NWSPEC
NWS6500 Spectrometer
NWS6500 Spectrometer
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Description:
NWS6500 Spectrometer: Precision Spectroscopy for Demanding Applications
The NWS6500 series represents a new standard in miniature fiber-optic spectrometers, combining exceptional sensitivity and stability for a wide range of demanding analytical and research applications. Featuring a low stray light optical bench, low-noise electronics, and a high quantum efficiency back-illuminated CCD detector, the NWS6500 delivers superior performance across the UV-Vis-NIR spectrum.
Its deep-cooled CCD, capable of thermoelectric cooling up to 40°C below ambient, significantly reduces dark current and thermal noise, enabling extended integration times and improved detection limits. This makes the NWS6500 ideal for low-light level applications and environments with fluctuating temperatures.
Key Features & Benefits:
High Signal-to-Noise Ratio (SNR): Ensures accurate and reproducible measurements, even for weak signals.
Deep-Cooled CCD Detector: Minimizes thermal noise, enabling longer integration times and enhanced sensitivity.
Back-Illuminated CCD: Maximizes light collection efficiency, providing superior sensitivity across the spectral range.
Enhanced UV Response: Extends spectral coverage into the UV region for a broader range of applications.
Low Stray Light Optical Design: Reduces background noise, improving accuracy in complex spectral environments.
Compact and Robust Design: Provides portability and reliable performance in both laboratory and field settings.
Versatile Software Suite: Offers comprehensive tools for data acquisition, processing, analysis, and instrument control.
Resolution:
Typical Applications:
Fluorescence Spectroscopy: High-sensitivity detection and quantification of fluorophores in diverse samples.
Raman Spectroscopy: Molecular fingerprinting for material identification, structural analysis, and chemical process monitoring.
Microscopy Spectroscopy: Spectral characterization of microscopic features in materials and biological samples.
Astronomy: Low-light level detection and spectral analysis of celestial objects.
Environmental Monitoring: Detection and quantification of pollutants in water, air, and soil.
Materials Science: Characterization of optical properties, thin film analysis, and material composition determination.
General Spectroscopy: A versatile platform for absorbance, transmission, reflection, and emission measurements in a wide variety of laboratory applications.
Items | Specification |
Spectral Range | 200 - 1100 nm (Model Dependent, specify range for each model) |
Optical Resolution | Up to 0.50 nm FWHM (Model Dependent, specify for each model) |
Wavelength Resolution | Up to 0.30 nm |
Stray Light | < 0.1% |
Order-Sorting Filter | Optional |
Detector Type | Back-thinned CCD array (Hamamatsu) |
Spectral Coverage | 200 - 1100 nm |
Number of Pixels | 1024 |
Pixel Size (H) | 24 μm |
Pixel Size (V) | 24 μm |
Pixel Height | 24um * 128 |
Sensitivity | 2.2 μV/e- |
Optical Design | f/4, Symmetrical Czerny-Turner |
Focal Length | 100; 110 mm |
Entrance Slit | Standard 70 μm (optional sizes available) |
Fiber Optic Connector | SMA9050, 0.22 NA |
Electrical Specification | |
Signal-to-Noise Ratio | 1200:1 |
Linearity | >99% |
Integration Time | 6 ms - 30 min |
Dynamic Range | 8000:1 |
A/D Converter | 16-bit, lossless |
Acquisition Speed | 6 ms + integration time |
Communication Interface | USB 2.0 |
Expansion Port | 16-pin external trigger port |
Operating System Support | Windows, Android, Linux, WinCE |
Power Consumption | 450 mA @ 5V DC |
Cooling | 4 A @ 5 V DC |
Dimensions | 182 x 110 x 50 mm |
Weight | 1600 g |
Mounting |
Standard 3-point mounting holes |
