SOPHIA ® Featuring ultra-low noise electronic components, high sensitivity (>95% QE), speed, and flexibility, with multi port readout capabilities up to 16 MHz and high frame rates. ArcTec ™ Technology can achieve thermoelectric cooling without the need for coolers or low-temperature coolers.
>95% peak quantitative easing
2 electronic readings
Fast, multi port reading
ArcTec ™ Deep cooling
Main features
Ultra flexible performance
SOPHIA offers multiple readout modes, providing complete trigger support and independently optimized clocks for each combination, and can even capture ultrafast events.
SOPHIA also includes an on-site replaceable internal mechanical shutter to enhance flexibility.
Ultra flexible performance
SOPHIA offers multiple readout modes, providing complete trigger support and independently optimized clocks for each combination, and can even capture ultrafast events.
SOPHIA also includes an on-site replaceable internal mechanical shutter to enhance flexibility.
ArcTec ™ cooling technology
ArcTec ™ Cooling technology utilizes a fully metal sealed vacuum design to prevent exhaust or long-term degradation. Utilize customized heat sink design to ensure efficient heat dissipation of sensors and electronic components.
ArcTec ™ Provide air cooling only, liquid cooling only (suitable for vibration sensitive environments), or combined cooling.
SOPHIA 4096B Characteristics
Improved optical design
SOPHIA4096B features an improved field of view flattener and reduces the distance and thickness of the window from the CCD surface. It provides improved edge clarity and lower distortion.
Repeatable CCD positioning
With the ability to 'zero' variability in mechanical assembly, SOPHIA 4096B can achieve precise and repeatable CCD orientation. Adjustable tilt, pitch, and z-axis translation reduce the requirements for system level adjustments.
Multi TEC design
The redesigned CCD cooling mechanism and vacuum chamber ensure uniform heat dissipation of large-sized CCDs and can withstand thermal cycling.
Supported by LightField software
The powerful and intuitive software has a built-in math engine that allows for complete control of cameras and spectrometers, as well as real-time image analysis and spectral data.
LightField software seamlessly integrates hardware control and direct data acquisition into National Instruments' LabVIEW ® MATLAB with MathWorks ® Waiting in the program. The software also fully supports IntelliCal automatic wavelength and intensity calibration.
SOPHIA can also be fully controlled by PICAM SDK, eliminating any overhead that may occur when communicating through other development environments.
Product specifications
B: Back illuminated R: Deep depletion
X: eXcelon ™ Technical UV: UV Enhancement
MB intermediate frequency anti reflection coating A: astronomical deep depletion
AR: Double anti reflective coating
-Dark current at 90 ℃ |
0.0001 e-/p/s |
Image Area |
27.6 x 27.6 mm |
Deep cooling temperature |
It can be cooled to below -90 ℃ using a liquid cooler or air |
Cooling method |
Thermoelectric air or liquid cooling |
Supported interfaces |
USB 3.0 |
Model
model | imaging array |
sensor type |
pixel size |
SOPHIA 2048B-132-VS-R |
2048 X 2048 |
Back illuminated, deeply depleted |
13.5 x 13.5 μm |
SOPHIA 2048B-132-VS-UV |
2048 X 2048 |
Back illuminated, UV enhanced |
13.5 x 13.5 μm |
SOPHIA 2048B-152-VS-X | 2048 X 2048 |
Back illuminated with eXcelon ™ |
15.0 x 15.0 μm |
SOPHIA 2048B-152-VS-MB |
2048 X 2048 |
Back illuminated, medium frequency anti reflective coating |
15.0 x 15.0 μm |
SOPHIA 4096B-154-MB |
4096 X 4096 |
Back illuminated, medium frequency anti reflective coating |
15.0 x 15.0 μm |
SOPHIA 4096B-154-X |
4096 X 4096 |
Back illuminated with eXcelon ™ |
15.0 x 15.0 μm |
SOPHIA 4096B-154A–MB |
4096 X 4096 |
Back illuminated, astronomical mid frequency |
15.0 x 15.0 μm |
SOPHIA 4096B-154A–AR |
4096 X 4096 |
Back illuminated, astronomical depth depletion, dual anti reflective coating |
15.0 x 15.0 μm |