The Maya2000 Pro spectrometer provides high sensitivity, covering approximately 165-1100 nanometers (specific wavelength range depends on different grating configurations). They are very suitable for measuring deep ultraviolet light (vacuum ultraviolet light), ultraviolet visible light, and visible near-infrared light.
Inside each Maya2000 Pro spectrometer, there is a thin back illuminated array FFT-CCD detector mounted on a robust and configurable optical mount with low-noise electronic components. There are various accessories and optical sockets for you to choose from. Our application sales engineers can assist you in selecting configurations based on your measurement needs.
Product Features
90% quantization rate
Low electronic noise
Optical resolution (FWHM can reach~0.035nm); The resolution depends on the number of lines on the grating and the size of the slit
14 grating options, including HC-1 composite grating that can cover the range of 175-1100nm
● Optional slits include 5 μ m, 10 μ m, 25 μ m, 50 μ m, 100 μ m, and 200 μ m
The focusing lens of the detector can enhance the signal strength
Signal measurement can be controlled by software programming (single or continuous), and operated by GPOs digital interface spectrometer
application
Suitable for scientific experiments with low brightness and high UV sensitivity requirements
specifications
Physical parameters |
Maya2000 Pro |
size: |
149 x 109.3 x 50.4 mm |
Weight: |
0.96 kg |
detector |
|
Type: |
Thin back illuminated type,2D |
Options: |
Hamamatsu S10420(UV)-The best option for visible light applications |
Hamamatsu S11510(Visible)-The best option for near-infrared light applications |
|
Quantum efficiency: |
75% peak @ 600 nm (S10420) |
85% peak @ 700 nm (S11510) |
|
optics |
|
Spectral range (detector response): |
165-1100 nm (S10420)(The specific wavelength range depends on different grating configurations) |
400-1180 nm (S11510)(The specific wavelength range depends on different grating configurations) |
|
Optical resolution(FWHM): |
Depends on the grating line density and slit size (with multiple options available) |
Full Signal to Noise Ratio: |
~450:1 |
Dynamic range: |
15000:1 (typical) |
Integral time: |
7.2 ms -5second |
Fiber optic connector: |
SMA 905Up to numerical aperture0.22A single fiber optic cable |
electron |
|
Power requirements: |
500 mA @ +5 VDC |
Trigger mode: |
4Modes |
Strobe function: |
have |
Interface: |
USB 2.0, RS-232 |
environmental condition |
|
Temperature: |
0°Cto+50°C(Operating temperature) |
Humidity: |
0-90%(No condensation) |