks can be ordered together to form a subassembly or even a complete custom spectroscopy solution.
Fiber Light GuidesWe offer a selection of fiber optic and liquid light guides to choose from depending on the application. Lens based fiber-coupler with f/# matching optics for SMA and ferrule (part number 220F, or 220F-AFC for FC Mount fibers). | ||
Direct fiber-coupler with no optics for 10 mm and 0.25″ ferrule with thumbscrew x-y adjusters, (part number AFO-XY) Mirror based fiber-coupler for 10 mm ferrule (part number J23078640). Contact us for information about SMA and FC adapters. Simple fiber-adapter for 0.25″ ferrule (part number 120F). |
Internal Filter WheelsUV-Vis: iHR internal filter wheel mounts at the entrance port only (not suitable for side entrance). The UV-Vis part number is AFW-IHR-UVVIS, and it include a blank window, 320 nm LP and 550 nm LP filters. 3 mm filter-thickness only. NIR: iHR internal filter wheel mounts at the entrance port only (not suitable for side entrance). The near-IR part number is AFW-IHR-NIR, and it includes a blank window, and 1000 nm LP filters. 1 mm filter-thickness only. |
Optical ChoppersIf you would like to use an optical chopper with your spectrograph/monochromator, then we have a number of solutions. To learn more Optical Accessoriesclick here. |
Single Channel Detectors
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Spectroscopy Cameras
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Broad Band Light Sources
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Specifications
Specifications Using standard 1200 line/mm ruled grating at 435 nm | ||
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iHR320 | iHR550 | |
Focal length | 320 mm | 550 mm |
Aperture ratio | f/4.1 | f/6.4 |
Wavelength range | 150 to 1500 nm with 1200 gr/mm grating | |
Flat Field Size | 30 mm x 12 mm | |
Bandpass | Continuously adjustable from 0 to 16 nm (1,200 g/mm) | Continuously adjustable from 0 to 9 nm (1,200 g/mm) |
Reciprocal linear dispersion at slit | 2.31 nm/mm (1,200 g/mm) | 1.34 nm/mm (1,200 g/mm) |
Resolution with exit slit and PMT | 0.06 nm (1,200 g/mm) | 0.025 nm (1,200 g/mm) |
Stray Light (measured at 1 nm from 514 nm laser with HORIBA Scientific holographic gratings) | 1.5 x 10 -4 (typical) | 1 x 10 -5 (typical) |
Accuracy | +/- 0.2 nm | |
Scan Speed | 160 nm/s | |
Step Size | 0.002 nm | |
Reproducibility | +/- 0.075 nm | |
Optical path height | 98 mm | |
Grating size | 68 x 68 mm | 76 x 76 mm |
Slit adjustment | 0 to 2 mm width (2.25 micron step size) |
Monochromator Dimensions | ||
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iHR320 | iHR550 | |
Length | 417 mm long (16.4 inches) | 648 mm long (25.51 inches) |
Width | 422 mm wide (16.6 inches) | 460 mm long (18.09 inches) |
Height | 192 mm high (7.6 inches) | 193 mm long (7.78 inches) |
Weight | 20 kg (45 lbs) | 28 kg (62 lbs) |