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Bintel Glebe
Usually ready for pickup in 24 hours
Bintel 84 Wentworth park road, Glebe, 2073, NSW
Phone:(02) 9518 7255
Hours:
Monday9:30 am–5:30 pm
Tuesday9:30 am–5:30 pm
Wednesday9:30 am–5:30 pm
Thursday9:30 am–5:30 pm
Friday9:30 am–5:30 pm
Saturday9:30 am–4 pm
SundayClosed
Research Grade Cameras
Discover our range of professional imaging systems from SBIG, FLI, ATIK, QSI, QHY, and ZWO. Designed for precision, sensitivity, and unmatched image quality, these cameras meet the exacting demands of scientific research, astrophotography, and observatory installations. From capturing faint galaxies to recording high-resolution planetary details, they deliver the performance required for serious data collection and produce images that both captivate and educate.
Not sure which camera is right for your needs? Our team has extensive experience with research and educational imaging projects, and we’re here to help you choose the ideal system for your observatory, school, or program.
18 products
18 products
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$6,499.00
In two decades, much has changed beyond recognition. Sensors are now back-illuminated CMOS with native 16-bit digitisation. QE is an amazing 90% and readout is a speedy 120 million pixels per second over USB3, a performance that once was unimaginable. What is maintained by QSI’s newest cameras is the integrated design, attention to detail, and bulletproof reliability.
In the design of the 700 series we have taken our best technology. Filterwheels are mechanically indexed to ensure the most precise location for perfect flat fields. The fused silica window is dew resistant and is coated on both sides with high transmission anti-reflective coating to minimise halos. The cameras use a highly efficient 2-stage Peltier cooler that draws less current and delivers more cooling than some other cameras.
The QSI 726 is the optimum camera for most amateur telescopes. The
28mm diagonal IMX571 maximises the sharpest parts of a telescope’s
image and is less affected by coma and vignetting than larger sensors.
As with its bigger brother the 760, cable clutter is reduced thanks to
the integrated filter wheel (36mm), 2 USB2 in sockets and power out.
Power sockets have threaded connections for maximum reliability.
| Image Sensor | Sony IMX455 mono CMOS sensor | Sony IMX571 mono CMOS sensor |
| Resolution | 9576 × 6380 | 6244 × 4168 |
| Pixel Pitch | 3.76 um | 3.76 um |
| Sensor Size | 43.3mm diagonal (36mm x 24mm) | 28.3mm diagonal |
| Full Well | 51,000 e- | 51,000 e- |
| Read Noise | 1.2 e- | 1.7 e- (typical) |
| Set Point Cooling at ambient of 20 C | -25 °C | -25°C |
| Frame Rate | 2 FPS (Full Frame image) | 4FPS (Full Frame image) |
| Mount Type | M54 × 0.75 | M54 × 0.75 |
| ADC | 16 bit | 16 bit |
| Backfocus Distance | 31 mm | 31 mm |
| Reading Mode | Rolling shutter | Rolling shutter |
| Exposure Range | 1 ms - 24 hours | 1 ms - 24 hours |
| Dark Current | 0.005 e-/p/s | 0.0008 e-/p/s |
| Filter Wheel Mechanical indexing for reproducible flats | Filterwheel for 2" or unmounted filters, 5 or 7 position | 50mm/ 36mm filters |
| Accessories | Off-Axis guide unit | Off-Axis guide unit |
| Computer System | Windows 10+ Linux USB 3.0 8GB | Windows 10+ Linux USB 3.0 8GB |
| Requirements | Ram 64 bit Operating System. | Ram 64 bit Operating System |
ZWO ASI461MM-Pro adopts Sony medium format IMX461 sensor. It has the native 16-bit ADC with 65536 levels, back-illuminated structure and high quantum efficiency, and a great performance in DSO imaging. Milky way imaging and scientific research.
It features very low readout noise and nearly zero visible fixed pattern noise.
100 mega Pixels of 11656 x 8750. The 3.76 um pixel accommodates an impressive full well capacity of 50.3ke. While at Bin2 mode, you can get and even larger full well capacity of 198e and a large pixel size of 7.5um x 7.5um.
ASI461MM-Pro is a 100MP camera with a large sensor size of 44mm x 33mmand a high resolution
Note: External Power supplies are need for all ASI cooled cameras. We recommend you use a 12v@3amp DC adapter (5.5 x 21. Center Pole Positive)
No Amp Glow
Traditional CMOS sensors produce a weak infrared light source during operation, which is often seen in the corners of uncalibrated images. This is a tell-tale sign of “amp glow”. As the ASI 4612MM-Pro uses zero amp glow circuitry, you won’t have to worry about amp glow even when using high gain, long exposure imaging.
Anti -Dew
ASI461MM-Pro come with a polyimide heat that sits on top of the protective window. It will heat the window to avoid dew problems.
The power consumption of the heater is around 5W. You can turn this function off in your imaging software if you want to save power.
Camera Performance
HCG Mode
ASI461MM-Pro is integrated with HCG mode, which can get help greatly reduce readout noise and keep the dynamic range at a high level when you’re using higher gain.
Set gain 100, then the HCG mode will be automatically turned on. The readout noise can be very low, while the dynamic range is basically unchanged.
Quantum Efficiency
QE curves and readout noise are two of the most important elements to measure a camera’s performance. Based on our calculations, the QE peak values of ASI461MM-P is 91% @ 460nm
Absolute Quatum Efficiency
Relative Quantum Efficiency
Two Stage TEC Cooling
The TEC cooling system of the ASI461MM-Pro can precisely control the temperature of the sensor, and lower it to 30 – 35 degrees C below ambient temperature
Product details
Connection to External Device
Structural Dimensions
SKU: ASI461MM-Pro
$7,499.00
The Atik 16200 Monochrome camera has been designed from the ground up around the KAF-16200 sensor. With a diagonal measurement of 35mm (APS-H format) and 6 μm pixels this camera is an incredible mix of high resolution and sensor real estate.
It is a great match for a range of telescopes, and all at a much more accessible price than the likes of KAF-11002 and KAF-16803 based cameras.
The design sees the CCD housed in a sealed, argon-purged chamber, complemented by a powerful dual-stage peltier and heatsink for optimum cooling. This camera has the lowest delta you’ve ever seen from Atik, at -45°C typical, and a whopping -50°C max.
Atik 16200 Monochrome Technical Specifications
- Sensor Type: CCD - KAF-16200
- Horizontal Resolution: 4499 pixels
- Vertical Resolution: 3599 pixels
- Pixel Size: 6 µm x 6 µm
- ADC: 16 bit
- Readout Noise: 9e- typical value
- Gain Factor: 0.6e-/ ADU
- Full Well: ~40,000e-
- Dark Current: >0.25 electrons/second at 0°C
- Interface: USB 2.0 High Speed
- Power: 12v DC 2.5A
- Maximum Exposure Length: Unlimited
- Minimum Exposure Length: 200 ms
- Cooling: Thermoelectric set point with max ΔT=>-50°C (-45°C typ.)
- Weight: approx. 1.3 kg
- Backfocus: ±19.5 mm
- Available as mono or colour, with colour version to follow early 2017
Multiple Readout Modes
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. See details at “Multiple Readout Modes and Curves” Part.
Random change thermal noise suppression function
You 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.
UVLO Protection
UVLO(Under Voltage Locking) is to protect the electronic device from damage caused by abnormally low voltages.
Our 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. For 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.
Optimizing USB Traffic to Minimize Horizontal Banding
It 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.
A typical Periodic Horizontal Noise under certain USB_TRAFFIC values.
After Adjusting the USB Traffic to avoid the periodic horizontal noise.
Reboot the camera by power off and on
The 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.
Specifications
| Model | QHY461PH |
| Image Sensor | SONY IMX461 BSI CMOS Sensor |
| Pixel Size | 3.76um x 3.76um |
| Color / Mono Version | Mono Only |
| Image Resolution | 11760 × 8896 |
| Effective Pixels | 102 Megapixels |
| Effective Image Area | 44mm x 33mm |
| Sensor Surface Glass | AR+AR Multi-Coating Clear Glass |
| Full Well Capacity (1×1, 2×2, 3×3) | 50ke- / 200ke- / 450ke- in Standard Mode 80ke- / 320ke- / 720ke- in Extend Full Well Mode |
| A/D | 16-bit (0-65535 greyscale) for 1X1Binning18bit in 2X2 19BIT in 3X3 20BIT in 4*4 software Binning |
| Sensor Size | TYPICAL 3.4inch |
| Read Noise | 1e to 3.7e (in HGC mode) |
| Dark Current | Approx 0.003e/pixel/sec @ -20C |
| Exposure Time Range | 50us – 3600sec |
| Frame Rate | 2.7FPS @ 8BIT 1.3FPS@16BIT on USB3.0 2.7FPS @ 16BIT 6FPS @ 14BIT on 10Gigabit Fiber |
| Shutter Type | Electric Rolling Shutter |
| Computer Interface | USB3.0 |
| Filter Wheel Interface | 4PIN QHYCCD CFW Port |
| Built-in Image Buffer | 1GByte DDR3 Buffer |
| Cooling System | Dual Stage TEC cooler(-35C below ambient with air cooling). |
| Anti-Dew Heater | Yes |
| Telescope Interface | – |
| Optic Window Type | AR+AR High Quality Multi-Layer Anti-Reflection Coating |
| Back Focal Length | 32.5mm |
Camera Curves
$26,424.00
Our high performance Aluma® CCD Series cameras offer capabilities and features not available in any other scientific-grade imaging camera. This lightweight (2.2 lbs) and compact (4.5″ x 4.5″ x 4″ with handles) camera includes two-stage cooling, USB 2.0 interface, ultra-reliable even-illumination shutter, and fast low-noise readout.
The Aluma CCD series supports a wide range of accessories, including the 8-position AFW-8-36R filter wheel.
The Aluma CCD77-00 has an extremely high sensitivity, 260,000 pixel back-illuminated CCD sensor with 24 micron pixels. These are research-grade cameras designed for longer focal length instruments typically with apertures greater than 40 cm.
Aluma CCD is a new generation of research cameras tuned for even better performance. Over two years of collaboration with university researchers helped us bring you an enhanced new Aluma CCD series that represent the ultimate in a high-performance mid-sized 16-bit CCD detector. Using E2V’s best-in-class research grade back-illuminated sensors, the Aluma CCD77-00 gives you the high sensitivity, low noise, and high well depth needed for the most demanding research applications.
Aluma CCD Features include:
- High-performance CCD imaging sensors currently manufactured by SONY and Teledyne E2V
- Light weight, compact design
- Centered optical axis for optimum instrument balance
- Ultra reliable even-illumination (photometric) mechanical shutter
- USB 2.0 interface
- Full frame image buffering eliminates readout artifacts
- 2-Stage TE cooling with typical -50C from ambient
- Twin variable speed fans with SmartCoolingTM technology
- High accuracy temperature regulation
- Built-in RBI Pre-flash (full frame front-illuminated sensors only)
- External TTL trigger inputs and output
- Included 110V / 220V power supply and optional 12VDC operation
- User-rechargeable desiccant plug
- Built-in 1/4-20 tripod mount
- Support for high precision 8-position filter wheels
- Bulletproof firmware update capability – virtually impossible to “brick”
Software Included
All Aluma CCD models ship with MaxIm LT for Windows – a special version of MaxIm DL specific to our cameras. Aluma CCD also supports third-party applications through ASCOM and native drivers.
Compact and Lightweight Design
Aluma CCD cameras measure just 4.25″ x 4.25″ x 4.0″ with handles (3.5″ without handles) and weigh just 2.2 lbs (1 kg).
Even-Illumination Shutter
All Aluma CCD cameras include a mechanical shutter, which is used for both dark/bias calibration frames and for shuttering exposures on full frame sensors. Rather than using a complex iris shutter, which are prone to failure, the Aluma CCD uses a twin vane shutter and direct drive motor for high repeatability, reliability, and extremely long life. The shutter is designed to be “even illumination” for the best accuracy in photometric measurements.
Extreme Sensitivity CCD 77-00 Image Sensor
The Aluma CCD77-00 uses the 0.26 megapixel E2V CCD 77-00 sensor, featuring peak quantum efficiency (QE) of 93% with midband coatings. This full frame, back-illuminated sensor is designed for the ultimate in sensitivity. We offer Midband coating for the highest quantum efficiency. Other coatings are available on special order.
CCD 77-00 Quantum Efficiency Curves The CCD 77-00 has 512 x 512 pixels at 24 microns square, for a 12.3 mm square chip size. This back-illuminated full-frame CCD sensor has extremely low noise and extremely high sensitivity. Combining this high-performance sensor with Aluma CCD’s high cooling performance and low readout noise results in exceptionally clean images. SmartCoolingTM
All Aluma CCD cameras include our powerful new SmartCooling technology. The two-stage cooler, powerful fans, and advanced heat sink designed using thermal flow simulation combine to produce typical cooling delta from ambient of -50C. This is quite a feat considering the Aluma CCD’s very compact and lightweight package. SmartCooling automatically adjusts the fan speed to optimize cooler performance and power consumption. The camera’s firmware is constantly monitoring the sensor and heat sink temperatures, as well as controlling the cooler power. When full cooling power is needed – when ramping down or running near full power – the fans ramp up to their maximum speed, resulting in the strongest possible cooling. When less cooling power is needed the fans automatically slow to reduce noise levels and power consumption. SmartCooling also prevents any possibility of overheating by backing off power if the heat sink gets too hot – so you don’t need to worry if your camera is baking in a hot observatory during the day. Advanced Software Included
All Aluma CCD cameras come with our MaxIm LT software – a $249 value! MaxIm LT is a special version of our venerable MaxIm DL software that provides complete control of your camera, filter wheel, and autoguider, plus advanced image processing capabilities. If you wish you can upgrade to MaxIm DL Pro to get complete observatory integration and even more processing and analysis capabilities. Included Accessories Each Aluma CCD camera package includes: Optional Filter Wheel
The optional AFW-8-36R 8-position filter wheel provides a fast, quiet, and low-cost option. It holds standard 36 mm filters, and inserts are available for 1-1/4″ filters, which are suitable for smaller format CCD sensors. The optional AFW-16-36R filter wheel, attached via AFW to Small Format Camera Adapter, provides for a full sixteen 36 mm filters. Please note that the AFW wheels work with large format accessories, and do not accommodate screw-in 1-1/4″ filters due to their height.
Antiblooming
n
Binning Modes
Horizontal 1, 2, 3, 4; Vertical 1-255
Computer Interface
USB 2.0
Cooling Delta
50 °C
Exposure
0.12-3600 sec
Filter Size
36mm / 1.25"
Filter Wheel Option
y
Full Well Capacity
300,000 e-
Imaging / Pixel Array
512 x 512
OAG Option
StarChaser
Peak QE
93%
Pixel Digitization Rate
1 MPix/sec
Pixel Size
24 μm
Power
12 VDC, 5A max
Shutter
Mechanical, Even-illumination
Temperature Regulation
y
Total Pixels
262,000 pixels
Weight
0.997kg (2.2 lbs)
$8,899.00
Our new high-performance SBIG Aluma CCD 814 camera offers capabilities and features not available in any other scientific-grade imaging camera. This lightweight (1kg) and compact (114mm x 114mm x 102mm with handles) camera includes two-stage cooling, USB 2.0 interface, ultra-reliable even-illumination shutter, and fast low-noise readout.
The SBIG Aluma CCD 814 supports a wide range of accessories, including the 8-position FW8S-Aluma filter wheel with micron-level filter positioning, StarChaser SC-2 off-axis guide camera, and AO-8A Adaptive Optics accessory.
The SBIG Aluma CCD 814 has a high-sensitivity, low-noise 9 megapixel CCD sensor with 3.69-micron pixels. It is ideal for taking high spatial resolution, long-duration exposures with minimal amp glow, dark current, and noise. It also includes the ability to perform high ratio analog binning, which is important for applications such as spectroscopy.
SBIG Aluma CCD 814 is a new generation of research cameras tuned for even better performance. Over two years of collaboration with university researchers helped us bring you an enhanced new Aluma CCD series that represent the best value in a high-performance mid-sized 16-bit CCD detector. We have carefully refined the camera electronics for improved performance, minimum amp glow, and low noise. Using SONY’s best-in-class CCDs, you’ll get the precision and ultra-clean images of a CCD with the sensitivity of CMOS technology.
Aluma CCD814 – Incredible Sensitivity
The ICX-814 CCD is one of the best optical sensors ever produced, with a peak quantum efficiency of over 75%, very broad spectral sensitivity, and extraordinary blue sensitivity. It also has very low read noise, a large dynamic range, and an extremely low dark current. This combination of high sensitivity and very low noise means you get cleaner, deeper images – faster.
- High-performance CCD imaging sensors currently manufactured by SONY and Teledyne E2V
- Lightweight, compact design
- Centered optical axis for optimum instrument balance
- Ultra-reliable even-illumination (photometric) mechanical shutter
- USB 2.0 interface
- Full frame image buffering eliminates readout artifacts
- 2-Stage TE cooling with typical -50C from ambient
- Twin variable speed fans with SmartCoolingTM technology
- High accuracy temperature regulation
- Built-in RBI Pre-flash (full frame front-illuminated sensors only)
- External TTL trigger inputs and output
- Included 110V / 220V power supply and optional 12VDC operation
- User-rechargeable desiccant plug
- Built-in 1/4-20 tripod mount
- Support for high precision 8-position filter wheels
- Works with StarChaser SC-2 off-axis guide camera and AO-8A adaptive optics
- Bulletproof firmware update capability – virtually impossible to “brick”
Advanced Software Included
All Aluma CCD models ship with MaxIm LT for Windows – a special version of MaxIm DL specific to our cameras. Aluma CCD also supports third-party applications through ASCOM and native drivers.
Compact and Lightweight Design
Aluma CCD cameras measure just 114mm x 114mm x 102mm with handles (89mm without handles) and weigh just 1 kg(2.2 lbs).
Mechanical Shutter
The SBIG Aluma CCD 814 has electronic shuttering, allowing a minimum exposure of just 0.001s. In addition, it has a high-reliability mechanical shutter, which facilitates accurate dark/bias calibration frames.
High-Performance ICX-814 Image Sensor
The SBIG Aluma CCD 814 uses the popular 9-megapixel SONY ICX-814ALG sensor. This sensor has 3388 x 2712 pixels at 3.69 microns square, for a 12.48 mm x 9.98 mm chip size.
This is a high-sensitivity interline CCD sensor with an extremely low dark current and very low read noise. Combining this high-performance sensor with Aluma CCD’s high cooling performance and low readout noise results in exceptionally clean images.
This sensor includes microlens technology that concentrates light on the sensitive area of each pixel. The CCD’s sensitivity peaks in the center of the visible spectrum at 550 nm, and maintains high sensitivity throughout the visible spectrum. The ICX-814 is particularly good in blue compared to other sensors on the market.
SmartCoolingTM
All Aluma CCD cameras include our powerful new SmartCooling technology. The two-stage cooler, powerful fans, and advanced heat sink designed using thermal flow simulation combine to produce a typical cooling delta from an ambient of -50C. This is quite a feat considering the Aluma CCD’s very compact and lightweight package.
SmartCooling automatically adjusts the fan speed to optimize cooler performance and power consumption. The camera’s firmware is constantly monitoring the sensor and heat sink temperatures and controlling the cooler power. When full cooling power is needed – when ramping down or running near full power – the fans ramp up to their maximum speed, resulting in the strongest possible cooling. When less cooling power is needed the fans automatically slow to reduce noise levels and power consumption. SmartCooling also prevents any possibility of overheating by backing off power if the heat sink gets too hot – so you don’t need to worry if your camera is baking in a hot observatory during the day.
Advanced Software Included
All SBIG cameras come with our MaxIm LT software – a $200 value! MaxIm LT is a special version of our venerable MaxIm DL software that provides complete control of your camera, filter wheel, and autoguider, plus advanced image processing capabilities. If you wish you can upgrade to MaxIm DL Pro to get complete observatory integration and even more processing and analysis capabilities.
Included Accessories
Each Aluma CCD camera package includes:
- MaxIm LT software – please use this form to request your license
- Deluxe carrying case
- Universal power supply (110V / 220V, 50-60 Hz)
- 2″ Nosepiece adapter
- USB flash drive containing software, drivers, and documentation
- 15 foot (4.5 m) USB cable
Optional Micron-Precision Filter Wheel
The optional FW8S-Aluma 8-position filter wheel includes a positive centering mechanism that precisely centers each filter in the exact same position every time. This single-pixel accuracy completely eliminates ghost images of dust spots and other artifacts after flat-fielding.
Positive detent mechanism provides single-pixel filter position accuracy
Precision flat-fielding with utlra-accurate indexing
The above left image shows a dust spot on the filters. A flat-field calibration frame was taken, then the filter wheel was rotated several times before taking a second picture, which was flat-field calibrated, above right. No evidence of the dust spot is visible. This high precision results in the highest quality images and excellent photometric accuracy.
The Aluma wheel holds standard 36 mm filters, and inserts are available for 1-1/4″ filters, which are suitable for smaller format CCD sensors.
The Aluma filter wheel replaces the camera’s front plate, resulting in the minimum possible back-focus, ensuring that the camera / filter wheel combination will reach focus on the widest possible variety of optical systems.
Optional StarChaser SC-2 Off-Axis Guide Camera
For astronomical imaging the Aluma CCD series works the StarChaser SC-2 Off-Axis Guide Camera. This provides reliable guiding with no impact from optical train flexure. It also supports the operation of the optional AO-8A Adaptive Optics accessory.
Optional AO-8A Adaptive Optics
All Aluma CCD models can operate with the AO-8A Adaptive Optics accessory. The AO-8A uses a tip-tilt window to quickly and precisely adjust the image position in response to autoguider feedback. With Adaptive Optics there is no backlash, stiction, or lag, and the movements are extremely precise and accurate. This allows the AO-8A to not only remove the effects of periodic error, drift, and wind gusts, but also reduce the effects of atmospheric seeing
$8,099.00
The Aluma CCD 694 supports a wide range of accessories, including the 8-position FW8S-Aluma filter wheel with micron-level filter positioning, StarChaser SC-2 off-axis guide camera, and AO-8A Adaptive Optics accessory.
The Aluma CCD 694 has a high-sensitivity, low-noise 6 megapixel CCD sensor with 4.54 micron pixels. It is ideal for taking high spatial resolution, long duration exposures with minimal amp glow, dark current, and noise. It also includes the ability to perform high ratio analog binning, which is important for applications such as spectroscopy.
Aluma CCD is a new generation of research cameras tuned for even better performance. Over two years of collaboration with university researchers helped us bring you an enhanced new Aluma CCD series that represent the best value in a high-performance mid-sized 16-bit CCD detector. We have carefully refined the camera electronics for improved performance, minimum amp glow, and low noise. Using SONY’s best-in-class CCDs, you’ll get the precision and ultra-clean images of a CCD with the sensitivity of CMOS technology.
Aluma CCD 694 – Incredible Sensitivity
The ICX-694 CCD is one of the best optical sensors ever produced, with peak quantum efficiency over 75%, very broad spectral sensitivity, and extraordinary blue sensitivity. It also has very low read noise, large dynamic range, and extremely low dark current. This combination of high sensitivity and very low noise means you get cleaner, deeper images – faster.
- High-performance CCD imaging sensors currently manufactured by SONY and Teledyne E2V
- Lightweight, compact design
- Centered optical axis for optimum instrument balance
- Ultra-reliable even-illumination (photometric) mechanical shutter
- USB 2.0 interface
- Full frame image buffering eliminates readout artifacts
- 2-Stage TE cooling with typical -50C from ambient
- Twin variable speed fans with SmartCoolingTM technology
- High accuracy temperature regulation
- Built-in RBI Pre-flash (full frame front-illuminated sensors only)
- External TTL trigger inputs and output
- Included 110V / 220V power supply and optional 12VDC operation
- User-rechargeable desiccant plug
- Built-in 1/4-20 tripod mount
- Support for high precision 8-position filter wheels
- Works with StarChaser SC-2 off-axis guide camera and AO-8A adaptive optics
- Bulletproof firmware update capability – virtually impossible to “brick”
Advanced Software Included
All Aluma CCD models ship with MaxIm LT for Windows – a special version of MaxIm DL specific to our cameras. Aluma CCD also supports third-party applications through ASCOM and native drivers.
Compact and Lightweight Design
Aluma CCD cameras measure just 114mm x 114mm x 102mm with handles (89mm without handles) and weigh just 1 kg(2.2 lbs).
Mechanical Shutter
The SBIG Aluma CCD 814 has electronic shuttering, allowing a minimum exposure of just 0.001s. In addition, it has a high-reliability mechanical shutter, which facilitates accurate dark/bias calibration frames.
High-Performance ICX-694 Image Sensor
The Aluma CCD 694 uses the popular 6-megapixel SONY ICX-694ALG sensor. This sensor has 2750 x 2200 pixels at 4.54 microns square, for a 14.6 mm x 12.8 mm chip size.
This is a high-sensitivity interline CCD sensor with an extremely low dark current and very low read noise. Combining this high-performance sensor with Aluma CCD’s high cooling performance and low readout noise results in exceptionally clean images.
This sensor includes microlens technology that concentrates light on the sensitive area of each pixel. The CCD’s sensitivity peaks in the center of the visible spectrum at 550 nm, and maintains high sensitivity throughout the visible spectrum. The ICX-694 is particularly good in the blue compared to other sensors on the market.
SmartCoolingTM
All Aluma CCD cameras include our powerful new SmartCooling technology. The two-stage cooler, powerful fans, and advanced heat sink designed using thermal flow simulation combine to produce a typical cooling delta from an ambient of -50C. This is quite a feat considering the Aluma CCD’s very compact and lightweight package.
SmartCooling automatically adjusts the fan speed to optimize cooler performance and power consumption. The camera’s firmware is constantly monitoring the sensor and heat sink temperatures and controlling the cooler power. When full cooling power is needed – when ramping down or running near full power – the fans ramp up to their maximum speed, resulting in the strongest possible cooling. When less cooling power is needed the fans automatically slow to reduce noise levels and power consumption. SmartCooling also prevents any possibility of overheating by backing off power if the heat sink gets too hot – so you don’t need to worry if your camera is baking in a hot observatory during the day.
Advanced Software Included
All SBIG cameras come with our MaxIm LT software – a US$200 value! MaxIm LT is a special version of our venerable MaxIm DL software that provides complete control of your camera, filter wheel, and autoguider, plus advanced image processing capabilities. If you wish you can upgrade to MaxIm DL Pro to get complete observatory integration and even more processing and analysis capabilities.
Included Accessories
Each Aluma CCD camera package includes:
- MaxIm LT software – please use this form to request your license
- Deluxe carrying case
- Universal power supply (110V / 220V, 50-60 Hz)
- 2″ Nosepiece adapter
- USB flash drive containing software, drivers, and documentation
- 15 foot (4.5 m) USB cable
Optional Micron-Precision Filter Wheel
The optional FW8S-Aluma 8-position filter wheel includes a positive centering mechanism that precisely centers each filter in the exact same position every time. This single-pixel accuracy completely eliminates ghost images of dust spots and other artifacts after flat fielding.
Positive detent mechanism provides single-pixel filter position accuracy
Precision flat-fielding with utlra-accurate indexing
The above left image shows a dust spot on the filters. A flat-field calibration frame was taken, then the filter wheel was rotated several times before taking a second picture, which was flat-field calibrated, above right. No evidence of the dust spot is visible. This high precision results in the highest quality images and excellent photometric accuracy.
The Aluma wheel holds standard 36 mm filters, and inserts are available for 1-1/4″ filters, which are suitable for smaller format CCD sensors.
The Aluma filter wheel replaces the camera’s front plate, resulting in the minimum possible back-focus, ensuring that the camera / filter wheel combination will reach focus on the widest possible variety of optical systems.
Optional StarChaser SC-2 Off-Axis Guide Camera
For astronomical imaging the Aluma CCD series works the StarChaser SC-2 Off-Axis Guide Camera. This provides reliable guiding with no impact from optical train flexure. It also supports the operation of the optional AO-8A Adaptive Optics accessory.
Optional AO-8A Adaptive Optics
All Aluma CCD models can operate with the AO-8A Adaptive Optics accessory. The AO-8A uses a tip-tilt window to quickly and precisely adjust the image position in response to autoguider feedback. With Adaptive Optics there is no backlash, stiction, or lag, and the movements are extremely precise and accurate. This allows the AO-8A to not only remove the effects of periodic error, drift, and wind gusts, but also reduce the effects of atmospheric seeing
From $15,889.00
SBIG Aluma AC2020BSI
Extreme sensitivity back-illuminated Scientific CMOS camera. 4-megapixel sensor with 6.5-micron pixels, Adaptive Optics capable, StarChaser Guider compatible.
SBIG Aluma AC2020BSI features a Class 1 sensor.
A fused silica chamber window is available with VIS-NIR and UV-VIS optical coating options.
Coming soon – available for preorder.
The SBIG Aluma AC Series represents the state-of-the-art in Advanced Scientific CMOS cameras for astronomical imaging systems. The camera’s advanced design permits high-speed download via the USB 3.0 connection to the control computer. The SBIG Aluma AC2020BSI uses the Gpixel GSENSE2020BSI-H CMOS sensor with 4 million pixels at 6.5 microns in a 2048 x 2048 array. The sensor measures just over 13.3mm square. The Aluma AC series has powerful two-stage cooling and supports optional water cooling. Aluma AC cameras can be operated directly from a 12VDC 8A power supply.
Design features include:
Back-Illuminated Sensor
Incredible sensitivity! High-performance back-illuminated sensors are flipped over and thinned during manufacture, so incoming light does not encounter any circuitry before hitting the sensitive pixel area. This provides optimum sensitivity across the entire visible spectrum – and beyond.
The sensor in the GSENSE2020BSI-H has a peak quantum efficiency of 91%, with a broad peak in the visible spectrum. For near UV and IR applications, it features good sensitivity all the way from 200 nm to 1000 nm.
Chamber Window Coating Options
The GSENSE2020BSI-H sensor is windowless, which provides the optimum sensitivity across the sensor. For windowless sensors we recommend recharging the desiccant plug annually, to avoid any risk of moisture contamination on the sensor.
The fused silica optical window on the sealed sensor chamber is available with two standard coating options, depending on your application. VIS-NIR provides optimal sensitivity from 400 nm through 1000 nm. UV-VIS provides optimal transmission from 250 nm through 700 nm.
StackPro™
The SBIG Aluma AC2020BSI scientific CMOS camera features StackPro™, a revolutionary feature that performs image stacking inside the camera.
CMOS sensors often have more limited well depth and bit depth than their CCD predecessors. At the same time, the modern CMOS sensors have much lower read noise than the equivalent CCD. This low read noise can be used to advantage, by stacking many shorter exposures to achieve the same final result. This does however result in a lot of extra disk usage and post-processing.
StackPro™ performs the stacking automatically, inside the camera. It automatically subdivides your exposure into up to 16 individual subexposures, and stacks them inside the camera prior to download. This eliminates the excessive amounts of data cluttering up your hard drive. Stacking can also be used as an alternative to High Dynamic Range (HDR) mode.
HDR Mode
The sensor in the AC2020BSI is capable of operating in HDR mode, where high-gain and low-gain images are read out simultaneously. Our included MaxIm LT software features an HDR merge feature, which greatly simplifies the process of producing clean, highly linear images.
Superior Cooling
Proven pin heatsink design shared with industry-leading STX series cameras gets the heat out while providing low vibration. Includes SmartCooling™ intelligent thermoelectric cooling and fan operation.
Water Circulation Ready
For high ambient temperature environments, the liquid cooling option improves thermal performance and helps minimize dark current.
User Rechargeable Desiccant
SBIG pioneered including a high-tech user-replaceable cartridge with a ceramic filter and molecular sieve desiccant. Unlike competing cameras, which require factory service when their chamber desiccant eventually saturates out, the user can easily recharge the desiccant. This eliminates the need for costly service – not to mention the associated downtime and shipping costs. This feature is especially important in high-humidity locations.
Electronic and Mechanical Shutters
The GSENSE CMOS sensor has an electronic rolling shutter. In addition, the Aluma AC series cameras include a mechanical shutter to enable convenient dark-frame subtraction for optimal performance and sensitivity. This is essential for remote/robotic operation.
Optional 12 Position Filter Wheel
The SBIG Aluma AC2020BSI is compatible with the new 12 position SBIG AFW-12-50R filter wheel, utilizing 50 mm round filters.
It is also compatible with the 7 position FW7-STX filter wheel, utilizing 50 mm square filters.
Self-Guiding and Adaptive Optics Options Available
The available SBIG StarChaser SC-3 is an excellent low-cost option for integrated autoguiding in front of the filters, and it supports our SBIG AO-X Adaptive Optics accessory.
The AO-X uses a tip-tilt window to quickly and precisely adjust the image position in response to autoguider feedback. With Adaptive Optics there is no backlash, stiction, or lag, and the movements are precise and accurate. This allows the AO-X to not only remove the effects of periodic error, drift, and wind gusts but also reduce the effects of atmospheric seeing. When used with an Aluma AC camera, the AO-X requires the StarChaser SC-3.
For more information please see AO-X.
USB 3.0 Interface
The Aluma AC includes a USB 3.0 interface port for high-speed downloads. For installations where longer cable lengths are required, the port is also compatible with USB 2.0.
I2C AUX Port
The STX cameras have a convenient auxiliary control port (also known as an I2C AUX port), which controls the filter wheel and provides optional external trigger interfaces. Unlike older SBIG models, the AUX port is not used for AO-X control, as this function is now handled by the optional SBIG StarChaser SC-3 off-axis guiding camera.
MaxIm LT Software
All SBIG cameras come with our MaxIm LT software – a $200 value! MaxIm LT is a special version of our venerable MaxIm DL software that provides complete control of your camera, filter wheel, and auto guider, plus advanced image processing capabilities. If you wish you can upgrade to MaxIm DL Pro to get complete observatory integration and even more processing and analysis capabilities.
Included Accessories
All Aluma AC cameras include a deluxe carrying case, universal power supply, Aluma AC power extension cable, USB 3.0 cable, and MaxIm LT software.
Specifications
| Exposure |
0.001-3600 sec |
|---|---|
| OS Compatibility | Windows 7, 8, 10 x86/x64, MacOS 10.14 "Mojave" x86 binaries, Ubuntu 18.04 LTS x64, Raspbian Buster armhf, Ubuntu MATE arm64 |
| Full Frame Download | 0.1 sec |
| Weight | 3.5 lbs / 1.6 kG |
| Filter Size | 50mm Square |
| Read Noise (typ) | 1.2 e- in 2-CMS Readout Mode, 1.6 e- Regular Mode |
| Temperature Regulation | Yes |
| Computer Interface | USB 3.0 |
| Power | 12 VDC 8A |
| Cooling Delta | ~ 40 °C typical, water cooling option included |
| Adaptive Optics Option | AO-X with StarChaser SC-3 |
| A/D Converter | Dual 12 bit with HDR capability |
| Dark Current e-/p/s | 0.16 e-/p/sec @ -20C |
| Full Well Capacity | 55,000 e- |
| Sensor Size | 13.3 mm x 13.3 mm |
| Imaging / Pixel Array | 2048 x 2048 |
| Shutter | Rolling electronic, Mechanical dark shutter |
| Self-Guiding In Front of Filters | Yes with StarChaser |
| Pixel Size | 6.5 um |
| Total Pixels | 4 million |
| Filter Wheel Option | FW7-STX |
| OAG Option | StarChaser |
| Imaging Sensor | Gpixel GSENSE2020BSI |
| Chamber Window | VIS-NIR, UV-VIS |
From $9,565.00
In two decades, much has changed beyond recognition. Sensors are now back-illuminated CMOS with native 16-bit digitisation. QE is an amazing 90% and readout is a speedy 120 million pixels per second over USB3, a performance that once was unimaginable. What is maintained by QSI’s newest cameras is the integrated design, attention to detail, and bulletproof reliability.
In the design of the 700 series we have taken our best technology. Filterwheels are mechanically indexed to ensure the most precise location for perfect flat fields. The fused silica window is dew resistant and is coated on both sides with high transmission anti-reflective coating to minimise halos. The cameras use a highly efficient 2-stage Peltier cooler that draws less current and delivers more cooling than some other cameras.
The QSI 760 is our flagship product. The full frame IMX455 is widely regarded as the premium sensor for astronomers. The integrated 2”/50mm filter wheel minimises back focus, essential for the widest compatibility with focal reducers. Cable clutter is reduced thanks to the integrated filter wheel, 2 USB2 in sockets and power out. Power sockets have threaded connections for maximum reliability.
| Image Sensor | Sony IMX455 mono CMOS sensor | Sony IMX571 mono CMOS sensor |
| Resolution | 9576 × 6380 | 6244 × 4168 |
| Pixel Pitch | 3.76 um | 3.76 um |
| Sensor Size | 43.3mm diagonal (36mm x 24mm) | 28.3mm diagonal |
| Full Well | 51,000 e- | 51,000 e- |
| Read Noise | 1.2 e- | 1.7 e- (typical) |
| Set Point Cooling at ambient of 20 C | -25 °C | -25°C |
| Frame Rate | 2 FPS (Full Frame image) | 4FPS (Full Frame image) |
| Mount Type | M54 × 0.75 | M54 × 0.75 |
| ADC | 16 bit | 16 bit |
| Backfocus Distance | 31 mm | 31 mm |
| Reading Mode | Rolling shutter | Rolling shutter |
| Exposure Range | 1 ms - 24 hours | 1 ms - 24 hours |
| Dark Current | 0.005 e-/p/s | 0.0008 e-/p/s |
| Filter Wheel Mechanical indexing for reproducible flats | Filterwheel for 2" or unmounted filters, 5 or 7 position | 50mm/ 36mm filters |
| Accessories | Off-Axis guide unit | Off-Axis guide unit |
| Computer System | Windows 10+ Linux USB 3.0 8GB | Windows 10+ Linux USB 3.0 8GB |
| Requirements | Ram 64 bit Operating System. | Ram 64 bit Operating System |
From $56,360.00
The Kepler KL6060 FI camera delivers an expansive field of view (FOV), exceptional low-noise performance, high frame rates, and outstanding dark current specifications. As our most cost-effective large-format camera, it is perfectly suited for space domain awareness and other high-precision imaging applications that demand both reliability and performance.
| Sensor | GSENSE6060 FI |
| Diagonal Size (mm) | 83.9mm |
| Resolution | 6144 x 6144 |
| Pixel Size | 10um |
| Bit depth | 16-bit |
| Full Well | 95ke- |
| Read Noise | 4.2 e- |
| Dark current | 0.07 EPS @ -20c |
| Shutter | Rolling |
| Peak QE | 73%% |
| Interface | USB 3 QSFP |
| Frame Rate | 19 FPS (QSFP) |
Optional Accessories
Quantum Efficiency
Quantum efficiency (QE) measures how effectively a detector converts incoming photons into electrons. In our graphs, QE is expressed as a percentage. A sensor’s QE typically varies based on its architecture, coatings, and materials. High QE remains a crucial consideration for applications such as astronomy, space debris imaging, and life science research.
From $143,850.00
The Kepler KL6060 BI camera features a back-illuminated sensor, offering unparalleled sensitivity for even the most challenging low-light environments. With its large field of view (FOV), low-noise performance, and high frame rates, the KL6060 BI is ideal for Space Domain Awareness and other critical low-light imaging applications, where both reliability and performance are paramount.
| Sensor | GSENSE6060 BI |
| Diagonal Size (mm) | 83.9mm |
| Resolution | 6144 x 6144 |
| Pixel Size | 10um |
| Bit depth | 16-bit |
| Full Well | 95ke- |
| Read Noise | 3.0 e- |
| Dark current | 0.1 EPS @ -20c |
| Shutter | Rolling |
| Peak QE | 95% |
| Interface | USB 3 QSFP |
| Frame Rate | 11 FPS (QSFP) |
Optional Accessories
Quantum Efficiency
Quantum efficiency (QE) measures how effectively a detector converts incoming photons into electrons. In our graphs, QE is expressed as a percentage. A sensor’s QE typically varies based on its architecture, coatings, and materials. High QE remains a crucial consideration for applications such as astronomy, space debris imaging, and life science research.
From $25,090.00
The KL4040 shares the same large area as the KAF-16803 CCD, but with a giant improvement in throughput, substantially lower noise, and higher quantum efficiency. The KL4040 has become an industry favorite for time-resolved applications such as space domain awareness.
| Sensor | GSENSE4040 FI |
| Diagonal Size (mm) | 52.1mm |
| Resolution | 4096 x 4096 |
| Pixel Size | 9um |
| Bit depth | 16-bit |
| Full Well | 70ke- |
| Read Noise | 3.7e |
| Dark current | 0.15 EPS @ -20c |
| Shutter | Rolling |
| Peak QE | 73% |
| Interface | USB 3 QSFP |
| Frame Rate | 23 FPS (QSFP) |
Optional Accessories
Quantum Efficiency
Quantum efficiency (QE) measures how effectively a detector converts incoming photons into electrons. In our graphs, QE is expressed as a percentage. A sensor’s QE typically varies based on its architecture, coatings, and materials. High QE remains a crucial consideration for applications such as astronomy, space debris imaging, and life science research.
From $41,660.00
For years we dreamed of a back-illuminated version of the KAF-16803 CCD – and here it is, except with high throughput and lower noise. The KL4040 BI has the high sensitivity of a CCD42-40, but with twice the area and 20% lower cost.
| Sensor | GSENSE4040 BI |
| Diagonal Size (mm) | 52.1mm |
| Resolution | 4096 x 4096 |
| Pixel Size | 9um |
| Bit depth | 16-bit |
| Full Well | 70ke- |
| Read Noise | 2.3e |
| Dark current | 0.15 EPS @ -20c |
| Shutter | Rolling |
| Peak QE | 94% |
| Interface | USB 3 QSFP |
| Frame Rate | 23 FPS (QSFP) |
Optional Accessories
Quantum Efficiency
Quantum efficiency (QE) measures how effectively a detector converts incoming photons into electrons. In our graphs, QE is expressed as a percentage. A sensor’s QE typically varies based on its architecture, coatings, and materials. High QE remains a crucial consideration for applications such as astronomy, space debris imaging, and life science research.
From $16,470.00
The Kepler KL400FI provides high sensitivity, ultra-low noise with high frame rates, all at a game-changing price to performance ratio. An ideal camera for those applications requiring a sensor without microlenses.
| Sensor | GSENSE400 FI |
| Diagonal Size (mm) | 31.9mm |
| Resolution | 2048x2048 |
| Pixel Size | 11um |
| Bit depth | 16-bit |
| Full Well | 120ke- |
| Read Noise | 1.5e- |
| Dark current | 0.15 EPS @ -20c |
| Shutter | Rolling |
| Peak QE | 68% |
| Interface | USB 3 QSFP |
| Frame Rate | 24 FPS HDR / 48 FPS LDR |
Optional Accessories
Quantum Efficiency
Quantum efficiency (QE) measures how effectively a detector converts incoming photons into electrons. In our graphs, QE is expressed as a percentage. A sensor’s QE typically varies based on its architecture, coatings, and materials. High QE remains a crucial consideration for applications such as astronomy, space debris imaging, and life science research.
From $20,530.00
Extreme sensitivity, including excellent QE at 240 nm, coupled with ultra-low noise make this camera ideal for challenging applications requiring high dynamic range despite short exposures at high frame rate.
| Sensor | GSENSE400 BI |
| Diagonal Size (mm) | 31.9mm |
| Resolution | 2048x2048 |
| Pixel Size | 11um |
| Bit depth | 16-bit |
| Full Well | 120ke- |
| Read Noise | 1.6e- |
| Dark current | 0.4 EPS @ -20c |
| Shutter | Rolling |
| Peak QE | 95% |
| Interface | USB 3 QSFP |
| Frame Rate | 24 FPS HDR / 48 FPS LDR |
Optional Accessories
Quantum Efficiency
Quantum efficiency (QE) measures how effectively a detector converts incoming photons into electrons. In our graphs, QE is expressed as a percentage. A sensor’s QE typically varies based on its architecture, coatings, and materials. High QE remains a crucial consideration for applications such as astronomy, space debris imaging, and life science research.
$9,749.00
Designed and manufactured in the USA with same extreme reliability as the thousands of FLI OEM cameras. Install in remote observatories around the world with complete confidence in a long, trouble-free life. High sensitivity with exceptionally low noise and dark current. Great combination of resolution and frame rate.
| Sensor | IMX571 |
| Diagonal Size (mm) | 28.2 |
| Resolution | 6244 x 4168 |
| Pixel Size | 3.76um |
| Bit depth | 15-bit |
| Full Well | 50ke- |
| Read Noise | 1e- |
| Dark current | 0.002 EPS @ -20c |
| Shutter | Rolling |
| Peak QE | 91%% |
| Interface | USB 3 QSFP |
| Frame Rate | 7FPS |
Optional Accessories
Quantum Efficiency
Quantum efficiency (QE) measures how effectively a detector converts incoming photons into electrons. In our graphs, QE is expressed as a percentage. A sensor’s QE typically varies based on its architecture, coatings, and materials. High QE remains a crucial consideration for applications such as astronomy, space debris imaging, and life science research.
$8,439.00
Designed and manufactured in the USA with same extreme reliability as the thousands of FLI OEM cameras. Install in remote observatories around the world with complete confidence in a long, trouble-free life. High sensitivity CMOS camera with 90% quantum efficiency and 15.9 mm diagonal field of view is an ideal replacement for 1" format CCDs.
| Sensor | IMX533 |
| Diagonal Size (mm) | 16mm |
| Resolution | 3003 x 3003 |
| Pixel Size | 3.76um |
| Bit depth | 14-bit |
| Full Well | 50ke- |
| Read Noise | 1e- |
| Dark current | 0.002 EPS @ -20c |
| Shutter | Rolling |
| Peak QE | 91%% |
| Interface | USB 3 QSFP |
| Frame Rate | 20FPS |
Optional Accessories
Quantum Efficiency
Quantum efficiency (QE) measures how effectively a detector converts incoming photons into electrons. In our graphs, QE is expressed as a percentage. A sensor’s QE typically varies based on its architecture, coatings, and materials. High QE remains a crucial consideration for applications such as astronomy, space debris imaging, and life science research.
$14,699.00
Designed and manufactured in the USA with same extreme reliability as the thousands of FLI OEM cameras. Install in remote observatories around the world with complete confidence in a long, trouble-free life. Full frame sensor with 90% quantum efficiency and massive 43.1mm diagonal field of view to increase throughput.
| Sensor | IMX455 |
| Diagonal Size (mm) | 43.2 |
| Resolution | 9568 x 6300 |
| Pixel Size | 3.76um |
| Bit depth | 16-BIT |
| Full Well | 50ke- |
| Read Noise | 1e- |
| Dark current | 0.002 EPS @ -20C |
| Shutter | Rolling |
| Peak QE | 91% |
| Interface | USB 3 QSFP |
| Frame Rate | 4FPS |
Optional Accessories
Quantum Efficiency
Quantum efficiency (QE) measures how effectively a detector converts incoming photons into electrons. In our graphs, QE is expressed as a percentage. A sensor’s QE typically varies based on its architecture, coatings, and materials. High QE remains a crucial consideration for applications such as astronomy, space debris imaging, and life science research.
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