QHY461 (Photographic Version) + FREE Custom Adapter + Free Insured International Express Shipping
- SKU:
- QHY461-PH
- Availability:
- Accepting order now!
- Weight:
- 5.00 KGS
- Shipping:
- Calculated at Checkout
Benefiting from its back-illuminated pixel structure, the QHY411 has a large full well of 80ke-. And when using 2 * 2 binning, the full well can reach 320ke-, corresponding to a merged pixel size of 7.5um * 7.5um. Combined with the low readout noise, the camera has a large dynamic range advantage.
Updated: now QHY411 supports 3*3 onchip binning. Learn more at “QHY411 3*3 Onchip Binning 12bit (high frame rate)Mode Instructions” part.
Native 16 bit A/D: The new Sony sensor has native 16-bit A/D on-chip. The output is real 16-bits with 65536 levels. Compared to 12-bit and 14-bit A/D, a 16-bit A/D yields higher sample resolution and the system gain will be less than 1e-/ADU with no sample error noise and very low read noise.
BSI: One benefit of the back-illuminated CMOS structure is improved full well capacity. 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.
TRUE RAW Data: In the DSLR implementation there is a RAW image output, but typically it is not completely RAW. Some evidence of noise reduction and hot pixel removal is still visible on close inspection. This can have a negative effect on the image for astronomy such as the “star eater” effect. However, QHY Cameras offer TRUE RAW IMAGE OUTPUT and produces an image comprised of the original signal only, thereby maintaining the maximum flexibility for post-acquisition astronomical image processing programs and other scientific imaging applications.
Zero Amplify Glow: This is also a zero amplifer glow camera.
Cooling & Anti-dew Control: In addition to dual stage TE cooling, QHYCCD implements proprietary technology in hardware to control the dark current noise. The optic window has 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.
Sealing Technology: Based on almost 20-year cooled camera design experience, The QHY cooled camera has implemented the sealing control solutions. The sensor itself is kept dry with our silicon gel tube socket design for control of humidity within the sensor chamber. By the way, there’s no oil leaking.
(Free Custom Adapter & Insured International Express Shipping by Cyclops Optics)
QHY461 Highlights
- 100 Megapixels Full Frame sensor (44*33mm)
- Short Back Focus: 16mm
- Monochrome sensor
- 14.1 stop of dynamic range
- Backside-illuminated sensor (High QE)
- 16 Bit Analog-Digital Converter
- Ultra low 1e- read-out noise
- Very low dark current
- USB 3.0 & 10G Fiber connection
FREE Cyclops Optics Custom Adapter Fabrication Service

As usual at Cyclops Optics, we offer an exclusive FREE high precision custom fabricated adapter (original: US$150 or above) for our customers to match with your optical system. We will provide you professional opinion when designing the custom adapter to fit your needs.
Cyclops Optics International Service Center for QHYCCD
Cyclops Optics is the official dedicated QHYCCD partner to support ALL global warranty and maintenance services. This secures your reliable purchase and journey of QHYCCD products.