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Fiber Optic Spectrometers General Purpose Spectrometers

DETAIL

The HS4096 is a compact miniature fiber optic spectrometer with a configurable spectral range, offering high resolution (up to 0.07 nm), low stray light (~0.1%), and excellent thermal stability (wavelength drift <0.2 pixel/°C). It is equipped with low quantization dark noise and an increased number of spectral channels, making it ideal for laser measurement, plasma emission spectroscopy, color analysis, absorbance measurement, and Raman spectroscopy. It is a high-performance, cost-effective industrial-grade fiber optic spectrometer.


  • Features

  • Low stray light: ~0.1%
  • High resolution: up to 0.07 nmLow-temperature drift design, wavelength temperature drift ~0.2pixel/
  • Key-SMA905 design, compatible with Oceanhood’s multi-core dense cluster fiber (insertion consistency ≤7%)
  • Equipped with UV-enhanced linear array 4096-pixel CMOS detector, UV spectral response is strong, more spectral channel
  • High performance AD quantization sampling circuit, CCD quantization background noise 20 RMS (minimum integration time);
  • Supports multiple communication interfaces: USB, RS232, and 24PIN interactive interface.
  • Configure proprietary DAC and ADC, can achieve supporting light source enable, intensity control and power feedback.
 

  • Specification

Optical parameters
Optical fiber interface Key-SMA905
Number of pixels 4096 pixels
Stray light ~0.1%
Wavelength shift with temperature ~0.2pixel/
Consistency of optical fiber insertion and removal 7%
Function parameters
AD sampling 16bit
Data interface USB2.0、RS232
Extended function interface 24PIN
Acquisition mode Single, continuous, software trigger, synchronous external trigger, asynchronous reset external trigger
Detector integration time 60μs-65S
CCD read noise1 ≤20
CCD dynamic range2 3200:1
Signal-to-noise ratio 400:1
Response linearity3 98%
Others
Weight 260g
Dimension 98×80×24 mm
Operating temperature 0℃~40℃
Working humidity 20%-85%
1.CCD readout noise: RMS value of the CCD readout noise at the minimum integration time.
2.CCD dynamic range: calculated under minimum integration time as (saturation value − dark noise baseline) / standard deviation of CCD readout noise, evaluated according to Oceanhood Opto-Electronics standards.
3.Response linearity: The response nonlinearity is measured before calibration.
 

 
  • Products
Model Spectral Range Spectral resolution
Start End
10µm
25µm
50µm 100µm
200µm
HS4096-200-800
200 800 0.60 1.00 1.20 2.00 3.80
HS4096-750-1100
750 1100 0.40 0.50 0.70 - -

► Spectral range and parameters can be customized.
► Resolution values may vary by 120% from nominal.


 

  • Demensional drawing


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  • Testing results
Dark noise (Integral time:10ms)

 

Dark noise (Integral time:100s)


 
Deuterium tungsten light source (Integration time:5ms)
 
Mercury argon light source

 
 

Photoluminescence (PL) measurement results