Frame buffer is a dedicated high-speed memory component integrated directly into the camera hardware. When the camera sensor captures an image, the data is first written to the frame buffer memory at extremely high speeds. From there, it's transmitted to your computer at the rate supported by your USB connection.
The GPM462C features native 12-bit ADC, providing 4096 gray levels for capturing subtle tonal gradations and color information. The camera supports hardware ROI (Region of Interest) functionality - smaller ROI sizes achieve higher frame rates, which is particularly useful in guiding applications where only a small area containing the guide star needs high-speed acquisition.
Flexible Pixel Binning
The GPM462C supports digital pixel binning from 1×1 to 8×8 in either stacking or averaging method. Pixel binning technology can improve signal-to-noise ratio, particularly useful in faint guiding conditions by combining adjacent pixels to enhance guide star signals while reducing read noise impact.
Built-in ST4 Autoguider Interface
The GPM462C features a built-in standard ST4 autoguider port for easy connection to the autoguider. This design simplifies guiding system configuration, reduces cable connections, and improves system reliability. Compatible with mainstream guiding software like PHD Guiding, MetaGuide, Nebulosity, MaxIm DL, and others for precise autoguiding control.

Comprehensive Connection Options
The GPM series cameras offer versatile connection options designed for seamless integration with various telescope setups and guiding systems. The diagram below illustrates the complete connection architecture, showing how the camera interfaces with your mount, computer, and other astronomical equipment for optimal guiding performance.

Connection Features:
- USB 2.0 Type-C interface for both data transfer and power supply
- ST4 autoguider port for direct mount connection
- Compatible with all major guiding software platforms
- No external power supply required - powered entirely through USB
Broad Software Compatibility
The GPM462C supports multiple driver interfaces including Native, ASCOM, and WDM, compatible with mainstream astronomy software such as PHD Guiding, Nebulosity, MaxIm DL, SharpCap, MetaGuide, FireCapture, and AstroArt. Provides multi-platform SDK support for Windows, Linux, macOS, including development interfaces for Native C/C++, C#/VB.NET, Python, Java, DirectShow, and Twain.
Convenient Power System
The camera operates via USB 2.0 interface. Upon establishing a connection with the host system using the USB 2.0 cable, the device is primed for operation. This design is particularly suitable for field observations, reducing power cable complexity.
Technical Specifications
Core Performance Parameters
| Maximum Frame Rate (USB 2.0) |
12-bit: 8.9 FPS @ 1920×1080 8-bit: 17.8 FPS @ 1920×1080 |
| Read Noise |
HCG: 0.70-1.08e⁻ | LCG: 1.48-2.4e⁻ |
| Full Well Capacity |
HCG: 4.8ke⁻ | LCG: 12.7ke⁻ |
| Peak Quantum Efficiency |
>89% |
| Dynamic Range |
74.1 dB |
| Signal-to-Noise Ratio |
40.8 dB |
| Exposure Time Range |
0.1ms - 1000s |
| Gain Range |
1× - 500× |
Basic Technical Specifications
| Sensor |
Sony IMX462 Color Back-illuminated CMOS |
| Image Resolution |
2.1 Megapixels (1920×1080) |
| Pixel Size |
2.9μm × 2.9μm |
| Sensor Size |
1/2.8-inch (diagonal 6.39mm) |
| Imaging Area |
5.57mm × 3.13mm |
| Shutter Type |
Rolling Shutter |
| ADC Bit Depth |
12-bit |
| Frame Buffer |
Built-in |
| Gain Modes |
HCG/LCG dual mode switching |
| Spectral Response Range |
380-690nm (with IR cut window) |
Interface and Physical Specifications
| Data Interface |
USB 2.0 Type-C |
| Guide Interface |
Built-in ST4 autoguider port |
| Camera Adapter |
Standard 1.25-inch for telescope connection Standard C adapter for industrial lens |
| Back Focal Distance |
8.5mm (17.5mm with C-mount, 12.5mm with CS-mount) |
| Protective Window |
IR-cut filter/AR-window |
| External Dimensions |
Diameter 37mm × Height 72.4mm |
| Weight |
70 grams |
| Cooling Method |
Passive cooling |
| Supported Systems |
Windows XP/Vista/7/8/10 (32 & 64 bit) Mac OS X, Linux |
| SDK Support |
Native C/C++, C#/VB.NET, Python Java, DirectShow, Twain, etc. |
The GPM462C provides HCG and LCG gain modes that can be flexibly switched according to different imaging requirements, delivering excellent performance under various conditions.
LCG Low Conversion Gain Mode Performance
Camera Settings: Full resolution, RAW 12-bit mode, LCG mode
LCG mode provides full well capacity of 12.1ke⁻, offering good headroom for bright targets. This mode maintains good signal-to-noise ratio while providing wide dynamic range (74.1dB), preventing overexposure on bright targets, particularly suitable for solar, lunar photography and bright planetary imaging.

HCG High Conversion Gain Mode Performance
Camera Settings: Full resolution, RAW 12-bit mode, HCG mode
HCG mode is optimized for low-light guiding, providing low read noise (minimum 0.70e⁻). At high gain settings, read noise remains at low levels, making it ideal for capturing faint guide stars, with good performance in deep sky object photography.


In the Box

Warranty
Touptek 2-Years Warranty