QHYCCD QHY461M PRO Scientific Medium Format Monochrome Camera
- Class 1 Scientific-Grade BSI Sensor
- Monochrome Medium Format
- Dual Air and Liquid Cooling System
- 2 x 10 Gigabit Fiber Interface
- Native 16-bit A/D Conversion
- Multiple Flexible Readout Modes
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Lancer l'assistant d'imagerieVérifiez quelles tailles de filtres et d'adaptateurs dégagent le capteur avec QHYCCD QHY461M PRO Scientific Medium Format Monochrome Camera, et la lumière perdue dans les coins.
Vérifier le vignettageThe QHY461M PRO is a scientific-grade medium format camera, built around a Class 1 monochrome, back-side illuminated sensor for professional research and imaging. Data transfer is handled by a dual 10 Gigabit fiber interface, ensuring high-speed readout for demanding applications like space object surveys and satellite tracking.
At the core of the QHY461M PRO is a medium format, back-side illuminated (BSI) monochrome sensor. The BSI architecture maximizes quantum efficiency by placing the sensor's wiring layer behind the photodiodes, while its native 16-bit A/D conversion delivers exceptional dynamic range. This camera is specified with a Class 1 sensor, indicating the highest grade of cosmetic and performance quality for scientific applications.
For consistent, low-noise results, the QHY461M PRO incorporates a powerful dual cooling system. It features both high-speed air cooling and ports for a liquid cooling circuit, providing maximum flexibility for thermal management. This ensures stable sensor temperatures and minimized thermal noise, whether deployed in an observatory dome or a remote field installation.
To manage the immense data generated by its medium format sensor, the QHY461M PRO is equipped with a dual 10 Gigabit fiber interface. This high-throughput connection is critical for achieving the highest possible frame rates and for applications that require rapid, full-frame downloads. The dual-port design provides the bandwidth necessary for large-scale surveys and tracking fast-moving objects without compromise.
The QHY461M PRO offers multiple readout modes to adapt to various imaging scenarios. This flexibility allows you to prioritize different performance characteristics, such as lowest read noise, highest full well capacity, or maximum frame rate. With access to on-chip binning and different readout architectures, you can optimize the camera's configuration for everything from faint-flux astronomical imaging to high-speed satellite tracking.
The primary distinction between the QHY461M Pro and its sibling, the QHY411 Pro, lies in sensor size and total resolution. The choice depends entirely on your instrument's corrected image circle and scientific goals.
The QHY461M PRO is designated as a scientific camera due to several key features. It uses a Class 1 sensor, the highest grade available, ensuring minimal defects. Its combination of air and liquid cooling provides robust thermal stability for low-noise, repeatable measurements. Finally, its native 16-bit A/D converter and multiple readout modes offer the dynamic range and flexibility required for research applications.
For large astronomical surveys, speed is critical. The QHY461M PRO's dual 10 Gigabit fiber interface provides the massive bandwidth needed to download its large, 100-megapixel files very quickly. This minimizes the dead time between exposures, maximizing the amount of sky you can cover in a single night.
The QHY461M PRO's 44mm x 33mm medium format sensor requires a telescope with a large, well-corrected image circle. It is an ideal match for high-end instruments like large-aperture Richey-Chrétien (RC) telescopes, corrected Dall-Kirkhams, or large astrographs designed specifically for wide-field imaging. Using it with a smaller telescope would result in significant vignetting.
The dual system offers maximum flexibility. Air cooling is sufficient for many environments and provides a simple, self-contained solution. For observatories in warmer climates or for applications requiring the absolute lowest and most stable sensor temperatures, the liquid cooling circuit provides superior thermal performance by efficiently transferring heat away from the camera body.
To create color images with the monochrome QHY461M PRO, you will need a set of astronomical filters (typically Luminance, Red, Green, and Blue) and a filter wheel. You take separate exposures through each filter and then combine them during image processing to create a full-color (LRGB) result. This method provides the highest possible resolution and signal-to-noise ratio.
The choice depends on your telescope's corrected image circle. The QHY411 Pro has a larger 150MP sensor (54x40mm) and is the better choice only if your telescope can illuminate that entire area without vignetting. The QHY461M PRO has a 100MP sensor (44x33mm) and is a better match for a wider range of large astrographs, ensuring you are only paying for the sensor area your telescope can actually use effectively.
| Configuration | Scientific Cameras - QHY461M PRO; Class 1, Mono BSI, Air and Liquid Cooling, 2 x 10BG |
| Sensor | Sony IMX461 BSI |
| Color or mono | Monochrome |
| Sensor width | 44 mm |
| Sensor height | 33 mm |
| Sensor diagonal | 54.8 mm |
| Resolution (W x H) | 11664 x 8748 |
| Pixel size | 3.76 µm |
| Back focus (sensor to front face) | 16 mm (28.5 mm with tilt adjust ring) |
| ADC | 16-bit |
| Full well | 80,000 e- (Extended Fullwell mode), 50,000 e- (Standard mode) |
| Read noise (min-max) | 1 e- to 3 e- (HGC mode) |
| Shutter | Electronic Rolling Shutter |
| Cooled | Yes, dual-stage TEC |
| Cooling delta T | -35°C below ambient (air), -45°C (water cooling) |
| Buffer memory | 2GB DDR3 |
| Data interface | USB 3.0, 2 x 10Gigabit Fiber |
| Max frame rate at full resolution | USB 3.0: 2.7 fps (8-bit), 1.7 fps (16-bit); PCIE: 3.0 fps (8-bit), 2.0 fps (16-bit) |
| Power requirement | 12V (11V to 13.8V), 49.2W at 100% TEC |
| Weight | 2900 g |