The EGS-210 Echelle Grating Spectrometer developed by Light Spectrum Technology Co., Ltd. is a high-performance, compact high-resolution spectrometer. It is suitable for Laser-Induced Breakdown Spectroscopy (LIBS), Inductively Coupled Plasma Emission Spectroscopy (ICP), Plasma Spectroscopy, and Raman Spectroscopy detection, as well as astronomical research such as spectroscopy of exoplanets and other high-end scientific research and industrial applications.
- Resolution better than 0.03nm@300nm
- Wide dynamic range, continuous coverage from 180nm to 1100nm wavelength
- Compact, portable, reliable, with no moving grating components
- Compatible with various high-performance array detectors, such as deep-cooled CCD, ICCD, EMCCD, and sCMOS
- Flexible optical system configuration according to customer requirements for optimal performance
- The EGS-210 employs a two-dimensional cross-dispersion echelle grating-prism optical path structure with a focal length of 210mm and an aperture of F/9. This spectrometer can simultaneously measure spectra in the 200nm-1100nm range with a resolution of 0.03nm.
- The echelle grating disperses light through high-order, high-diffraction angles, with angular dispersion determined by the diffraction angle, which is 3-6 times that of traditional high-density gratings. The spectrometer then separates the spectral orders through a prism, ultimately forming a two-dimensional cross-dispersed spectral analysis system.
- By using a two-dimensional array detector for spectral signal detection, it fully utilizes the spatial signal acquisition capability of the array detector. The EGS-210 requires no moving optical elements, effectively ensuring the stability and reliability of the spectrometer.
- The EGS-210 is compatible with deep-cooled CCD, ICCD, EMCCD, and sCMOS detectors. The detector target surface can reach up to 20mm×30mm, and when paired with a 14mm×10mm ICCD detector, it can achieve full-element LIBS analysis in the 200nm-900nm wavelength range.
Technical Specifications of EGS-210
| Model | EGS-210-General | EGS-210-UV | EGS-210-VIS-NIR |
|---|---|---|---|
| Optical Structure | Optimized for full spectrum | Optimized for deep UV | Optimized for VIS-NIR |
| Wavelength Range(nm) | 200-1100 | 180-800 | 400-1100 |
| Focal Length(mm) | 210 | ||
| F-number | F/9 | ||
| Wavelength Resolution | 0.03nm @313.155nm (Φ50um slit) | ||
| Wave Number Resolution | Better than 2cm-1 | ||
| Wavelength Accuracy(nm) | 0.2 | ||
| Slit Width | 10um-100um optional; Custom large slits available for enhanced light flux or resolution | ||
| Fiber Interface | SMA905 | ||
| Dimensions | 242mm×86mm×155mm (without detector) | ||
| Weight(kg) | 6.1 (without detector) | 6.1 (without detector) | 6.1 (without detector) |
| Detector | Deep-cooled CCD, ICCD, EMCCD, and sCMOS | ||
| Applications | General high-resolution spectroscopy applications including LIBS, ICP, Plasma Spectroscopy, and Raman Spectroscopy | High-resolution, full-element atomic spectroscopy applications including LIBS, ICP, Plasma Spectroscopy, and UV Raman Spectroscopy | High-throughput VIS-NIR spectroscopy and Raman spectroscopy applications; Expandable to infrared spectrometer (1um-10um) range |
Combined Spectrum of Deuterium, Mercury, and Halogen Lamps Measured by EGS-210
313.155nm and 313.183nm Spectral Lines
