QHYCCD MiniCAM8 Mono Deep Sky Combo EVO

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.

High Near-Infrared 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-infrared 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-infrared band and 92% in the visible wavelength band.

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 of the 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 Amplify Glow

QHY miniCAM8 is also a zero amplifer 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.

Linearity HDR Mode

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.

See QHYCCD's website for Curve Graphs

Filters Introduction

This set includes 7 filters: LRGB and 3 nm SHO.
Compared with the original Deep Sky Filter Set, the EVO version features upgraded optical-coating technology and narrower bandpasses for the narrowband filters. The filters have an OD value of 5.

Sample Images

VdB 62 Nebula, By Abdullah Al-Harbi

• Camera: QHYCCD miniCAM8 Mono Deepsky Combo
• Telescope: Askar 600 ‎‏
• Mount: HAE EC 69 ‎‏
• Exposure: L 300*40, R 300*48, G 300*36, B 300*35, Ha 300*43
• Total integration: 16.8 hours
• Bortal class 5/6

The Rosette Nebula, By Luca Bartek

• Camera: QHYCCD miniCAM8 Mono Deepsky Combo
• Telescope: Askar FRA600
• Exposure:
  QHYCCD H-alpha 7nm: 38×600″(6h 20′)
  QHYCCD OIII 7nm: 21×600″(3h 30′)
  QHYCCD SII 7nm: 44×600″(7h 20′)
• Integration: 17h 10′

NGC 281, By Nicolas Bricaud

• Camera: miniCAM8M gain 78/ offset 50-Linearity HDR mode
• Telescope: doublet refractor TS72/420 ED with 0.79X corrector / reducer
• Mount: Sky-Watcher Star Adventurer Gti mount
• Frames: 5x300s with Sll filter, 10x300s with Ha filter and 5x300s with Olll filter

Graphics

The peak quantum efficiency of the miniCAM8M reaches 91.2% in the OIII band, 80.9% in the Ha band, 78.7% in the SII band, and 40.1% in the methane band.

Technical Specifications

Mechanical Drawing:

In the Box

MiniCAM8M EVO COMBO

• Camera
• 12V 5A Power Adapter    
• 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
• LRGB + 3nm SHO Filter 

Manual & Warranty

QHYCCD 2-Years Warranty

Full Camera Manual