{"title":"Zwo camera 1.25 inch planetary","description":"","products":[{"product_id":"zwo-asi183mc-colour","title":"ZWO ASI183MC Colour CMOS Camera","description":"\u003ch2\u003eThe ASI183MC, ZWO's most sensitive camera to date with a peak absolute Q.E. of 84% in mono made possible by a back illuminated sensor.\u003c\/h2\u003e\n\u003cp\u003e\u003cbr\u003e\u003c\/p\u003e\n\u003cp\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/Logo-of-183MM-MC_EF_BC_88_E6_96_B0_EF_BC_89_jpg.png\"\u003e\u003cimg class=\"aligncenter size-full wp-image-8909\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/Logo-of-183MM-MC_EF_BC_88_E6_96_B0_EF_BC_89_jpg.png\" alt=\"Logo-of-183MM MC（新）.jpg\" width=\"750\" height=\"268\"\u003e\u003c\/a\u003e\u003c\/p\u003e\n\u003ch2\u003eIntroducing the ASI183 camera series, the most sensitivie cameras in ZWO history. Peak Q.E. of the mono sensor reaches 84%!\u003c\/h2\u003e\n\u003cdiv id=\"tmpl_contentMenu_bar\"\u003e\n\u003cdiv id=\"sidGlobalnav\"\u003e\n\u003cdiv id=\"tmpl_contentMenu_bar_base\"\u003e\n\u003cdiv id=\"nav2nd\"\u003e\n\u003ch3\u003e▶IMX183CLK-J\/CQJ-J\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv id=\"tmpl_main\"\u003e\n\u003cdiv id=\"sidContents\"\u003e\n\u003cdiv class=\"section btm_bd\"\u003e\n\u003cp\u003eDiagonal 15.86 mm Approx. 20.48M-Effective Pixel Monochrome\/Color CMOS Image Sensor\u003c\/p\u003e\n\u003cp\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/IMX183CQJ-4K-Sensor.png\"\u003e\u003cimg class=\"aligncenter size-full wp-image-8842\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/IMX183CQJ-4K-Sensor.png\" alt=\"IMX183CQJ-4K-Sensor\" width=\"257\" height=\"150\"\u003e\u003c\/a\u003e\u003c\/p\u003e\n\u003ch3\u003e▶High-Speed and High-Picture-Quality Rolling Shutter-Type Back-Illuminated CMOS Image Sensors\u003c\/h3\u003e\n\u003cp\u003eIn the astronomic application field, Sony IMX183CLK-J (monochrome) and IMX183CQJ-J (color) sensors uses a very high sensitivity back-illuminated structure with high resolution 2.4 μm square unit pixel. The optical size is \u003cstrong\u003e1 inch\u003c\/strong\u003e.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003ch2\u003eAstrophotography Performance\u003c\/h2\u003e\n\u003cp\u003eThe ASI183 cameras has a very large full well capacity（\u003cstrong\u003e15000e\u003c\/strong\u003e） for such small pixel size, \u003cstrong\u003e1.6e\u003c\/strong\u003e read noise @ 30DB, and \u003cstrong\u003e12stops\u003c\/strong\u003e dynamic range @ Gain=0. The ASI183 cameras also utilize firmware features to minimize amplifier glow for maximum performance in astrophotography.\u003c\/p\u003e\n\u003cp\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/183-Gain-RN-DR-FW-vs-gain1.jpg\"\u003e\u003cimg class=\"aligncenter size-full wp-image-8847\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/183-Gain-RN-DR-FW-vs-gain1.jpg\" alt=\"183 Gain RN DR FW vs gain\" width=\"750\" height=\"1334\"\u003e\u003c\/a\u003e\u003c\/p\u003e\n\u003ch2\u003e\u003cstrong\u003eHigh Speed\u003c\/strong\u003e\u003c\/h2\u003e\n\u003cp\u003eFast FPS can be used in solar and lunar imaging, as well as for live viewing\/EAA.The high speed readout may also be used for real-time focusing, true lucky imaging of double stars and other small objects, planetary imaging of the major planets in the solar system, and much more.\u003c\/p\u003e\n\u003cp\u003e\u003cstrong\u003e10Bit ADC\u003c\/strong\u003e\u003cbr\u003e5496×3672 19fps\u003cbr\u003e3840×2160 41.04fps\u003cbr\u003e1920×1080 80.10fps\u003cbr\u003e1280×720 117.30fps\u003cbr\u003e\u003cstrong\u003e12bit ADC \u003c\/strong\u003e\u003cbr\u003e5496×3672 19fps\u003cbr\u003e3840×2160 36.12fps\u003cbr\u003e1920×1080 70.48fps\u003cbr\u003e1280×720 103.23fps\u003c\/p\u003e\n\u003ch2\u003eHigh QE\u003c\/h2\u003e\n\u003cp\u003eSony’s back-illuminated Exmor R technology, giving it excellent Deep Sky performance. ASI183 QE peak reaches a remarkable 84%. In Ha channel, QE is still over 60%.\u003c\/p\u003e\n\u003cp\u003eHaving high QE means more of the light that enters your telescope and reaches the sensor is actually used. With 84% peak Q.E. and no less than ~50% within the visible spectrum, the ASI183 will utilize a high percentage of the light that reaches it, improving your signal quality.\u003c\/p\u003e\n\u003cp\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/183QE1.jpg\"\u003e\u003cimg class=\"aligncenter size-full wp-image-8848\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/183QE1.jpg\" alt=\"183QE\" width=\"750\" height=\"420\"\u003e\u003c\/a\u003e\u003c\/p\u003e\n\u003ch2\u003eUSB 3.0 Port \u0026amp; ST4 Port\u003c\/h2\u003e\n\u003cp\u003e\u003cstrong\u003eUSB 3.0 Port: \u003c\/strong\u003eProvide 5Gb bandwidth to make it possible for ASI183 to run at 19 fps (12bit, normal mode) or 19 fps (10bit, high speed mode) at full resolution(20.18Mega).\u003c\/p\u003e\n\u003cp\u003e\u003cstrong\u003eST4 Port: \u003c\/strong\u003eCan be used connect with auto guide port of mount, for guiding.\u003c\/p\u003e\n\u003cp\u003e \u003c\/p\u003e\n\u003cp\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/183MC.jpg\"\u003e\u003cimg class=\"aligncenter wp-image-8894\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/183MC.jpg\" alt=\"183MC\" width=\"400\" height=\"400\"\u003e\u003c\/a\u003e\u003c\/p\u003e\n\u003ch2\u003e\u003ca href=\"\/wp-content\/uploads\/2017\/11\/ZWO_ASI183_Manual_EN.pdf\"\u003e\u003cspan style=\"color: #0000ff;\"\u003eASI 183MC Instruction Manual\u003c\/span\u003e\u003c\/a\u003e\u003c\/h2\u003e\n\u003ch2\u003eMechanical Drawing\u003c\/h2\u003e\n\u003cp\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/asi183-Mechanical-Drawing.jpg\"\u003e\u003cimg class=\"aligncenter size-full wp-image-8896\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/asi183-Mechanical-Drawing.jpg\" alt=\"asi183-Mechanical-Drawing\" width=\"700\" height=\"500\"\u003e\u003c\/a\u003e\u003c\/p\u003e\n\u003ch2\u003eWhat is in the box?\u003c\/h2\u003e\n\u003cp\u003eASI183 box includes all necessary cables, adapters, and manuals.\u003c\/p\u003e\n\u003cp\u003e\u003ca href=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/183PACKAGE-1024x7681.jpg\"\u003e\u003cimg class=\"aligncenter size-full wp-image-8915\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/183PACKAGE-1024x7681.jpg\" alt=\"183PACKAGE-1024x768\" width=\"750\" height=\"366\"\u003e\u003c\/a\u003e\u003c\/p\u003e\n\u003c!-- Camera Technical Details --\u003e\n\u003ch3 style=\"color:#000;\"\u003eCamera Technical Details\u003c\/h3\u003e\n\u003ctable style=\"width:100%; border-collapse:collapse;\"\u003e\n  \u003ctbody\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e\u003cstrong\u003eSensor\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e1″ CMOS IMX183CLK-J \/ CQJ-J\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e\u003cstrong\u003eSensor Diagonal\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e15.9 mm\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e\u003cstrong\u003eResolution\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e20.18 MP (5496 × 3672)\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e\u003cstrong\u003ePixel Size\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e2.4 μm\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e\u003cstrong\u003eBayer Pattern\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003eRGGB\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e\u003cstrong\u003eShutter Type\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003eRolling shutter\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e\u003cstrong\u003eExposure Range\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e32 μs – 2000 s\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e\u003cstrong\u003eROI\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003eSupported\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e\u003cstrong\u003eST4 Guider Port\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003eYes\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e\u003cstrong\u003eRead Noise\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e1.6 e⁻ @ 30 dB gain\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e\u003cstrong\u003eQE Peak\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e84%\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e\u003cstrong\u003eFull Well Capacity\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e15 ke⁻\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e\u003cstrong\u003eADC\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e12-bit\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e\u003cstrong\u003eInterface\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003eUSB 3.0 \/ USB 2.0\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e\u003cstrong\u003eAdaptor\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e2″ \/ 1.25″ \/ M42 × 0.75\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e\u003cstrong\u003eDimensions\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003eφ62 mm × 36 mm\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e\u003cstrong\u003eWeight\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e120 g (4.2 oz, without lens)\u003c\/td\u003e\n\u003c\/tr\u003e\n  \u003c\/tbody\u003e\n\u003c\/table\u003e\n\n\u003c!-- Environmental Conditions --\u003e\n\u003ch3 style=\"color:#000;\"\u003eEnvironmental Conditions\u003c\/h3\u003e\n\u003ctable style=\"width:100%; border-collapse:collapse;\"\u003e\n  \u003ctbody\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e\u003cstrong\u003eWorking Temperature\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e−5°C to 45°C\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e\u003cstrong\u003eStorage Temperature\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e−20°C to 60°C\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e\u003cstrong\u003eWorking Relative Humidity\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e20% – 80%\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e\u003cstrong\u003eStorage Relative Humidity\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e20% – 95%\u003c\/td\u003e\n\u003c\/tr\u003e\n  \u003c\/tbody\u003e\n\u003c\/table\u003e\n\n\u003c!-- Max FPS - 10-bit ADC --\u003e\n\u003ch3 style=\"color:#000;\"\u003eMax FPS at Full Resolution (10-bit ADC)\u003c\/h3\u003e\n\u003ctable style=\"width:100%; border-collapse:collapse;\"\u003e\n  \u003cthead\u003e\n    \u003ctr\u003e\n      \u003cth style=\"padding:10px; border:1px solid #ddd; text-align:left;\"\u003eResolution\u003c\/th\u003e\n      \u003cth style=\"padding:10px; border:1px solid #ddd; text-align:left;\"\u003eMax FPS\u003c\/th\u003e\n    \u003c\/tr\u003e\n  \u003c\/thead\u003e\n  \u003ctbody\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e5496 × 3672\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e19 fps\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e3840 × 2160\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e41.04 fps\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e1920 × 1080\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e80.10 fps\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e1280 × 720\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e117.30 fps\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e640 × 480\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e169.92 fps\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e320 × 240\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e308.17 fps\u003c\/td\u003e\n\u003c\/tr\u003e\n  \u003c\/tbody\u003e\n\u003c\/table\u003e\n\n\u003c!-- Max FPS - 12-bit ADC --\u003e\n\u003ch3 style=\"color:#000;\"\u003eMax FPS at Full Resolution (12-bit ADC)\u003c\/h3\u003e\n\u003ctable style=\"width:100%; border-collapse:collapse;\"\u003e\n  \u003cthead\u003e\n    \u003ctr\u003e\n      \u003cth style=\"padding:10px; border:1px solid #ddd; text-align:left;\"\u003eResolution\u003c\/th\u003e\n      \u003cth style=\"padding:10px; border:1px solid #ddd; text-align:left;\"\u003eMax FPS\u003c\/th\u003e\n    \u003c\/tr\u003e\n  \u003c\/thead\u003e\n  \u003ctbody\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e5496 × 3672\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e19 fps\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e3840 × 2160\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e36.12 fps\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e1920 × 1080\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e70.48 fps\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e1280 × 720\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e103.23 fps\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e640 × 480\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e149.53 fps\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003ctr\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e320 × 240\u003c\/td\u003e\n\u003ctd style=\"padding:10px; border:1px solid #ddd;\"\u003e271.19 fps\u003c\/td\u003e\n\u003c\/tr\u003e\n  \u003c\/tbody\u003e\n\u003c\/table\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":42045233791045,"sku":"ASI183MC","price":849.0,"currency_code":"AUD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/zwo-asi183mc-colour-cmos-camera-214502.jpg?v=1731541396"},{"product_id":"zwo-asi585mc","title":"ZWO ASI585MC Colour Camera","description":"\u003ch2 style=\"text-align: center;\"\u003eAstronomical OSC camera with large full well capacity\u003cbr\u003eASI585MC\u003c\/h2\u003e\n\u003cp style=\"text-align: center;\"\u003eASI585MC adopts Sony IMX585 CMOS sensor. As one of ZWO's latest OSC planetary cameras, it features a large sensor format of 1\/1.2\", a high resolution of 3840*2160, and a surprisingly amazing characteristic of ZERO AMP GLOW! The pixel size is 2.9um*2.9um. In 12-bit mode, it produces 46.9 FPS with super low readout noise!\u003c\/p\u003e\n\u003cp\u003e \u003c\/p\u003e\n\u003ch2 style=\"text-align: center;\"\u003e\u003cimg height=\"442\" width=\"800\" alt=\"ASI585MC\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/asi585mc-copy-800x442.jpg\" title=\"ASI585MC\" class=\"aligncenter wp-image-122042 size-medium\"\u003e\u003c\/h2\u003e\n\u003cp\u003e \u003c\/p\u003e\n\u003ch4 style=\"text-align: center;\"\u003e8.29MP Senor\u003c\/h4\u003e\n\u003cp style=\"text-align: center;\"\u003eASI585MC has the same pixel size of the ASI462MC at 2.9um, but its resolution is 4 times that of ASI462MC, which is a total of 8.29 megapixels. The sensor size is 11.13*6.26mm, and the diagonal length is 12.84mm. The 1\/1.2\" large sensor format makes it very suitable for solar and lunar imaging. It can also be used as an all-sky camera or live camera to observe and monitor cloud cover, rain, meteors and other weather conditions.\u003c\/p\u003e\n\u003cp\u003e\u003cimg height=\"470\" width=\"682\" alt=\"ASI585MC\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/asi585mc2-copy-800x551.jpg\" class=\"aligncenter wp-image-122043\"\u003e\u003c\/p\u003e\n\u003ch4 style=\"text-align: center;\"\u003eSTARVIS 2\u003c\/h4\u003e\n\u003cp style=\"text-align: center;\"\u003eASI585MC adopts the Latest SONY IMX585 sensor with STARVIS 2 technology. Featuring zero amp glow, lower dark current noise, and 3 times larger full well capacity, this camera is regarded as an upgrade of ASI485MC. It is also more sensitive to red, green and near infrared (NIR) lights compared to ASI485MC, especially in \u0026gt;850nm wavelength range, its light sensitivity is 1.5 times greater than ASI485MC.\u003c\/p\u003e\n\u003cp\u003e\u003cimg height=\"249\" width=\"800\" alt=\"\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/asi585mc3-copy-800x249.jpg\" style=\"text-align: center;\" class=\"size-medium wp-image-122046 aligncenter\"\u003e\u003c\/p\u003e\n\u003cp\u003e \u003c\/p\u003e\n\u003ch4 style=\"text-align: center;\"\u003eUpgraded Model\u003c\/h4\u003e\n\u003cp style=\"text-align: center;\"\u003eThe ASI585MC is an upgraded camera to the ASI485MC. Compared with the ASI485MC, it has the characteristics of a larger full well depth and no amp glow.\u003cbr\u003eModel \u003cimg height=\"587\" width=\"547\" alt=\"\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/asi585mc4-copy-745x800.jpg\" class=\"wp-image-122047 aligncenter\"\u003e\u003c\/p\u003e\n\u003ch4 style=\"text-align: center;\"\u003eLarge Full Well Depth\u003c\/h4\u003e\n\u003cp style=\"text-align: center;\"\u003eThanks to the back-illuminated sensor structure and advanced pixel technology, the camera has very low readout noise and a large full well depth. Especially in low light conditions, the camera performs excellent, capturing very clear images of celestial objects.\u003c\/p\u003e\n\u003ch4 style=\"text-align: left;\"\u003eCamera Curve\u003c\/h4\u003e\n\u003ch5 style=\"text-align: left;\"\u003eLow read noise, high dynamic range\u003c\/h5\u003e\n\u003cp style=\"text-align: left;\"\u003eThe camera has a built-in HCG mode, which can effectively reduce readout noise at high gain and allow the camera to maintain the same high dynamic range as it does low gain. When the gain is 252, the HCG mode is automatically turned on and the Dynamic range reaches a level close to 12bit. \u003c\/p\u003e\n\u003cp style=\"text-align: left;\"\u003eThe readout noise is as low as 1.5.\u003c\/p\u003e\n\u003cp style=\"text-align: center;\"\u003e\u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/585mc_update2.jpg?v=1742865314\" alt=\"\"\u003e\u003c\/p\u003e\n\u003cp style=\"text-align: center;\"\u003e\u003cimg height=\"784\" width=\"800\" alt=\"\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/asi585mc7-800x784.jpg\" class=\"alignnone size-medium wp-image-122051\"\u003e \u003cimg height=\"631\" width=\"800\" alt=\"\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/asi585mc9-800x631.jpg\" class=\"size-medium wp-image-122052 aligncenter\"\u003e\u003cimg height=\"800\" width=\"456\" alt=\"\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/asi585mc8-456x800.jpg\" class=\"size-medium wp-image-122053 aligncenter\"\u003eaintain the same high dyn\u003cimg height=\"631\" width=\"800\" alt=\"\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/asi585mc9-800x631.jpg\" class=\"size-medium wp-image-122052 aligncenter\"\u003eamic range as it does at low gain. When the gain is 150, the HCG mode is automatically turned on and the dynamic range reaches a level close to 12bit. The readout noise is as low as 0.8e.\u003c\/p\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":42045270425669,"sku":"ZWO-ASI585MC","price":669.0,"currency_code":"AUD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/zwo-asi585mc-836391.jpg?v=1731541425"},{"product_id":"zwo-asi-662mc-colour-camera","title":"ZWO ASI 662MC Colour Camera","description":"\u003ch6\u003eThe NEW ZWO ASI 662MC One Shot Color Camera with High Sensitivity\u003c\/h6\u003e\n\u003cp\u003eThe new ZWO ASI 662MC adopts the Sony IMX662 sensor, has a rolling shutter, a frame size of 1\/2.8\", and a pixel size of 2.9um, and has 2.07million pixels (1920 x 1080). In high-speed mode, the CMOS sensor can output 102.6 frames per second at full resolution and provide a low read noise level.\u003c\/p\u003e\n\u003cp\u003e\u003cimg class=\"wp-image-126217 aligncenter\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI662MC-c.jpg\" alt=\"\" width=\"571\" height=\"313\"\u003e\u003c\/p\u003e\n\u003ch6\u003eLarge Full Well capacity, not easy to overexposure\u003c\/h6\u003e\n\u003cp\u003eThe ZWO ASI 662MC adopts the Sony 662MC sensor with the latest technology. Compared to the previous generation of sensors, it has a very low readout noise and extremely large full well capacity which is 3 times larger than that of the IMX462MC. This helps effectively with overexposure issues and allows longer exposure s. In low light conditions, the camera performs excellently, capturing very clear images of celestial objects.\u003c\/p\u003e\n\u003ch6\u003eSTARVIS 2\u003c\/h6\u003e\n\u003cp\u003eZWO ASI 662MC adopts the latest Sony IMX662 sensor with advanced STARVIS 2 technology. \u003cstrong\u003eFeaturing zero amp glow, higher sensitivity to red and Near Infrared (NIR) light, 3 times the full well capacity. it can be regarded as an upgrade of the ASI462MC. Also, its dark current noise is several times lower than the ASI462MC.\u003c\/strong\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cimg class=\"wp-image-126137 aligncenter\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI678-d.jpg\" alt=\"\" width=\"303\" height=\"261\"\u003e\u003c\/p\u003e\n\u003ch6\u003eUSB3.0 and 256M DDR Memory\u003c\/h6\u003e\n\u003cp\u003eThe camera is equipped with a USB 3.0 transmission interface and a built-in 256MB DDR cache to ensure stable and secure data transmission. Under long exposure, it effectively avoids frame dropping and greatly reduces the glow effect caused by slow reading speed.\u003c\/p\u003e\n\u003cp\u003e\u003cimg class=\"aligncenter wp-image-126215\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI662MC-d.jpg\" alt=\"ZWO ASI 662MC\" width=\"544\" height=\"576\"\u003e\u003c\/p\u003e\n\u003ch6\u003eNo Amp Glow\u003c\/h6\u003e\n\u003cp\u003eZWO ASI 662MC exhibits zero amp glow, no matter how long the exposure and how high the gain value is. Since it is implemented directly at the hardware level, it does not require software control.\u003c\/p\u003e\n\u003cp\u003e\u003cimg class=\"wp-image-126214 aligncenter\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI662MC-f.jpg\" alt=\"\" width=\"445\" height=\"261\"\u003e\u003c\/p\u003e\n\u003cp style=\"text-align: center;\"\u003e\u003cstrong\u003e300 Second exposure with ASI 462MC\u003c\/strong\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cimg class=\"wp-image-126218 aligncenter\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI662MC-m.jpg\" alt=\"\" width=\"446\" height=\"264\"\u003e\u003c\/p\u003e\n\u003cp style=\"text-align: center;\"\u003e\u003cstrong\u003e300 Second exposure with ASI662MC\u003c\/strong\u003e\u003c\/p\u003e\n\u003ch6\u003eQuantum Efficiency\u003c\/h6\u003e\n\u003cp\u003eThe QE curve and noise readout are very important parameters to measure the camera's performance. Higher QE and lower readout noise are necessary to improve the image signal-to-noise ratio.\u003c\/p\u003e\n\u003cp\u003e\u003cstrong\u003eCamera Curve low read noise, high dynamic range\u003c\/strong\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cimg class=\"aligncenter wp-image-126222\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI662MC-i.jpg\" alt=\"ZWO ASI 662MC\" width=\"459\" height=\"325\"\u003e\u003c\/p\u003e\n\u003cp\u003eReadout noise includes pixel noise, circuit noise, and ADC quantization noise. The lower the readout noise, the better. As can be seen, the readout noise of the ZWO ASI 662MC is very low compared to CCD camera. The built-in HCG mode can effectively reduce the readout noise at high gain and allow the camera to maintain the same high dynamic range as it does at low gain. When the gain is 252, the HCG mode is automatically tuned on and the dynamic range rises back to 12-bit.\u003c\/p\u003e\n\u003cp\u003e\u003cimg class=\"size-full wp-image-126213 aligncenter\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI662MC-h.jpg\" alt=\"\" width=\"537\" height=\"800\"\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cimg class=\"wp-image-126221 aligncenter\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI662MC-j.jpg\" alt=\"\" width=\"550\" height=\"367\"\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cimg class=\"wp-image-126220 aligncenter\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI662MC-k.jpg\" alt=\"\" width=\"546\" height=\"513\"\u003e\u003c\/p\u003e\n\u003ch1 style=\"text-align: center;\"\u003e\n\u003cstrong\u003e What's in the box\u003c\/strong\u003e\u003cimg class=\"wp-image-126219 aligncenter\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI662MC-l.jpg\" alt=\"\" width=\"530\" height=\"323\"\u003e\n\u003c\/h1\u003e\n\u003cp\u003e \u003c\/p\u003e\n\u003cp\u003e \u003c\/p\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":42045270491205,"sku":"ZWO-ASI662MC","price":249.0,"currency_code":"AUD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/zwo-asi-662mc-colour-camera-149822.jpg?v=1731541300"},{"product_id":"zwo-asi678mc-colour-camera","title":"ZWO ASI678MC Colour Camera","description":"\u003ch4 style=\"text-align: left;\"\u003e            \u003cimg class=\"aligncenter wp-image-126150\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI678-m.jpg\" alt=\"ZWO ASI678MC\" width=\"329\" height=\"312\"\u003e\n\u003c\/h4\u003e\n\u003ch4\u003eZWO ASI6781MC\u003c\/h4\u003e\n\u003cp\u003eZWO ASI678MC adopts Sony's Latest generation sensor IMX678 with excellent near-infrared response. With the advantages of Large full well capacity, high dynamic range and low readout noise, this camera has been tested and found to have perfect performance in planetary imaging, solar and lunar imaging.\u003c\/p\u003e\n\u003ch6\u003e\u003cimg class=\"size-full wp-image-126141 aligncenter\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI678-l.jpg\" alt=\"\" width=\"700\" height=\"378\"\u003e\u003c\/h6\u003e\n\u003ch6\u003eClear in low light\u003c\/h6\u003e\n\u003cp\u003eThanks to the back-illuminated sensor structure and advanced pixel techno[ogy, the camera has very low readout noise and an ultra-high sensitivity. Especially in Low light conditions, the camera performs very well and is able to capture very clear images of celestial objects.\u003c\/p\u003e\n\u003ch6\u003eSTARVIS 2\u003c\/h6\u003e\n\u003cp\u003eZWO ASI678MC can be regarded as an upgrade of ASI178MC. It adopts the latest SONY IMX678 sensor with advanced STARVIS 2 technology. Compared to ASI178MC, \u003cstrong\u003ethis camera features zero amp glow, lower readout noise and higher sensitivity. The dark current noise is greatly decreased; the performance of near-infrared is greatly improved.\u003c\/strong\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cimg class=\" wp-image-126137 aligncenter\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI678-d.jpg\" alt=\"\" width=\"555\" height=\"479\"\u003e\u003c\/p\u003e\n\u003ch6\u003eUSB 3.0 \u0026amp; 256M DDR3 Memory\u003c\/h6\u003e\n\u003cp\u003eThe camera is equipped with a USB 3.0 transmission interface and a built-in 256MB DDR3 cache to ensure stable and secure data transmission. Under Long exposure, it effectively avoids frame dropping and greatly reduces the glow effect caused by slow reading speed.\u003c\/p\u003e\n\u003ch6\u003eUpgraded Model\u003c\/h6\u003e\n\u003cp\u003eThe ZWO ASI678MC is an upgraded product of the ASI178MC. Compared to the ASI178MC, the ASI678MC has lower read noise, lower dark noise, and no amp glow.\u003c\/p\u003e\n\u003ctable width=\"448\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd width=\"178\"\u003e\u003cstrong\u003eModel \u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd width=\"135\"\u003e\u003cstrong\u003eASI678MC \u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd width=\"135\"\u003e\u003cstrong\u003e ASI178MC\u003c\/strong\u003e\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003e\u003cstrong\u003eColor or Mono\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd\u003e Color\u003c\/td\u003e\n\u003ctd\u003eColor\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003e\u003cstrong\u003eWith or Without\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd\u003e With\u003c\/td\u003e\n\u003ctd\u003e Without\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003e\u003cstrong\u003eFormat \u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd\u003e 1\/1.8\"\u003c\/td\u003e\n\u003ctd\u003e 1\/1.8\"\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003e\u003cstrong\u003eResolution \u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd\u003e 3840*2160\u003c\/td\u003e\n\u003ctd\u003e 3096*20\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003e\u003cstrong\u003ePixel Size\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd\u003e2ųm\u003c\/td\u003e\n\u003ctd\u003e2.4ųm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003e\u003cstrong\u003eReadout Noise\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd\u003e 0.6-2.7e\u003c\/td\u003e\n\u003ctd\u003e(1e@8db\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003e\u003cstrong\u003eQE Peak\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd\u003e 83%\u003c\/td\u003e\n\u003ctd\u003e 80%\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003e\u003cstrong\u003eFull Well\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd\u003e 11.27ke\u003c\/td\u003e\n\u003ctd\u003e 15ke\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003e\u003cstrong\u003eADC \u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd\u003e 12bit\u003c\/td\u003e\n\u003ctd\u003e 14bit\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003e\u003cstrong\u003eBackfocus\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd\u003e 12.5mm\u003c\/td\u003e\n\u003ctd\u003e 12.5mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003e\u003cstrong\u003eMAX FPS\u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd\u003e 47.5 fps\u003c\/td\u003e\n\u003ctd\u003e 60 fps\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003e\u003cstrong\u003eDiagonal \u003c\/strong\u003e\u003c\/td\u003e\n\u003ctd\u003e 8.86mm\u003c\/td\u003e\n\u003ctd\u003e8.95mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003cp\u003e\u003cspan style=\"color: #000000; font-family: Arial, Helvetica, sans-serif; font-size: 1.2rem; letter-spacing: 0em;\"\u003eNo Amp Glow\u003c\/span\u003e\u003c\/p\u003e\n\u003cp\u003eZWO ASI678MC exhibits zero amp glow, no matter how long the exposure and how high the gain value is.  Since it is implemented directly at the hardware level, it does not require software control.\u003c\/p\u003e\n\u003cp\u003e\u003cimg class=\"size-full wp-image-126136 aligncenter\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI678-e.jpg\" alt=\"\" width=\"581\" height=\"450\"\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cimg class=\" wp-image-126135 aligncenter\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI678-f.jpg\" alt=\"\" width=\"567\" height=\"372\"\u003e\u003c\/p\u003e\n\u003ch6\u003eHCG Mode\u003c\/h6\u003e\n\u003cp\u003eThe camera has a built-in I-ICG mode, which can effectively reduce readout noise at high gain. This allows the camera to maintain the same high dynamic range as it does at [ow gain. When the gain is 182, the I-ICG mode is automatically turned on. The readout noise is as low as 0.8e, and the dynamic range can still reach a level close to 12bit.\u003c\/p\u003e\n\u003cp\u003e\u003cimg class=\"aligncenter wp-image-126134\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI678-g.jpg\" alt=\"ZWO ASI678MC\" width=\"554\" height=\"843\"\u003e\u003c\/p\u003e\n\u003ch6\u003eQuantum Efficiency\u003c\/h6\u003e\n\u003cp\u003eThe QE curve and readout noise are very important parameters to measure the camera's performance. Higher QE and tower readout noise are necessary to improve the image signal-to-noise ratio.\u003c\/p\u003e\n\u003cp\u003e\u003cimg class=\"aligncenter wp-image-126145\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI678-h.jpg\" alt=\"ZWO ASI678MC\" width=\"551\" height=\"399\"\u003e\u003c\/p\u003e\n\u003ch6\u003eDark Current Noise\u003c\/h6\u003e\n\u003cp\u003eASI678MC has much lower dark current noises than ASI178, bringing it has better image signal-to-noise ratios. If we compare the darks frames captured with these two cameras, it can be easily found that the frame from ASI678 has much Less noise and rooks much smoother.\u003c\/p\u003e\n\u003cp\u003e\u003cimg class=\"aligncenter wp-image-126144\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI678-i.jpg\" alt=\"ZWO ASI678MC\" width=\"585\" height=\"446\"\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cimg class=\"size-full wp-image-126143 aligncenter\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI678-j.jpg\" alt=\"\" width=\"800\" height=\"555\"\u003e \u003cimg class=\"size-full wp-image-126142 aligncenter\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI678-k.jpg\" alt=\"\" width=\"797\" height=\"673\"\u003e\u003c\/p\u003e\n\u003cp\u003e\u003cimg class=\"size-full wp-image-126153 aligncenter\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI678-b-1.jpg\" alt=\"\" width=\"800\" height=\"566\"\u003e\u003c\/p\u003e\n\u003ch6\u003e\u003cspan style=\"color: #3366ff;\"\u003e\u003ca style=\"color: #3366ff;\" href=\"https:\/\/www.bintel.com.au\/wp-content\/uploads\/2022\/06\/ASI678MC.pdf\"\u003e\u003cstrong\u003eInstruction Manual\u003c\/strong\u003e\u003c\/a\u003e\u003c\/span\u003e\u003c\/h6\u003e\n\u003cp\u003e\u003cstrong\u003eSKU:\u003c\/strong\u003e ZWO-ASI678MC\u003c\/p\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":42045270523973,"sku":"ZWO-ASI678MC","price":499.0,"currency_code":"AUD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/zwo-asi678mc-colour-camerazwo-asi678mc-416813.jpg?v=1731541425"},{"product_id":"zwo-asi715mc-colour-camera","title":"ZWO ASI715MC Colour Camera","description":"\u003cp\u003eThe AS1715MC is a sensitive color camera with a 1\/2.8\" sensor and 8.46 megapixel resolution. With the Sony STARVIS technology used, this camera has low readout noise (0.72e) and ultra-high sensitivity, making it ideal for astronomical imaging of the planets and smaller\u003cbr\u003e\ndeep-sky objects and also for microscope photography.\u003c\/p\u003e\n\u003cp\u003e\u003cimg class=\"alignnone size-medium wp-image-145513\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/715MC-1--800x429.jpg\" alt=\"\" width=\"800\" height=\"429\"\u003e\u003c\/p\u003e\n\u003cp\u003eHigh Transmission Speed The camera is equipped with a USB 3.0 transmission interface and a built-in 256MB DDR cache to ensure stable and secure\u003cbr\u003e\ndata transmission.\u003c\/p\u003e\n\u003cp\u003e\u003cimg class=\"alignnone size-medium wp-image-145514\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/715MC-800x631.jpg\" alt=\"\" width=\"800\" height=\"631\"\u003e\u003c\/p\u003e\n\u003cp\u003eUSB 3.0 Port \u0026amp; ST4 Guide USB 3.0 Port: Provides 5Gb bandwidth to allow AS1715MC to run at\u003cbr\u003e\n45.1fps (10bit, high speed mode). ST4 Port: Can be used to connect with the auto guide port of mount\u003cbr\u003e\nfor guiding\u003c\/p\u003e\n\u003cp\u003e.\u003cimg class=\"alignnone wp-image-145515\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/715MC-2-800x628.jpg\" alt=\"ASI715MC\" width=\"497\" height=\"390\"\u003e\u003c\/p\u003e\n\u003cp\u003eReadout Noise Readout noise includes pixel noise, circuit noise, and ADC quantization noise. The lower the readout noise, the better. As can be seen, the readout noise of ASI715MC is very low. As the gain value goes high, the readout noise goes down.\u003c\/p\u003e\n\u003cp\u003e\u003cimg class=\"alignnone wp-image-145516 size-medium\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/715mc-3-544x800.jpg\" alt=\"ASI715MC\" width=\"544\" height=\"800\"\u003e\u003c\/p\u003e\n\u003cp\u003eQuantum Efficiency The QE curve and readout noise are very important parameters to measure the camera's performance. Higher QE and lower readout\u003cbr\u003e\nnoise are necessary to improve the image signal-to-noise ratio. According to our estimation, the QE peak value of ASI715MC is about80%.\u003cimg class=\"alignnone wp-image-145517 size-medium\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/715mc-4-800x563.jpg\" alt=\"ASI715MC\" width=\"800\" height=\"563\"\u003e\u003c\/p\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":42045304602693,"sku":"ZWO-ASI715MC","price":339.0,"currency_code":"AUD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/zwo-asi715mc-colour-camera-586535.jpg?v=1731541425"},{"product_id":"zwo-asi676mc-colour-camera","title":"ZWO ASI676MC Colour Camera","description":"\u003cp\u003eIntroducing the ASI676MC, the all-sky camera featuring a unique square\u003cbr\u003e1\/1.6-inch image sensor and a super high resolution of 12MP! It is perfectly suited for meteor recording and full sky surveillance. The\u003cbr\u003esquare format facilitates easier composition, making mosaic stitch simpler and more efficient, and the high resolution brings you clear details of the Sun and our Moon. With this camera, you may start your marvelous journey\u003cbr\u003eto explore the boundless night sky.\u003c\/p\u003e\n\u003cp\u003e\u003cimg alt=\"\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ZWO_ASI676_specs.jpg?v=1735863537\"\u003e\u003c\/p\u003e\n\u003ch4\u003eWhy Square Format?\u003c\/h4\u003e\n\u003cp\u003eOne of the biggest benefits of AS1676MC's square format is it makes the whole mosaic construction process much easier by eliminating the need to consider the difference between the long and wide\u003cbr\u003esides of the format during mosaic stitching. Not only that, the square format also makes the AS1676MC more compatible with various types of lenses such as fisheye lenses and wide-angle lenses. Thus,\u003cbr\u003eASI676MC is more suitable for tasks such as meteor\u003cbr\u003erecording and full sky surveillance.\u003c\/p\u003e\n\u003ch4\u003eStarvis 2 Technology\u003c\/h4\u003e\n\u003cp\u003eSTARVIS is a sensor technology developed by Sony that surpasses the sensitivity of the human eye. STARVIS 2 is an advancement of STARVIS technology,\u003cbr\u003esupporting an even higher dynamic range. With this technology, ASI676MC exhibits lower readout noise and dark current, along with significantly enhanced\u003cbr\u003esensitivity in the near-infrared spectrum.\u003c\/p\u003e\n\u003ch4\u003eNo Amp Glow\u003c\/h4\u003e\n\u003cp\u003eAS1676MC does not have any amp glow, no matter\u003cbr\u003ehow long the exposure and how high the gain value\u003cbr\u003eyou set.\u003c\/p\u003e\n\u003ch4\u003e256MB DDR3\u003c\/h4\u003e\n\u003cp\u003eThe camera is equipped with a USB 3.0 transmission interface and a built-in 256MB DDR3\u003cbr\u003ecache to ensure stable and secure data transmission.\u003c\/p\u003e\n\u003ch4\u003eHigher QE Lower Readout Noise\u003c\/h4\u003e\n\u003cp\u003eThe camera has a built-in HCG mode, which can effectively reduce readout noise at high gain. This allows the camera to maintain the same high dynamic range as it does at low gain. When the gain is 180, the HCG mode is automatically turned on. The readout noise is as low as 0.56e, and the dynamic range can still reach a level close to 11stops.\u003c\/p\u003e\n\u003ch4\u003eQuantum Efficiency \u003c\/h4\u003e\n\u003cp\u003eThe QE curve and readout noise are very important parameters to measure the camera's performance. Higher QE and lower readout noise are necessary to improve the image signal-to-noise ratio. According to our estimation, the QE peak value of ASl676MC is about 83%.\u003c\/p\u003e\n\u003ch4\u003eDark Current Noise\u003c\/h4\u003e\n\u003cp\u003eThe ASI676MC's lower dark current noise means that the image signal-to-noise ratio is also higher, especially when photographing dark objects, it produces images with better sharpness.\u003c\/p\u003e\n\u003ch4\u003eIR-Cut Coated Window\u003c\/h4\u003e\n\u003cp\u003eASI676MC is equipped with an IR-cut coated window in front of the sensor, with a diameter of 21mm and a thickness of 1.1mm. It effectively reduces infrared interference and improves image quality.\u003c\/p\u003e\n\u003cp\u003e\u003cimg alt=\"\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ZWO_ASI676_box.jpg?v=1735863443\"\u003e\u003c\/p\u003e","brand":"ZWO","offers":[{"title":"Default Title","offer_id":42251225399365,"sku":"ZWO-ASI676MC","price":599.0,"currency_code":"AUD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0609\/6673\/1845\/files\/ASI676MC.jpg?v=1735863600"}],"url":"https:\/\/bintel.com.au\/collections\/zwo-camera-1-25-inch-planetary.oembed","provider":"The Binocular and Telescope Shop","version":"1.0","type":"link"}