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【Voltage Compatibility】
When using electrical appliances, please note that they are designed for Japanese voltage specifications (90-110V), so if you use them with a different voltage, it may cause a malfunction.
【Plug Type】
Our products use Japanese plug types (A or B type).
Please use a conversion adapter if necessary.
【Important Note on Transformers and Adapters】
A transformer adjusts voltage to match your device’s requirements.
A conversion adapter only changes the plug shape and does not adjust voltage.
Using only a conversion adapter without a transformer may result in damage to the product.
【Liability】
We are not responsible for malfunctions or damages caused by improper use, such as operating the product without a transformer.
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The SV505C astronomical camera uses an IMX464 color sensor with 1/1.8 inch frame, resolution 2712*1538, and total pixels of about 4.2 million. Additionally, the active area of the IMX464 sensor is approximately twice that of the IMX462 sensor, allowing the IMX464 sensor to capture a wider area when using the same telescope.
The SV505C color CMOS camera has a QE of approximately 80%, very high sensitivity in the near-infrared region, and a very high signal-to-noise ratio in dark night environments. The SV505C planetary camera offers 8-bit and 12-bit RAW. Cameras are very sensitive to visible and near-infrared light. Very suitable for photographing details of solar system planets and lunar surfaces such as Mars, Jupiter, and Saturn.
Equipped with an ST4 guide port, it can be connected to the equatorial mount's AUTO GUIDE interface and use PHD2 guide software to control the equatorial mount's automatic guide. Adopts USB3.0 high-speed data transfer to capture planet, moon, and sun images quickly and efficiently. Compatible systems: Windows, Linux OS Raspberry Pi, Mac OS, Chrome OS.
The SV505C planetary camera uses HCG noise reduction technology, when increasing the gain, HCG mode is automatically turned on, which can significantly reduce readout noise while maintaining high dynamic range at low gain. Unique heat dissipation design keeps the camera operating temperature low. Long exposure during use will reduce noise to some extent and improve image quality.
At full resolution, the camera's frame rate can reach 93 fps and capture more frames at the same time. Shooting gaps can be used to quickly complete shooting, especially if the weather is not ideal.
Features: ◆1/1.8” COMS sensor SV505C uses Sony IMX464 sensor, the QE of the sensor is very high, the QE value is 80%, and the readout noise is 2.9e~0.7e ◆Pixel size is 2.9um, resolution is 2712 x 1538 pixels, diagonal is 9mm. ◆128MB DDRII buffer SV505C has a built-in 128MB DDRIII image buffer. The advantage of USB ◆This buffer ensures that no frames are lost or corrupted because the memory caches the images and transfers them to the computer when the interface is not busy or interrupted. However, even if the USB bus is occasionally busy with other peripherals, this buffer allows you to capture every frame without loss. It also allows you to run different cameras using the same computer without any transfer issues.
Supports BIN 1*1 or BIN 2*2 SV505C has ROI and BIN functions. You can set any resolution. A smaller region of interest (ROI) is read from the sensor and the image scale of the imaged object is not changed. It can also greatly improve the shooting rate. ◆BIN2*2 pixels can combine two adjacent pixels, improving camera sensitivity. ◆ST4 Guiding It is designed with ST4 guiding ports supported by PHD2 and ASCOM platforms. ◆Can be controlled using a computer. The telescope mount has an autoguiding port (commonly called an ST-4 port suitable for analog signals) that connects directly to the autoguider. ◆ USB3.0 high-speed transmission. Adopts USB3.0 high-speed data transfer to capture planet, moon, and sun images quickly and efficiently. ◆ ADC (Analog to Digital Converter) 12bit SV505C camera provides 8-bit and 12-bit RAW. ◆Special heat dissipation structure Unique
Heat dissipation design keeps the camera operating temperature low. Long exposure during use will reduce noise to some extent and improve image quality. ◆ AR Anti-Reflection Coated Lens Glass Cameras are extremely sensitive to visible light and near-infrared light. Different filters can be used to achieve different imaging. ◆HCG Digital Noise Reduction Technology HCG Digital Noise Reduction Technology allows you to significantly reduce readout noise while maintaining a high dynamic range.
