Application scenarios - nebulae, star clusters, star chains, galaxies

describe
The SV605CC adopts a diagonal 15.968mm (Type 1) CMOS sensor design, with a color square pixel array, each pixel measuring 3.76 μ m x 3.76 μ m. The sensor adopts a 14 bit A/D converter, and the 14 bit digital output can read signals of 9.07 million effective pixels at a high speed of 20 FPS. The readout noise is as low as 1.0e, which is very suitable for highdefinition, lownoise deep space object imaging.
Features:

Impressive 50ke full well capacity - helps reduce issues such as saturated stars.
HCG mode using HCG digital noise reduction technology, it can significantly reduce readout noise and maintain high dynamic range
No amplifier emission
Traditional CMOS sensors generate weak infrared light sources during operation, which are common in the corners of uncalibrated images and are a sign of "amplifier emission". Due to the zero amplifier lighting design of IMX533, the SV605CC camera has no amplifier lighting at all, whether it is longterm exposure or high gain, ensuring completely highquality "dark" images.
Cooling system
Thanks to the twostage TEC cooling, SV605CC can lower the temperature of CMOS sensors to 30 degrees Celsius below ambient temperature, greatly reducing the generation of dark current and sensor noise even under longer exposure times.
Suitable for various types of telescopes
1inch square sensor, better matching with telescope imaging, can avoid dark edges caused by uneven sensitivity of rectangular sensors; When imaging, turn on the cooling function to ensure more uniform cooling of the sensor, which can guarantee better cooling effect and achieve higher image quality.
256M DDR3 cache
The SV605CC has a builtin 256MB DDRIII image buffer. The advantage of an image buffer is that when the USB interface is not busy or interrupted, the memory will cache and transfer the image to the computer, so that frames will not be lost or damaged. This buffer also allows slower computers using USB 3.0 to capture every frame without losing it, even if the USB bus is occasionally busy with other peripheral devices. This buffer can also be used to run another camera on the same computer without USB transfer issues from SV605CC.

The SV605CC camera can be used with Windows, Linux, Mac OS, Chrome OS, and Raspberry Pi systems by running AstroDMx Capture.

Notes:
1、 Computer configuration requirements:


2. All software and drivers for this camera can be obtained from the SVBONY website.
Specifications:
Model SV605CC
Sensor color IMX533 CMOS
Image resolution 3008 * 3008
Total Pixel Size 9.0 Megapixels
Pixel size 3.76 μ m x 3.76 μ m
Target size 1 "
Diagonal 15.968mm

Shutter roller shutter
USB Type-B USB 3.0
High speed cache DDR3 256M
Exposure time 0.05ms-2000s
Read out noise from 1.0e-3.3e-
Quantitative easing peak 0.91
Fully charged 50ke-
ADC 14 bit
Temperature display software shows
TEC Semiconductor twostage cooling system


Pixel merging BIN1, BIN2, BIN3, BIN4
Operating systems Windows, Linux, Mac OS
Raspberry Pi, Chrome operating system
Protective window optical glass anti reflective film
Camera interface specifications 2 "/1.25"/M42X0.75
Rear focal length 6.5mm/17.5mm
Working current 300MA
Standby current 30mA

Packaging list:
① Camera bag x 1
② SV605CC camera x 1
③ 2inch cover plate x 1
④ M42-M48 ring x 1
⑤ T2-1.25 inch adapter x 1
⑥ 1.25inch Tshaped adapter x 1
⑦ M42M-M48F-16.5L x 1
⑧ M42M-M42F-21L x 1
⑨ T2 adapter x 1
⑩ User Manual x 1
⑪ USB 3.0 data cable x 1