Spectrometers

509 Spectrometers from 48 manufacturers listed on GoPhotonics

Find and compare spectrometer from the leading manufacturers. Filter results by wavelength, measurement techniques supported and other parameters to find the spectrometer that is right for you. Download Datasheets and Request Quotations.

Description:Ocean MZ5 ATR-MIR Spectrometer
Spectrometer Type:
Benchtop
Measuring Techniques:
Absorbance, MIR Spectroscopy, Transmission
Wavelength Range:
1818 to 909 cm-1 (5.5-11 µm)
Integration Time:
30 sec
Spectrum Band:
Mid-IR, IR
more info
Description:NIRQuest512-2.5 Small-footprint Spectrometer for Near-Infrared Measurements
Spectrometer Type:
Modular, Portable
Measuring Techniques:
Molecular Spectroscopy, cell density measurements
Wavelength Range:
190 to 1100 nm
Spectral Resolution:
5 nm
Spectrum Band:
UV/Visible
more info
Description:900 - 1700nm InGaAs NIR Spectrometer
Spectrometer Type:
Modular, Portable
Measuring Techniques:
NIR Measurements
Wavelength Range:
900 to 1700 nm
Spectral Resolution:
4 nm
Integration Time:
20µs to 600s
Spectrum Band:
NIR
A/D Resolution:
Digitilizer: 16 Bit or 65,535:1 Band
Stray Light:
0.0005
Entrance Slit:
25 µm
more info
Description:FLAME-CHEM Spectrometer Systems
Spectrometer Type:
Benchtop, Portable
Measuring Techniques:
Raman Spectroscopy, Transmission
Wavelength Range:
532/1064 and 785/1064 nm
more info
Description:75 mm Focal Length Symmetrical Czerny-Turner Fiber Optic Spectrometer
Spectrometer Type:
Benchtop
Measuring Techniques:
UV Spectroscopy, NIR Spectroscopy
Wavelength Range:
200 to 1160 nm
Spectral Resolution:
0.09 to 20 nm
Integration Time:
2 µs - 20 seconds
Spectrum Band:
UV, NIR, UV-NIR
Slitwidth:
10 µm, 25 µm, 50 µm, 100 µm, 200 µm, 500 µm
A/D Resolution:
16 Bit
Stray Light:
< 0.5%
more info
Spectrometer Type:
Modular
Measuring Techniques:
MIR Measurements
Wavelength Range:
1.5 to 6.3 µm
Spectral Resolution:
3 nm
more info
Description:Fiber-coupled Terahertz Spectrometer
Spectrometer Type:
Modular
Measuring Techniques:
Laboratory Spectrometer, Real-time measurements, P...
Wavelength Range:
1064 nm
Spectral Resolution:
3 THz
more info
Description:Multichannel Imaging Spectrometer with up to 32 Simultaneous UV-NIR Spectra
Spectrometer Type:
Benchtop
Measuring Techniques:
Fluorescence Spectroscopy, NIR Spectroscopy, Refle...
Wavelength Range:
185 to 1050 nm
Spectral Resolution:
1 nm
Spectrum Band:
UV-NIR
Slitwidth:
22 µm
Stray Light:
< 0.1% (typical)
more info
Description:High throughput, low stray light and great thermal stability Spectrometer
Spectrometer Type:
Benchtop
Measuring Techniques:
UV Spectroscopy, NIR Spectroscopy, VIS Spectroscop...
Wavelength Range:
200 to 1100 nm
Spectral Resolution:
0.61 to 0.72 nm
Integration Time:
6 ms to 10 seconds
Spectrum Band:
UV-VIS, VIS-NIR
Slitwidth:
10 µm
Stray Light:
>3 AU
more info
Description:USB2000+VIS-NIR-ES Application-ready Spectrometer for the visible and near-IR with Enhanced Sensitivity
Spectrometer Type:
Benchtop
Measuring Techniques:
Molecular Spectroscopy, Fluorescence Spectroscopy
Wavelength Range:
200 to 800 nm
Spectral Resolution:
5 nm
Spectrum Band:
UV/Visible
more info

Spectrometers & Spectroscopy

Spectroscopy is the study of the interaction of electromagnetic radiation in all its forms with matter. This interaction might give rise to electronic excitations, (e.g. UV), molecular vibrations (e.g. IR) or nuclear spin orientations (e.g. NMR).

When a light or other radiation falls upon certain material liquid, gas or solid, a part of it gets absorbed by the material. This absorption causes the atoms, the molecules, and the bonds between them to vibrate at the same range of frequencies as the incident radiation. As a result we either see illuminance or a change in polarization or change in dipole moment. This entirely depends upon the type of radiation we are using.

Spectroscopy is the study of changes that occur in a sample due to absorption of the radiation. Spectrometers use these changes to identify and evaluate the sample. When a beam of white light strikes a triangular prism it is separated into its various components (ROYGBIV). This is known as a spectrum. The optical system which allows production and viewing of the spectrum is called a spectroscope or spectrometer. There are many other forms of light which are not visible to the human eye and spectroscopy is extended to cover all of these.

How does a spectrometer work:

A spectroscopic instrument or spectrometer generally consists of an entrance slit, collimator, a dispersive element, such as a grating or prism, focusing optics and a detector. In a monochromator system there is normally also an exit slit, and only a narrow portion of the spectrum is projected on a single one-element detector. In monochromators the entrance and exit slits are in a fixed position and can be changed in width. Rotating the grating scans the spectrum. 

The basic function of a spectrometer is to take in light, break it into its spectral components, digitize the signal as a function of wavelength, and display it through a computer. The first step in this process is to direct light through a fiber optic cable into the spectrometer through a narrow aperture known as an entrance slit. The slit vignettes the light as it enters the spectrometer. In most spectrometers, the divergent light is then collimated by a concave mirror and directed onto a grating. The grating then disperses the spectral components of the light at varying angles, which are then focused by a second concave mirror and reflected on to the detector. Alternatively, a concave holographic grating can be used to perform all three of these functions simultaneously. This alternative has various advantages and disadvantages, which will be discussed in more detail later on.

Once the light is imaged onto the detector the photons are then converted into electrons which are digitized and read out through a USB (or serial port) to a computer. The software then interpolates the signal based on the number of pixels in the detector and the linear dispersion of the diffraction grating to create a calibration that enables the data to be plotted as a function of wavelength over the given spectral range. This data can then be used and manipulated for countless spectroscopic applications.