Feature

●The SV505C astronomy camera uses a 1/1.8" frame, resolution of 2712*1538, IMX464 color sensor, with a total of approximately 4.2 million pixels. In addition, the IMX464 sensor has a light reception area of about 2 times the IMX462 sensor, and when using the same telescope, the IMX464 sensor can shoot a wider area
●The SV505C color CMOS camera has a very high sensitivity in the near infrared area, with QE about 80% and has very high signal to noise ratio in dark night environments. The SV505C planetary camera provides 8-bit and 12-bit RAW. The camera is very sensitive to visible light and near infrared light. It is very suitable for photographing details of solar system planets such as Mars, Jupiter, Saturn, etc
●Equipped with ST4 guide port, connect to AUTO GUIDE interface of equatoritorial globe and control the automatic guide of equatoritorial rite. Adopting USB 3.0 high-speed data transfer, it can capture the images of the planet, moon and sun fast and efficient. Support System: Windows, Linux OS Raspberry Pi, Mac os, Chrome os
●The SV505C planetary camera uses HCG noise reduction technology to automatically turn on HCG mode when the gain is raised, maintaining a high dynamic range of low gains, while greatly reducing reading noise. Unique heat dissipation design will lower camera operating temperature. If exposed for a long period of time during use, it will reduce the noise and improve image quality
●At full resolution, the camera frame rate can reach 93 fps, allowing you to capture more frames at the same time. Especially if the weather is not ideal, you can use the shooting gap to complete your shooting quickly


Description

SV505C Color Planetary Camera

SV505C Color CMOS CameraSV505C Color CMOS Camera

The SV505C uses IMX464 12-bit ADC sensor, 1/1.8" frame, 2.9um pixel size, 12ke full well charging, and 42 million pixels.Infrared capture function.High sensitivity and ultra-low readout noise make it more subjective and higher resolution than IMX462 for planetary photography, sun and moon photography.

AR coatingAR coating

AR coating

The camera is very sensitive to visible light and near infrared light.You can use a variety of filters to achieve a variety of imaging.

HCG ModeHCG Mode

HCG Mode

Using HCG Digital Noise Reduction Technology, you can significantly reduce reading noise while maintaining a high dynamic range.

Low Read NoiseLow Read Noise

Low Read Noise

IMX464 read noise is 2.9e-0.7e.Low reading noise, suitable for planet, sun and moon photography.

High near infrared sensitivityHigh near infrared sensitivity

High near infrared sensitivity

The IMX464 features high sensitivity in the near infrared light area.Combined with IR850, CH4 and other filters, we offer a new shooting style.

IMX464 SensorIMX464 Sensor

The same telescope allows you to shoot a wider range. Especially when taking mosaics of the moon and the sun, the number of photos is less and more efficient.

Ports & Continuous Ring

Color CMOS CameraColor CMOS Camera
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128MB DDRIII Buffer128MB DDRIII Buffer

128MB DDRIII Buffer

The SV505C has a built-in 128MB DDRIII image buffer.The advantage of the image bufferer is that when the USB interface is not busy or interrupted, memory caches the image and transfers it to your computer, so the frame will not be lost or damaged.Whether your computer is slower speed with USB 3.0 or the USB bus is sometimes busy with other peripherals, you can capture all frames without loss.You can also use the same computer to run different cameras without the problem of USB transfer from SV505C.

Special heat dissipation structureSpecial heat dissipation structure

Special heat dissipation structure & ROI and BIN functions

Unique heat dissipation design will lower camera operating temperature.If exposed for a long period of time during use, it will reduce the noise and improve image quality.You can set any resolution.The smaller area of interest (ROI) is read from the sensor, and the image scale of the image on the image is not altered.It can also greatly improve your shooting rate.BIN2*2 pixels can be combined with two adjacent pixels to increase camera sensitivity.

Compatibility SystemCompatibility System

Note:

Computer Configuration Requirements:

Desktop computers are configured with Intel 4th generation i5 or above and have 4G or higher memory.Laptop configured Intel 6th generation i5 or above with 8g of memory

The SV505C Astronomy camera is suitable for use with refractor telescopes mounted on equatoritorial that can accurately track the movement of the sky. It is not suitable for taking pictures through the telescope eyepiece. Additional accessories or filters may be required for best results. If you use the SV505C camera to capture images through the telescopes eyepiece, you need to purchase the projection adapter of the eyepiece.All software and drivers of SV505C color astronomy cameras are available from the manufacturers website.

Specifications

CMOS Sensor: IMX464 1/1.8 shape (7.9 x 4.5 mm)
Total Pixels: 4.2 megapixels
Diagonal: 9mm
Resolution: 2712 x 1538
Pixel Size: 2.9μm x 2.9μm
Frame Rate: 93FPS
Exposure time: 64μs ~ 2000s
Read Noise: 2.9e-0.7e
Saturated Charge Capacity: 12000e
A/D Converter: 12-bit
Compatible System: Windows, Linux OS Raspberry Pi,Mac os, Chrome os
Flange Back: 6.5mm/12.5mm
Working Humidity: 30%-80%
Storage Humidity: 20%-90%
Operating Temperature: -10℃~+50℃
Storage Temperature: -20℃~+60℃