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ATP5030 High-resolution UV-Vis Spectrometer
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Product Code: ATP5030
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  • ATP5030 is a cooled, ultra-high resolution micro spectrometer newly developed by Optosky, ATP5030 is based on the M-type optical path structure independently developed by Optosky, with extraordinary ultra-high resolution;at the same time, it uses a cooled 2048 pixel linear array detector to achieve the ultimate ultra-high resolution, the highest resolution can reach 0.05nm,It is a miniature spectrometer suitable for various high-resolution applications, with high reliability, ultra-high speed, low cost, and high cost performance. It can be adapted to various environmental uses such as online testing.
  • ATP5030 adopts TEC electric cooling, the cooling temperature is -5℃. Greatly reduce the dark current and noise of the spectrometer, and improve the dynamic range and signal-to-noise ratio of the spectrometer.
  • ATP5030 can receive SMA905 optical fiber input light or free space light, and output the measured spectrum data through USB2.0 or UART port.
  • ATP5030 only needs a 5V DC power supply, which is very easy to integrate and use.

Detector type Linear array detector
Spectral range 200-1100 nm
Effective pixels 2048 pixels
Pixels dimension 14μm×200μm
Full well capacity 300 ke-
Sensitivity 1300 V/(lx·s)
Dark noise 13 RMS @ 13 ˚C
Optical parameter
Focal distance 75mm
Optical resolution 0.07-3 nm
Incident Interface SMA905 connector
Signal-to-noise >600:1
Dynamic range 8.5 x 107 (system); 2000:1 for a single acquisition
Working temperature -25 ~ 50 oC
Numberical aperture 0.07
Working humidity < 90% RH
Trigger YES (IN and OUT)
Cooling temperature TEC cooled, -5 ˚C
Scanning rate < 1 kfps
Wavelength range 350-800nm, 200-400nm, 200-850nm, 200-1000 nm, 600-1000nm, 800-1000nm
Slit Size 50 μm (10, 25, 50, 100, or 200 μm optional)
Optical Design Czerny-Turner
Physical parameters
Dimensions 135 × 99 × 46 mm
Weight 0.5 kg
Sealing Anit-sweat
Electrical parameter
A/D conversion resolution 16 bit
Integration time 0.1 ms - 256 second
Interface USB Type-C
Supply voltage DC4.5 to 5.5 V (type @5V)
Operating current <2.3A
Storage temperature -30°c to + 70 °c
  • Detector cooling temperature: -5 ℃;
  • M type optical path, higher resolution;
  • Spectral range: 200-1100 nm;
  • Spectral resolution: 0.05 ~ 2 nm;
  • Optical path structure: non-crossing C-T;
  • Detector: 2048 pixels;
  • Integration time: 0.1ms ~ 256s;
  • Power supply: DC 5V power supply;
  • ADC bit depth: 16 bits;
  • Data output interface: USB Type-C;
  • 20-pin expansion interface.

  • LIBS,Plasma luminescence detection;
  • Raman spectroscopy detection;
  • Wavelength monitoring, laser, LED and other luminous bodies;
  • Water quality analyzer;
  • UV flue gas analyzer;
  • LED sorting machine, color detection;
  • Spectral analysis, radiation spectroscopic analysis, spectrophotometric analysis;
  • Reflection and transmission spectrum detection.
What are High Resolution & High Sensitivity & TE cooled Spectrometer from Optosky?

ATP5100 Ultra-miniature, Cooled BT CCD, sized up to a coin.
ATP5040 crossed C-T, TE-cooled 4096 pixels CMOS external cooling, high sensitivity
ATP5020P crossed C-T, Hamamatsu CCD cooled, higher sensitivity, SNR & dynamic range is higher than Maya.
ATP5030P M-shape C-T, higher resolution and low stray light, Hamamatsu CCD
ATP5030 (2048pixels) & ATP5034 (4096pixels) CMOS+TE-cooler, M-shape C-T, high resolution
ATP5330 (2048pixels) & ATP5334 (4096pixels) Thin, cooled CMOS+TE cooled, M-shape C-T, super high resolution

How many topology structure of optical path for a spectrometer?
There are commonly divided into 4 types of optical path, including crossed C-T, M-shape C-T, concave grating optical path, transmittance grating opitcal path.
Crossed C-T: ATP2000P,ATP2002, ATP2400, ATP1010, ATP5020P, ATP5040, ATP6500
M-shape C-T: ATP3030, ATP3034, ATP3330/4 ATP5030, ATP5034, ATP5330/4 
Concave grating: ATP4230, ATP4020, ATP4050, ATP4070
let's see the M-shape optical path looks like a number "3", so our models uses the 3rd number "3" to indicate M-shape optical path models.
In generally, topology structure can decide resolution, sensitivity, stray light, and size of a spectrometer.
Crossed C-T topology structure employs better sensitivity and compact size.
M-shape C-T employs higher resolution and better stray light.
Concave grating optical path employs high stray light.

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