{"product_id":"qhy-268c-cooled-aps-c-back-illuminated-color-camera-110058","title":"QHY 268C PH  SBFL - Cooled Back-Illuminated Color Camera - APS-C Sensor - 110058","description":"\u003cp style=\"text-align: center;\"\u003e\u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0851\/2766\/files\/268_Square_Banner.jpg?v=1773692581\" alt=\"\"\u003e\u003c\/p\u003e\n\u003cp\u003eWith the advantage of low readout noise and high-speed readout, CMOS technology has revolutionized astronomical imaging. A color, back-illuminated, high-sensitivity astronomical imaging camera and still image video camera is the ideal choice for astro-imagers.\u003c\/p\u003e\n\u003cp\u003eThe QHY268C PH is a cooled, back-illuminated color CMOS camera based on the Sony IMX571 sensor with true 16-bit A\/D and 3.76μm pixels. This Sony sensor is an ideal CMOS sensor exhibiting no amplifier glow. 16-bit A\/D gives high-resolution sampling of the whole full well range. Digitizing 0-65535 levels yields a smooth image with a continuous gradation of greyscale levels.\u003c\/p\u003e\n\u003ch3\u003eFeatures\u003c\/h3\u003e\n\u003cp\u003e\u003cspan\u003e\u003cstrong\u003e1GB DDR3 image buffer\u003c\/strong\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cspan\u003eIn order to provide smooth uninterrupted data transfer of the entire 26MP sensor at high speed, the QHY268 has 1GB DDR3 image buffer. The pixel count of the latest generation of CMOS sensors is very high resulting in greater memory requirements for temporary and permanent storage.  \u003c\/span\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cspan\u003eThe QHY268 has adopted a large-capacity memory of up to 1GB.  Data throughput is doubled. This large image buffer meets the needs of high-speed image acquisition and transmission of the new generation of CMOS, making shooting of multiple frames smoother and less stuttered, further reducing the pressure on the computer CPU.\u003c\/span\u003e\u003cspan\u003e\u003cstrong\u003e\u003c\/strong\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cstrong\u003eNative 16 bit A\/D: \u003c\/strong\u003eThe Sony IMX571 sensor has native 16-bit A\/D on-chip. The output is real 16-bits with \u003cstrong\u003e65536 levels\u003c\/strong\u003e. 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.\u003c\/p\u003e\n\u003cp\u003e\u003cstrong\u003eBSI: \u003c\/strong\u003eOne 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.\u003c\/p\u003e\n\u003cp\u003e\u003cstrong\u003eTRUE RAW Data: \u003c\/strong\u003eIn 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. \u003c\/p\u003e\n\u003cp\u003eHowever,  QHY offers 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.\u003c\/p\u003e\n\u003cp\u003e\u003cstrong\u003eZero Amplify Glow: \u003c\/strong\u003eThis is also a zero amplifier glow camera.\u003c\/p\u003e\n\u003cp\u003e\u003cstrong\u003eCooling \u0026amp; Anti-dew Control: \u003c\/strong\u003eIn 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.\u003c\/p\u003e\n\u003cp\u003e\u003cstrong\u003eSealing Technology: \u003c\/strong\u003eBased 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.\u003c\/p\u003e\n\u003cdiv class=\"block lv3 on\"\u003e\n\u003cdiv id=\"c110\" class=\"tit\"\u003e\n\u003cstrong\u003eMultiple Readout Modes: \u003c\/strong\u003e Multiple Readout Modes are special for QHY 16-bit Cameras (QHY600\/268\/461\/411).  Different readout modes have different driver timing, etc., and result in different performance.\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"block lv3 on\"\u003e\n\u003cdiv class=\"cnt\"\u003e\n\u003cp\u003e\u003cspan\u003eYou may find some types of thermal noise can change with time in some back-illuminated CMOS cameras. This thermal noises has the characteristic of the fixed position of typical thermal noise, but the value is not related to the exposure time.  Instead, each frame appears to have its own characteristics.  The QHY600\/268\/461\/411 use an innovative suppression technology that can significantly reduce the apparent level of such noise.\u003c\/span\u003e\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"block lv3 on\"\u003e\n\u003cdiv id=\"c112\" class=\"tit\"\u003e\n\u003cstrong\u003eUVLO Protection: \u003c\/strong\u003e \u003cspan\u003eUVLO (Under Voltage Locking) is to protect the electronic device from damage caused by abnormally low voltages.\u003c\/span\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"cnt\"\u003e\n\u003cp\u003e\u003cspan\u003eOur daily life experience tells us that the actual operational voltage of an electrical device must not significantly exceed the rated voltage, otherwise it will be damaged. \u003c\/span\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cspan\u003eFor such precision equipment as cameras, long-term work at too low input voltage can also be detrimental to the working life of the camera, and may even make some devices, such as power manager, burn up due to long-term overload. In the all-in-one driver and SDK after 2021.10.23 stable version, the camera will give a warning when the input voltage of the camera is below 11V.\u003c\/span\u003e\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"block lv3 on\"\u003e\n\u003cdiv id=\"c113\" class=\"tit\"\u003e\n\u003cstrong\u003eOptimizing USB Traffic to Minimize Horizontal Banding: \u003c\/strong\u003eIt is common behavior for a CMOS sensor to contain some horizontal banding. Normally, random horizontal banding can be removed with multiple frame stacking so it does not affect the final image. However, periodic horizontal banding is not removed with stacking so it may appear in the final image. By adjust the USB traffic in Single Frame mode or Live Frame mode, you can adjust the frequency of the CMOS sensor driver and it can optimize the horizontal banding appeared on the image. This optimized is very effective to remove the periodic banding in some conditions.\u003c\/div\u003e\n\u003cdiv class=\"tit\"\u003e\u003cbr\u003e\u003c\/div\u003e\n\u003cdiv class=\"tit\"\u003e\n\u003cdiv id=\"c114\" class=\"tit\"\u003e\n\u003cstrong\u003eReboot the camera by power off and on: \u003c\/strong\u003eThe camera is designed to use the +12V to reboot the camera without disconnecting and reconnecting the USB interface. This means that you can reboot the camera simply by shutting down the +12V and then powering it back on. This feature is very handy for remote controlling the camera in an observatory. You can use a remotely controlled power supply to reboot the camera. There is no need to consider how to reconnect the USB in the case of remote control.\u003c\/div\u003e\n\u003cdiv class=\"tit\"\u003e\u003cbr\u003e\u003c\/div\u003e\n\u003cdiv class=\"tit\"\u003e\n\u003cdiv id=\"a2\" class=\"tit\"\u003e\u003cstrong\u003eMultiple Readout Modes and Curves: \u003c\/strong\u003e\u003c\/div\u003e\n\u003cdiv class=\"tit\"\u003e\n\u003cstrong\u003e\u003c\/strong\u003e\u003cbr\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"tit\"\u003e\n\u003cp\u003eMultiple Readout Modes are special for QHY 16-bit Cameras (QHY600\/268\/461\/411).  Different readout modes result in different performance. These readout modes are currently supported in the ASCOM, SharpCap and N.I.N.A.\u003c\/p\u003e\n\u003cp style=\"text-align: center;\"\u003e\u003cimg alt=\"\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0851\/2766\/files\/QHY268_Curves.png?v=1773689563\"\u003e\u003c\/p\u003e\n\u003cp style=\"text-align: center;\"\u003e\u003cimg alt=\"\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0851\/2766\/files\/268_Dynamic_Range.png?v=1773689704\"\u003e\u003c\/p\u003e\n\u003cp style=\"text-align: center;\"\u003e\u003cimg alt=\"\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0851\/2766\/files\/268_Full_Well.png?v=1773689703\"\u003e\u003c\/p\u003e\n\u003cp style=\"text-align: center;\"\u003e\u003cimg alt=\"\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0851\/2766\/files\/268_Readout.png?v=1773689703\"\u003e\u003c\/p\u003e\n\u003cp style=\"text-align: center;\"\u003e\u003cimg alt=\"\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0851\/2766\/files\/268_Dark_Current_vs_Temp.png?v=1773689704\"\u003e\u003c\/p\u003e\n\u003cp style=\"text-align: center;\"\u003e\u003cimg alt=\"\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0851\/2766\/files\/268_QE.jpg?v=1773689704\"\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cstrong\u003ePhotographic DSO Mode (Mode #0)\u003c\/strong\u003e\u003c\/p\u003e\n\u003cp\u003eThis mode is suitable for most DSO imaging situations. Since there is a drop in the noise between Gain 25 and Gain 26 (unity gain), we recommend it as default gain setting; however, gain0 is also good enough for a 16-bit sensor.\u003c\/p\u003e\n\u003cp\u003e\u003cstrong\u003eHigh Gain Mode  (Mode #1)\u003c\/strong\u003e\u003c\/p\u003e\n\u003cp\u003eThis mode is something like double native iso of some new digital cameras, whose danamic range can greatly incerase at the vary high iso value, like iso800, iso3200, etc. The high gain mode provide such improvement for QHYCCD 16bit cameras.\u003c\/p\u003e\n\u003cp\u003eWe recommend you choose this mode when you have to capture at high gain, for example, a vary dark object. \u003cstrong\u003ePlease note the switch point of HGC\/LGC of QHY600\/268\/461 is 56. That means you must set Gain 56 to make the best of it.\u003c\/strong\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cstrong\u003eExtended Fullwell Mode \u003c\/strong\u003e\u003cstrong\u003e(Mode#2) \u003c\/strong\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cspan\u003eWith a pixel size of 3.76um, these sensors already have an impressive full well capacity of 51ke. Nevertheless, QHYCCD has implemented a unique approach to achieve a full well capacity higher than 51ke- through innovative user controllable read mode settings. In Extended Fullwell Mode, the QHY600 can achieve an extremely large full-well charge value of nearly 80ke- and the QHY268 can achieve nearly 75ke-. Greater full-well capacity provides greater dynamic range and large variations in magnitude of brightness are less likely to saturate. \u003c\/span\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cstrong\u003e2CMS Modes\u003c\/strong\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cstrong\u003eExtended Fullwell Mode-2CMS (Mode#3)\u003c\/strong\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cstrong\u003ePhotographic DSO Mode-2CMS (Mode#4)\u003c\/strong\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cstrong\u003eHigh Gain Mode-2CMS (Mode#5)\u003c\/strong\u003e\u003c\/p\u003e\n\u003cp\u003eBased on the three basic modes above, 2CMS mode can greatly reduce readout noise by secondary sampling while keeping the same full well value and system gain. We prefer 2CMS modes than basic modes in astrophotography. By the way, the recommend gain values are the same as their basic modes.\u003c\/p\u003e\n\u003ch3\u003eSpecifications\u003c\/h3\u003e\n\u003ctable\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eModel\u003c\/td\u003e\n\u003ctd width=\"572\"\u003eQHY268C PH\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eCMOS Sensor\u003c\/td\u003e\n\u003ctd width=\"572\"\u003eSONY IMX571\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eMono\/Color\u003c\/td\u003e\n\u003ctd width=\"572\"\u003eColor\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eFSI\/BSI\u003c\/td\u003e\n\u003ctd width=\"572\"\u003eBSI\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003ePixel Size\u003c\/td\u003e\n\u003ctd width=\"572\"\u003e3.76μm*3.76μm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eEffective Pixel Area\u003c\/td\u003e\n\u003ctd width=\"572\"\u003e6252*4176\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eTotal Pixel Area\u003c\/td\u003e\n\u003ctd width=\"572\"\u003e6280*4210 (include optical black area and overscan area)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eEffective Pixels\u003c\/td\u003e\n\u003ctd width=\"572\"\u003e26 Megapixels\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eSensor Size\u003c\/td\u003e\n\u003ctd width=\"572\"\u003eAPS-C\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eA\/D\u003c\/td\u003e\n\u003ctd width=\"572\"\u003eNative 16-bit (0-65535 greyscale) A\/D\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eFull Well Capacity (1×1, 2×2, 3×3)\u003c\/td\u003e\n\u003ctd width=\"572\"\u003eStandard Mode\u003cbr\u003e51ke-\u003cbr\u003eExtended Full Well Mode\u003cbr\u003e80ke-\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eFrame Rates\u003c\/td\u003e\n\u003ctd width=\"572\"\u003eFull Resolution:\n\u003cp\u003e \u003c\/p\u003e\n\u003cp\u003e6.8FPS@8bit, 6FPS@16bit\u003c\/p\u003e\n\u003cp\u003ein 12 bit High Speed Mode: 8-bit, (12-bit out), 14.5fps max\u003c\/p\u003e\n\u003cp\u003eROI:\u003c\/p\u003e\n\u003cp\u003e2048lines, 13.6FPS@8bit, 11.5FPS@16bit\u003cbr\u003e1080lines, 25.4FPS@8bit, 19.5FPS@16bit\u003cbr\u003e768lines, 35FPS@8bit, 25FPS@16bit\u003cbr\u003e480lines, 50FPS@8bit, 34FPS@16bit\u003c\/p\u003e\n\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eReadout Noise\u003c\/td\u003e\n\u003ctd width=\"572\"\u003e1.1e- to 3.5e-\u003cbr\u003e(5.3e- to 7.4e- in Extended Full Well Mode)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eDark Current\u003c\/td\u003e\n\u003ctd width=\"572\"\u003e0.0005 e-\/pixel\/sec@-20℃，\u003cbr\u003e0.001 e-\/pixel\/sec@-10℃\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eExposure Time Range\u003c\/td\u003e\n\u003ctd width=\"572\"\u003e30μs-3600sec\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eRecommend Gain\u003c\/td\u003e\n\u003ctd width=\"572\"\u003e30 (PH Mode, or Extended Full Well Mode)\u003cbr\u003e56 (High Gain Mode)\u003cbr\u003e\u003cbr\u003e\n\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eAmp Control\u003c\/td\u003e\n\u003ctd width=\"572\"\u003eZero Amplifer Glow\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eShutter Type\u003c\/td\u003e\n\u003ctd width=\"572\"\u003eElectronic Rolling Shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eComputer Interface\u003c\/td\u003e\n\u003ctd width=\"572\"\u003eUSB3.0\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eBuilt-in Image Buffer\u003c\/td\u003e\n\u003ctd width=\"572\"\u003e1GB DDR3 Memory Buffer\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eCooling System\u003c\/td\u003e\n\u003ctd width=\"572\"\u003eDual Stage TEC cooler:\u003cbr\u003e– Long exposures (\u0026gt; 1 second) typically -35℃ below ambient\u003cbr\u003e– Short exposure (\u0026lt; 1second) high FPS, typically -30℃ below ambient（Test temperature +20℃）\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eOptic Window Type\u003c\/td\u003e\n\u003ctd width=\"572\"\u003eAR+AR High Quality Multi-Layer Anti-Reflection Coating\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eTelescope Interface\u003c\/td\u003e\n\u003ctd width=\"572\"\u003eSupport M54 or M48 (Combined with adapters )\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eBack Focal Length\u003cbr\u003e\u003cbr\u003e\n\u003c\/td\u003e\n\u003ctd width=\"572\"\u003e14.5mm（±0.2）\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eAnti-Dew Heater\u003c\/td\u003e\n\u003ctd width=\"572\"\u003eAvailable\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eHumidity Sensor\u003c\/td\u003e\n\u003ctd width=\"572\"\u003eNo, available in QHY268M only\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eFirmware\/FPGA remote Upgrade\u003c\/td\u003e\n\u003ctd width=\"572\"\u003eAvailable via Camera USB port\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd width=\"267\"\u003eWeight\u003c\/td\u003e\n\u003ctd width=\"572\"\u003e810g\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003cp\u003e \u003c\/p\u003e\n\u003ch3\u003eWhat's in the Box\u003c\/h3\u003e\n\u003cul\u003e\n\u003cli\u003eCamera\u003c\/li\u003e\n\u003cli\u003e\n\u003cmeta charset=\"UTF-8\"\u003e \u003cspan\u003eLocking Power Cable\u003c\/span\u003e\n\u003c\/li\u003e\n\u003cli\u003e\u003cspan\u003eUSB 3.0 Cable\u003c\/span\u003e\u003c\/li\u003e\n\u003cli\u003e\u003cspan\u003e12V Power Adapter\u003c\/span\u003e\u003c\/li\u003e\n\u003cli\u003e\u003cspan\u003eAV Power Cable\u003c\/span\u003e\u003c\/li\u003e\n\u003cli\u003e\u003cspan\u003eDesiccant Tube\u003c\/span\u003e\u003c\/li\u003e\n\u003cli\u003e\u003cspan\u003eM54 to 2” Nosepiece\u003c\/span\u003e\u003c\/li\u003e\n\u003cli\u003e\u003cspan\u003e5mm M54 Adapter\u003c\/span\u003e\u003c\/li\u003e\n\u003cli\u003e\u003cspan\u003e3mm M54 Adapter\u003c\/span\u003e\u003c\/li\u003e\n\u003cli\u003e\u003cspan\u003e3mm M54-M42 Adapter\u003c\/span\u003e\u003c\/li\u003e\n\u003cli\u003e\u003cspan\u003eDrive Download Instructions\u003c\/span\u003e\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003cdv class=\"cnt\"\u003e\u003cp\u003e\u003cstrong\u003eReadout Mode #0 (Photographic Mode)\u003c\/strong\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cstrong\u003eReadout Mode #1 (High Gain Mode)\u003c\/strong\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cstrong\u003eReadout Mode #2 (Extended Full Well Mode)\u003c\/strong\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cstrong\u003eReadout Mode #3 (Extend Full Well Mode-2CMS)\u003c\/strong\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cstrong\u003eReadout Mode #4 (Photographic Mode-2CMS)\u003c\/strong\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cstrong\u003eReadout Mode #5 (High Gain Mode-2CMS)\u003c\/strong\u003e\u003c\/p\u003e\u003c\/dv\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"QHYCCD","offers":[{"title":"Default Title","offer_id":43001628459121,"sku":"QHY-110058","price":2207.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0851\/2766\/files\/QHY268_Body_48cdbfae-e1fa-412f-a733-bdb32bac5ff5.jpg?v=1773690724","url":"https:\/\/khanscope.com\/products\/qhy-268c-cooled-aps-c-back-illuminated-color-camera-110058","provider":"Khan Scope Centre","version":"1.0","type":"link"}