Sony imx533 color cmos sensor
Product selling point
1. Sv605cc is equipped with a 15.968mm diagonal (Type 1) CMOS sensor with a square color pixel array and 3.76μm x 3.76μm per pixel.
2. Foldable and Portable: This camera is foldable and easy to carry, it can be easily stored in your backpack or bag.
3. The digital HCG noise suppression technology is adopted, and the readout noise can be greatly reduced while maintaining a high dynamic range.
4. Since the imx533 uses zero amp glow design, regardless of long exposure time or high gain, the sv605cc camera has no amplifier glow at all to ensure the absolutely high quality "dark" image.
Sv605cc is designed with a diagonal 15.968mm (Type 1) CMOS sensor with a color square pixel array and 3.76μm x 3.76μm per pixel. The sensor contains a 14-bit A/D converter, the 14-bit digital output allows the signals of 9.07 m effective pixels to be read out at a high speed of 20 fps. The readout noise is as low as 1.0e, making it well suited for high-resolution, low-noise deep space objects.
Low readout noise in HCG mode
The hcg digital noise reduction technology is adopted, and the readout noise can be greatly reduced while maintaining a high dynamic range.
No amp glow
Traditional cmos sensors produce a weak infrared light source during operation quite often seen in the corner of uncalibrated images as the telling story sign of "amp glow". Since the imx533 uses a zero amp glow design, regardless of long exposure time or high gain, the sv605cc camera has no amp glow at all, ensuring that the “dark” image is of completely high quality.
Better resolution & edge sharpness
The sv605cc camera has better resolution, which is very important when capturing small targets. The camera allows you to dramatically increase the overall detail of the celestial object you capture. In addition, the edge sharpness is almost the same as in the middle of the picture.
Tec cooling
Thanks to the two-stage tec cooling, the sv605cc can reduce the cmos sensor temperature to 30 degrees Celsius below ambient temperature. This can significantly reduce dark current generation and sensor noise even during longer exposure times. *The actual cooling degree is affected by the current ambient temperature and the camera works better when the degree of the sensor is between -5~+5℃.
USB 3.0 & 256m DDR3 buffer
The sv605cc has a built-in 256mb ddriiii image buffer. The advantage of the image buffer is that the memory caches the image and transfers it to the computer when the USB interface is idle or interrupted. so that the frame does not get lost or damaged. This buffer also allows a slower computer with USB 3.0 to capture every frame without loss, even if the USB bus is occasionally busy with other peripherals. This buffer also allows another camera to run on the same computer without USB transfer issues from the sv605cc.
Supported systems
Sv605cc camera works with windows, linux, mac os, chrome os and raspberry pi systems by running astro dmx capture.
For Windows system, also support N/A. n.a., Theskyx, Sharp cap and other software runs through ascom platform with ascom drivers.
Support roi & am
The sv505c camera has roi and am functions. Any resolution can be adjusted while the image scale of the imaged object remains unchanged, greatly improving the photo rate.
Bin1*1, 2*2, 3*3, 4*4 pixels can merge neighboring pixels and improve the sensitivity of the camera.
Ideal for short focal length telescopes
The 1 inch square sensor has a better degree of agreement with the telescopic imaging, which can avoid the dark edge caused by uneven light sensitivity of the rectangle sensor. Turn on the cooling function when imaging, the cooling of the sensor is more uniform, which can ensure a better cooling effect to achieve higher image quality.
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