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High Sensitivity & High Resolution Micro Spectrometer
Product Code: ATP5020
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Description:

Optosky ATP5020 UV-Vis spectrometer employs the ultra-high performance, high-sensitivity, high resolution, and cost-effective model. The award-winner spectrometer is called cooled Maya, it can even replace Maya and QE65 in SNR, sensitivity, and resolution. ATP5020 spectrometer is ideal for Raman system well. It uses 2048 x 64 pixel, a back-thinned CMOS+Cooler (-5℃). Sensor noise is reduced, and SNR is almost 2 times higher than others. Increased reliability can remain measure result do not change with temperature.

Customized design of CMOS+Cooler (-5℃) signal processing circuit built inside, Noise is lower can 3 counts is ahead of records in the industries.
ATP5020 spectrometer is designed with SMA905 optic fiber entrance connector or free space, and it outputs spectral data via USB2.0/UART

Features:

  • Detector:CMOS+Cooler (-5°C)
  • Detector parameters:2048×64pixel, 14×14um  Spectral
  • range: 190-1100nm (max.800)
  • Spectral resolution: 0.1-3 nm(depend on spectral range, slit width)
  • Optical path:Crossed C-T
  • Integration time:2ms-130s
  • Power supply:DC 5V±10% @ <2.3A
  • 18 bit, 570KHzA/D Converter
  • Entrance connector:SMA905 connector or free space
  • Output interface: high speed USB2.0 or UART
  • 20 pins, dual rows programmable extension connector

Detector
Detector type CMOS plus external cooling technology, TE-cooled to -5℃
Spectral range 180-1180 nm
Effective pixels 2048
Pixels dimension 14μm×14μm
Full well capacity 200 Ke-
Sensitivity 6.5 uV/e-
Dark noise 300 e-rms
Optical parameter
Focal distance 40/60mm
Optical resolution 0.06-2 nm
Incident Interface SMA905 connector,free space
Signal-to-noise >1300:1
Dynamic range 50000
Working temperature -10°c to + 50°c
Numberical aperture 0.11
Working humidity < 90% NC
Trigger YES (IN and OUT)
Cooling temperature -5°c
Full Well 300 ke-
Scanning rate < 1 kfps
Wavelength range 180-1180nm
Slit Size 50 μm (5, 10, 25, 50, 100, or 200 μm optional)
Optical Design f/4 crossed asymmetrical Czerny-Turner
Physical parameters
Dimensions 170×110×52 mm^3
Weight 0.8kg
Sealing Anit-sweat
Electrical parameter
A/D conversion resolution 18 bit
Integration time 1 ms - 30 s
Interface USB 2.0 (480MHz High speed)
Supply voltage DC4.5 to 5.5 V (type @5V)
Operating current <2.3A
Storage temperature -30°c to + 70 °c

Detector
Type
CMOS+Cooler (-5)
Spectral  range
190-1100 nm
Effective  pixels
2048×64
Pixel  sizes
14μm×14μm
Full  range
~200 ke-
Sensitivity
6.5 uV/e-
Dark  noise
6 e-
Optical parameters
Wavelength  range
190-1100 nm
resolution
0.1-3 nm (depend on slit, spectral range)
SNR
>8000:1
Dynamic  range
10000 :1
Operating temperature
-10-40 oC
Operating  humidity
< 85%RH
Optical parameters
Optical  path
f/4 crossed  C-T
Focal
77.5  mm  for  incidence /  111.6  mm  for   output
Entrance  slit width
5、10、25、50、100、150、200  μm  (optional) Available  in  customized  other widths
Entrance connector
SMA905  Fiber  optic  connector,  free  space
Electrical parameters
Integration time
10 ms - 65 second
Data output  port
USB 2.0
ADC in-depth
18 bit  (Actual output16bit)
Power supply
DC 5V±10%
Operating current
<2.3A
Storage temperature
-20°C to +70°C
Operating temperature
-10°C to +40°C
Physical  parameters
Size
170×110×52 mm
Weight
1.3 kg
Sealing
Anti-sweat

  • Raman spectrometer
  • Micro spectrophotometer, 
  • high-speed spectrophotometer
  • Spectral analysis /radiation spectrophotometer/ spectrophotometric analysis
  • Transmittance, absorbance, reflectance detection
  • Wavelength detection
  • LIBS


How to choose miniature raman spectrometer?

The ATP5020 is the lowcost micro raman spectrometer, whose customized for raman spectrometer employs high sensitivity and high resolution with cooled down to -5C.

What is the cooling temperature for the ATP5020?
It uses Hamamatsu s11639 plus external cooling technology to cool down to -5C proving constant measuring results.

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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