The QHY11 Mono is a small full frame size 36*24mm cooled CCD camera.
It uses the TrueSense KAI11002 CCD sensor and offers a big image circle.
The 11mega pixels and 9um pixel size offer you very sharp star and wide FOV area in many telescopes.
QHY11 has typical -45C delta T from ambient.
This temperature exceeds most of other cameras based KAI11002 or KAI11000. You can get lower thermal noise and less hot pixels with this camera.
QHY11’s small round case design allow it be installed in the the Hyperstar System or in the primary focus plane. With more and more new big image circle Schmidt camera come out, QHY11 is your right choice for such systems.
QHY11 also supply a cable clip which can make the contract of the USB port and power socket more solid.
The QHY11 Colour is available for Special Order… please contact Bernard for details 😀
Total pixel :4072*2720
Active pixels:4032*2688 11Mpixels
Pixel Size: 9.0um x 9.0um square
36mm*24mm imager size
Readout noise: 12-14e- @1Mpixel/s
Preview Speed: 3Mpixel/s
Download Time: 15sec@Low Speed. 8sec@High Speed
Peak QE: 50%
Microlensing on chip
16bit ADC with CDS and Preamp
USB2.0 High Speed interface
2-Stage TEC cooling
Build in 32MByte SDRAM buffer
Build in temp sensor
DC102 DC adapter & TEC Controller Supported
Image Gallery by Terry Hancock
Terry Hancock is using QHY11 to capture many magnificent wide-angle deep sky images.
These images show perfectly the complexity of nebulea and galaxies in great detail.
Terry’s works have created a sight-seeing tour of the deep space, which you can see through his telescope and camera .
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The QHY168C is a popular APS-C format cooled colour camera. The SONY Exmor IMX071 sensor has 4.8um pixels and 2.3e- to 3.2e- read noise. This sensor has been used in the Nikon D5100 DSLR camera. With read noise this low, it’s easier to detect a dim target against background noise.
The QHY178M cooled mono camera has a 6 megapixel CMOS sensor with 8,9mm diagonal and Delta T of -40°C. Small 2.4 micron pixels make it ideal for high resolution Planetary and Lunar imaging as well as for imaging Deep Sky objects.