New features!
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- New combos available:
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- Deep Space EVO (3nm.)
- Planetary, and
- Photometric
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- Filter sets can be purchased separately.
- Dedicated Off-Axis Guider for the miniCAM8 series.
- New combos available:
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| Featured Reviews from YouTubers |
miniCAM8 Combo available
miniCAM8M Mono Deep Sky Combo (7nm)
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miniCAM8C Color Deep Sky Combo
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Luminance (19*12*1.1 mm)
miniCAM8M Deep Sky Combo EVO (3nm) – New!
Compared with the original Deep Sky Filter Set, the EVO version incorporates improved optical-coating technology and offers narrower bandpasses on the narrowband filters. All filters provide an OD value of 5. |
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miniCAM8M Planetary Combo – New!
This package delivers excellent performance for imaging Jupiter, Saturn, Venus and other bright targets, as well as for advanced atmospheric studies (methane band, UV, sodium line) |
miniCAM8M Photometric Combo – New!
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Filter set available
Deep Sky Mono filter set – TWO VERSIONSStandard: LRGB + 7 nm SHO filters (total 7 pcs)+ filter disk – New!
Ideal for deep-sky imaging in both broadband and narrowband channels.
EVO: Set de filtros LRGB + 3 nm SHO filters (total 7 pcs)+ filter disk – New!
Ideal for deep-sky imaging in both broadband and narrowband channels. |
Deep Sky Color filter setLPF+HLP+FCE+UV/IR Cut filter set (total 4 pcs) + filter disk – New!Enhancement and protection filter set including:
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Planetary Mono filter setLRGB+20 nm CH₄ + 40 nm UV + 10 nm Na filter set (total 7 pcs) + filter disk – New!
For specialised planetary imaging. |
Photometric Mono filter setSloan photometric set (u’, g’, r’, i’, z’) (total 5 pcs) + filter disk – New!
Ideal for scientific and educational photometry applications.
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7 nm ArIII filter ×1 – New!
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Dedicated Off-Axis Guider for the miniCAM8 series – New! Featuring a large 14 × 10 mm prism and 55 mm back-focus. Includes:
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At just over 4 inches in diameter and a few inches thick, the new miniCAM8 is a compact, high resolution, high performance, cooled imaging system capable of exceptional, high-quality deep space images as well as high-quality, high-resolution planetary images.
So often, compactness in astroimaging is achieved at the expense of some other critical feature found in multi-component cooled systems, such sensor quality or thermoelectric cooling, etc. Such is not the case with the new miniCAM8. Based on Sony’s IMX585 8 MP sensor, the miniCAM8 includes full TE cooling capable of reaching a delta of -45℃ from ambient along with a built-in 8-position filter wheel for complete LRGB and narrowband imaging.
| First Images from Our Customers! | |
| By Nicolas Bricaud, with an ultra-light setup! | |
NGC 281 Nebula, Pacman Nebula |
IC 405 Nebula, Flaming Star Nebula |
| (*) The IMX585 is a 1/1.2″ sensor with 8 million pixels (3840 x 2160 resolution), widely used in high-performance cooled cameras, especially in the fields of astronomical observation and low-light imaging.The monochrome version removes the Bayer filter, significantly enhancing sensitivity, making it ideal for astrophotography, scientific imaging, and photometry applications. Generally, to provide HDR (high dynamic range) imaging, multi-exposure image capture is required, and the multiple images recorded at differing exposure times are composited into a single shot. This results in issues with artefacts. The latest sensor design adopts Sony’s new proprietary “STARVIS 2” technology, which delivers both high sensitivity and HDR imaging. It allows for imaging in a single exposure, which suppresses the occurrence of artifacts, delivering 88 dB HDR, approximately 8 times that of a conventional sensor without increasing the pixel size.It also increases the sensitivity in the near infrared range by approximately 1.7 times compared to a conventional sensor. |
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High Near-Infra-red Sensitivity
The IMX585 is a Sony Starvis II processor that enables high sensitivity and high dynamic range (HDR). It also improves sensitivity in the near-infra-red range by approximately 1.7 times* compared to the IMX485. The new camera QHY miniCAM8 has a maximum quantum efficiency of 60% in the near-infra-red band and 92% in the visible wavelength band.
*Official data provided by Sony: https://www.sony-semicon.com/cn/news/2021/2021062901.html
BSI
One benefit of the back-illuminated CMOS structure is improved full-well capacity. This is particularly helpful for sensors with small pixels. In a typical front-illuminated sensor, photons from the target entering the photosensitive layer of the sensor must first pass through the metal wiring that is embedded just above the photosensitive layer. The wiring structure reflects some photons and reduces the efficiency of the sensor.
In the back-illuminated sensor, the light is allowed to enter the photosensitive surface from the reverse side. In this case, the sensor’s embedded wiring structure is below the photosensitive layer. As a result, more incoming photons strike the photosensitive layer, and more electrons are generated and captured in the pixel well. This ratio of photon to electron production is called quantum efficiency. The higher the quantum efficiency, the more efficient the sensor is at converting photons to electrons, and hence the more sensitive the sensor is to capturing an image of something dim.
Zero A
mplify Glow
QHY miniCAM8 is also a zero amplifier glow camera.
Anti-Dew Technology
Based on almost 20-year cooled camera design experience, the QHY cooled camera has implemented the fully dew control solutions. The optic window has a built-in dew heater, and the chamber is protected from internal humidity condensation. An electric heating board for the chamber window can prevent the formation of dew, and the sensor itself is kept dry with our silicon gel tube socket design for control of humidity within the sensor chamber.
Cooling
In addition to dual-stage TE cooling, QHYCCD implements proprietary technology in hardware to control the dark current noise.
The native ADC of the IMX585 sensor is 12-bit. Compared to 16-bit, the 12-bit depth offers fewer bits, resulting in a relatively narrower dynamic range, which may lead to issues such as insufficient color gradation and potential information loss. During the product development of miniCAM8, QHYCCD merged high and low gain to extend the data to 16-bit. However, since this 16-bit depth is not native, a sudden shift in linearity might occur, affecting the smooth transition in images. To address this, QHYCCD developed the “Linearity HDR” mode, which uses an algorithm-based approach to correct image linearity through software, ensuring smoother transitions and richer color representation.
Specification
| Model | QHY miniCAM8 |
| CMOS Sensor | Sony IMX585 |
| Mono/Color | Both |
| BSI/FSI | BSI |
| Sensor Size | 1/1.2inch |
| Pixel Size | 2.9μm*2.9μm |
| Total Pixel Area | 3856*2180 |
| Effective Pixels | 8 MP |
| Full Well Capacity | 54ke- |
| Readout Noise | 0.76 – 7.8 e- |
| A/D | 12bit (output as 16-bit) |
| Full Frame Rates | Full Resolution: 41.5FPS@8bit，23.5FPS @16bit |
| ROI Frame Rates | Full Resolution 1080 Lines, 82FPS@8bit, 47FPS@16bit；640Lines, 177FPS@8bit, 105FPS@16bit |
| Exposure Time Range | 11μs-900sec |
| Shutter Type | Electronic Rolling Shutter |
| Built-in Image Buffer | 512MB DDR3 |
| Computer Interface | USB3.0 |
| Telescope Interface | 1.25 inc |
| Optic Window Type | AR+AR |
| Filter Wheel | Built-in 8-Position Carousel |
| Back Focal Length | 17.5mm |
| Cooling System | Dual Stage TEC cooler: Long exposures (> 1 second) typically -45℃ below ambient |
| Weight | 480g |
Curves
Mechanical Dimensions
Accessories
- Camera
- 12V 5A Power Adapter
- Standard Accessories
- Power Cable
- 12V Self-Locking Power Cable
- 1.3m USB3.0 Cable
- 1.25-inch Extension Ring
- Desiccant Tube
- Lens Mounting Clamp
- Screwdriver
- Camera Packaging Bag
* (LPF: Light Pollution Filter; HLP: Heavy Light Pollution Filter; FCE: Four-Channel Enhancement Filter)
