Atik Infinity Colour

Technical Specification

• Sensor Type: CCD - Sony ICX825
• Horizontal Resolution: 1392 pixels
• Vertical Resolution: 1040 pixels
• Pixel Size: 6.45 µm x 6.45 µm
• ADC: 16 bit
• Readout Noise: 6e- typical value
• Gain Factor: 0.37e-/ADU
• Full Well: ~24,000e-
• Speed: 2-3 frames per second
• Interface: USB 2.0 High Speed and ST4 compatible guide port
• Power: 12v DC 1A
• Maximum Exposure Length: 120 s
• Minimum Exposure Length: 1/1000 s
• Cooling: Passive
• Weight: approx. 340 gr
• Backfocus: 13mm

Link to Video from the Atik You tube channel below :

https://www.youtube.com/watch?v=28nuK8X6xbw

Specifications for the Atik 414EX Mono

Sony EXview HAD CCD II ICX825 sensor - Super Sensitive

The fact that you're reading this this shows you've made it past the most common trap in choosing a camera for astroimaging - how many megapixels is it?

There are 2 variables in your camera that are far more important to consider when imaging faint deep sky objects. Sensitivity and noise.

The sensitivity tells us how many precious photons will be converted to signal...this is were the new Sony ICX825 shines! But how much more sensitive is it? Compared with Atik's previous 314L+ at 650nm, the 414EX is 60% more sensitive. In fact, the 414EX is even more sensitive than the already spectacular 460EX, making it the perfect camera for the enthusiast with a limited budget. The graph below shows the striking difference between the ICX285 and ICX825:

Low noise and effective cooling

Atik's 414EX has more than just great sensitivity.

Another feature of the 414EXmaking it a winner for astrophotography is it's exceptionally low noise. When capturing a stunning portrait of your favourite deep sky target you will understand how delicately faint it is. This means the data you wish to capture is sparse.

If the electronics of the camera add noise (unwanted signal) to your image the end result will be lacking in detail and contrast. To ensure the contribution from noise is minimised Atik's 414EX has thermoelectric cooling that can easily lower the CCD chip to 30ºC below ambient, and is regulated, so that your image calibration is consistent. This results in a noise level so low that for most applications dark frames are an option rather than a requirement. The upshot is that you can spend more time imaging!

An image of M106 taken with Atik 414EX (courtesy of atik-cameras.com)

Specifications for the Atik 414EX Colour

Sony EXview HAD CCD II ICX825 sensor - Super Sensitive

The fact that you're reading this this shows you've made it past the most common trap in choosing a camera for astroimaging - how many megapixels is it?

There are 2 variables in your camera that are far more important to consider when imaging faint deep sky objects. Sensitivity and noise.

The sensitivity tells us how many precious photons will be converted to signal...this is were the Sony ICX825 shines! But how much more sensitive is it? Compared with Atik's previous 314L+ at 650nm, the 414EX is 60% more sensitive. In fact, the 414EX is even more sensitive than the already spectacular 460EX, making it the perfect camera for the enthusiast with a limited budget. The graph below shows the striking difference between the ICX285 and ICX825:

Low noise and effective cooling

Atik's 414EX has more than just great sensitivity.

Another feature of the 414EXmaking it a winner for astrophotography is it's exceptionally low noise. When capturing a stunning portrait of your favourite deep sky target you will understand how delicately faint it is. This means the data you wish to capture is sparse.

If the electronics of the camera add noise (unwanted signal) to your image the end result will be lacking in detail and contrast. To ensure the contribution from noise is minimised Atik's 414EX has thermoelectric cooling that can easily lower the CCD chip to 30ºC below ambient, and is regulated, so that your image calibration is consistent. This results in a noise level so low that for most applications dark frames are an option rather than a requirement. The upshot is that you can spend more time imaging!

Full-Frame Products Comparison

The ASI4400MC Pro is the latest addition to ZWO’s full-frame deep-sky camera lineup.
Positioned between the ASI6200MC Pro and the ASI2400MC Pro, the ASI4400MC Pro strikes the perfect balance between image quality and efficiency, giving users a versatile option within the full-frame lineup.

Comparison Table:

Full-Frame for a wider field of view

The ASI4400MC Pro uses a full-frame, back-illuminated sensor measuring 36 × 24 mm with a 43.3 mm diagonal. With 44 megapixels and 4.4 μm pixels, it delivers incredible resolution and light sensitivity in every shot. The full-frame format lets you capture the entire field your optics can deliver - no cropping, no lost edges - perfect for wide-field targets and large deep-sky objects. Each pixel supports a full-well capacity of 74,600 electrons, providing exceptional dynamic range. Bright stars retain their natural color and detail, while faint nebula structures and galaxy arms remain beautifully visible. The result is cleaner, more balanced images with outstanding tonal depth across the frame.

High Dynamic Range, Capturing Both Highlights and Faintest Details

The ASI4400MC Pro features a 14-bit analog-to-digital converter (ADC) that delivers a dynamic range of over 13 stops. This wide range allows a single exposure to capture both bright highlights and faint shadow details without clipping. Whether you’re imaging bright stars, nebula cores, or the delicate wisps of distant galaxies, more tonal information is preserved for smoother gradients and richer color depth. The result is a natural, well-balanced image straight out of the camera, with plenty of flexibility for post-processing and fine-tuning.

Efficient Cooling, Protecting Image Quality

The ASI4400MC Pro uses a powerful two-stage TEC cooling system capable of lowering the CMOS sensor temperature by 30°C to 35°C below ambient. This deep cooling dramatically reduces dark current and thermal noise, keeping your images clean and smooth - even during long exposures that last several minutes. The result is higher signal-to-noise ratio and improved image quality in every frame.
Note: Cooling performance varies with ambient temperature. The lower the ambient temperature, the smaller the achievable differential. Results are based on tests at 30°C ambient. While not found often in Australia, operation below -20°C is not recommended.

Glow Suppression Function*

The ASI4400MC Pro camera features ZWO’s proprietary Glow Suppression technology, which effectively controls sensor glow and maximizes overall imaging performance. This technology is implemented directly at the hardware level and does not require any software intervention.

USB 3.0 & 512MB DDR3 Memory

The ASI4400MC Pro includes a high-speed USB 3.0 interface with a built-in 512 MB DDR3 memory buffer. This design ensures fast and stable data transfer while reducing the risk of dropped frames or transmission errors. The result is reliable image capture, even during long exposures or high-speed downloads.

Anti-dew

The ASI4400MC Pro features a built-in polyimide heater bonded to the protective window to prevent dew and frost buildup, ensuring clear and reliable imaging throughout the night. 

* The heater draws about 5 watts of power and can be turned off through the software when conditions allow, not only to save power but also to reduce the load on USB hubs and external power supplies. 

*While Glow Suppression significantly reduces CMOS sensor glow, it does not eliminate it entirely. A small amount of glow may still be present; however, with dark-frame calibration, it has no impact on the final image quality.

Sensor Tilt Adjustment

The ASI4400MC Pro includes three sets of sensor tilt adjustment screws. Each set has a push and a pull screw that let you fine-tune the sensor’s alignment with your telescope’s optical axis. This adjustment helps correct any slight tilt that can cause stars to appear elongated or out of focus toward the edges of the frame, ensuring sharp, even focus across the entire image.

Camera Performance

The ASI4400MC Pro offers a dynamic range of up to 13 stops, allowing it to capture both bright highlights and faint shadow details in a single exposure. This wide range is key to achieving high dynamic range (HDR) performance, preserving fine tonal transitions and subtle color detail in deep-sky images. When the gain setting reaches 136, the camera automatically activates HCG (High Conversion Gain) mode, which greatly reduces read noise while maintaining full dynamic range. This means you can increase sensitivity for faint targets without adding unwanted gain noise, making it easier to capture clean, detailed images under a variety of conditions.

QE Value

The QE peak value of the ASI4400MC Pro camera is 80%.

Ultra-low Dark Current

Thanks to the ASI4400MC Pro’s advanced cooling system, thermal noise remains extremely low even during long exposures lasting several minutes. Dark current is a small electrical signal created by heat inside the sensor rather than by incoming light. By keeping the sensor temperature low, the camera minimizes this effect, producing cleaner, higher quality images with smoother backgrounds.

UV-IR Cut Filter

The ASI4400MC Pro is equipped with a UV-IR cut filter mounted in front of the sensor. This protective filter blocks unwanted ultraviolet and infrared light that can cause star bloat and color distortion, allowing only visible wavelengths to reach the sensor. By filtering out these non-visible wavelengths, the camera produces sharper stars, more accurate colors, and overall improved image quality in astrophotography.

Product Details

Lightweight Body: 700g
Interface Layout: USB 2.0, USB 3.0, DC
Fan Position & Heat Dissipation Vents
All-Metal Red Body

Connection Method

Mechanical Diagram

What's in the box?

Note：

External power supplies are needed for all ASl-cooled cameras. We recommend you use a 12V@3A~5A DC adapter (D5.5×2.1mm, center pole positive) or a lithium battery with 11-14V to power the camera. If the voltage exceeds this range, the camera will activate its automatic protection mechanism.

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

The Atik 383L+ is an 8-megapixel camera using the Truesense KAF-8300 CCD. Much has been written about this CCD to justify its place in astronomers' hearts. It can be succinctly summed up by saying that it's a fabulous CCD, with a huge number of good-sized pixels, and is currently available at an irresistible price.

This sensor has redefined mid-range astro-imaging, making multi-megapixel cooled cameras much more accessible.

Atik prides itself on providing cameras offering the very highest image quality at a reasonable cost. They have built on the success of the highly-regarded Atik 314 platform to support Kodak's KAF-8300. This immediately offers a huge number of advantages, including the very low read-noise circuits and the reliability of using this established design.

Specifications for the Atik 383L+ Mono

Mechanical Drawing

Quality hardware

The key to any high-quality camera is the ability to convert light collected by the sensor into digital information while ensuring that as little noise as possible is added. The digital image needs to truly reflect the light collected. The Atik 383L+ achieves this, by having:

• Very low read-noise, 7 electrons, on par with many Sony sensors, enabling faint details to be detected.
• Great linearity, with a regression correlation coefficient of R = 0.9998 over the range of 1,000 to 64,000, making the camera suitable for sensitive photometric measurements.
• The bias frame histogram from the camera shows the ideal Gaussian shape, indicating that maximum detail can be extracted on processing.

The Atik 383L+ is a dream combination of low-noise electronics and a scientific-grade sensor that we are able to offer at a fantastic price. Whether you are an established imager or are just starting, the Atik 383L+ is a great choice.

Instruction Manual

There's lots of advantages of using a CCD chip for deep-sky imaging compared to CMOS cameras. If you'd like to know more, read BINTEL's tech article here.

Please note this camera uses a "Grade 1" CCD chip.

Specifications

• CCD type: Sony ICX674ALG (mono) EXview CCD with ultra low dark current and vertical anti-blooming.
• CCD Full resolution pixel data: Pixel size: 4.54uM x 4.54uM, Image format: 1940 x 1460 pixels
• CCD Image area: 8.81mm (Horizontal) x 6.63mm (Vertical).
• CCD quality: Grade 1 or better – No bad columns, no dead pixels, no more than 50 ‘hot’ pixels (saturated in <10 seconds).
• Spectral Response: QE max at 580nM (~77%), 50% roll-off at 360nM and 770nM.
• Readout Noise: Typically only 3.5 electrons RMS
• Full-well capacity: Greater than 17,000 e- (unbinned)
• Anti-blooming: Overload margin greater than 800x.
• Dark current: Less than 0.003 electrons/second @ – 10C CCD temperature.
• Data format: 16 bits.
• System gain: 0.3 electrons per ADU
• Computer Interface: Built-in USB 2.0 compatible interface.
• Image download time: Typically 2 seconds at full resolution.
• Power requirements: 115VAC / 240VAC @ 12VA, or 12VDC @ 900mA max.
• Cooling system: Regulated set-point cooling supply with thermoelectric cooler to give a minimum CCD temperature of approximately -40C below ambient.
• Size: 75 x 70mm black anodised aluminium barrel with 42mm ‘T2’ thread at the CCD window end & input/output plugs at rear. CCD alignment screws are provided for setting the chip parallel to the focal plane.
• Weight: approx. 450g.

PRODUCT MANUAL Trius-PRO-674-handbook

PRODUCT DATASHEET 2022-SX-TRIUS-PRO-Blue-Camera-Specification

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.

Aluma CCD Features include:

• 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 SmartCooling^TM 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.

SmartCooling^TM

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

Aluma CCD 814 Instruction Manual

Our new high performance Aluma CCD 694 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 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.

Aluma CCD Features include:

• 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 SmartCooling^TM 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.

SmartCooling^TM

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

SBIG Aluma CCD 694 Instruction Manual

Atik One 6.0 + Atik GP + OAG Kit (Atik One Integrated Kit)

Atik One Integrated Kit

Looking for great value? For a limited time, you get three in one, the Atik One with the Atik GP, plus an M42 off-axis guider for an unbelievable price. Perfect for intermediate to experienced astrophotographer’s looking for a cooled CCD camera that takes stunningly detailed deep sky images.

The off-axis guider is a smaller version of our OAG, with the renowned smooth focusing system and moveable prism. Please note: The Kit is designed to be used as a single unit with the Atik One 6.0 or the Atik One 9.0. Its parts aren’t for independent use.

Atik One 6.0

The Atik One 6.0 features the same incredible 6 megapixel Sony ICX694 EXview sensor as our highly renowned Atik 460EX camera for outstanding sensitivity at a fantastic resolution purposely engineered for deep sky imaging. Housed in an advanced body with internal filter wheel, the One 6.0 provides an all-in-one solution for mono imaging.

Features of the One

Integrated and powerful, the Atik One series embodies Atik’s principles to bring you a high performance, simple to use platform, with internal filter wheel, all in a very compact and light package. It features an improved cooler, capable of reaching a stable -38C below ambient, and a CCD chamber design, filled with high purity Argon for a dry, condensation free environment and optimal thermal insulation.

The Atik One also features an internal USB hub and accessory power port, so that you can keep the cable clutter under control. In addition, two 1/4” tripod mounting holes are available to give you more options for mounting the camera and other accessories.

The 5 position integrated 1.25″ filter wheel features a mechanical roller for filter location ensuring the highest levels of reproducibility image after image. The filter wheel is natively controlled from our software or has an ASCOM driver for third party programs. Also included is a tool that allows filters to be loaded without opening the camera.

What's in the box?

• Atik One camera body
• Atik GP camera body
• M42 Off-axis guider body
• 2" adapter
• 0.5m mini-USB cable
• 3m USB cable
• 1.8m battery power connector
• CD-ROM with drivers, software and user's manual (PDF)
• Quickstart guide (paper)

Our highly acclaimed Artemis Capture software is included for camera control and data acquisition, along with a full ASCOM driver. These are also available from our Downloads page.

A universal (110-230V) power adapter is optional.

• Sensor Type: CCD - Sony ICX814
• Horizontal Resolution: 3380 pixels
• Vertical Resolution: 2704 pixels
• Pixel Size: 3.69 µM x 3.69 µM
• ADC: 16 bit
• Readout Noise: 5e- typical value
• Interface: USB 2.0 High Speed, with embedded hub
• Power: 12v DC 2A
• Maximum Exposure Length: Unlimited
• Minimum Exposure Length: 1/1000 s
• Cooling: Termoelectric set point with max ΔT=-38°C
• Weight: approx. 900 gr
• Backfocus: ~27mm
• Exclusively as mono

Convenience of use has been key during the design. The Atik One also features an internal USB hub and accessory power port, so that you can keep the cable clutter under control. Only 2 cables for your imaging gear! In addition to this, two 1/4” tripod mounting holes are available, to give you more options for mounting the camera, other accessories, or for managing the cables.

The 5 position integrated 1.25″ filter wheel features a mechanical roller for filter location ensuring the highest levels of reproducibility image after image. The filter wheel is natively controlled from our software or has an Ascom driver for 3rd party programs. To make filter changing less of a chore the camera comes with a tool to allow filters to be loaded without opening the camera.

Atiks own capture software (Artemis) is included for camera control and data acquisition, and plug-ins are included to allow use with Astroart and Maxim DL.

Dawn image processing software is also included.

System Requirements:

• Pentium IV PC with 512MB RAM
• Windows XP/Vista/Win7/Win8/Win8 (not RT)
• CD-ROM drive
• USB 2.0 port

A universal (110-230V) power adapter is optional.

The 12 megapixel sensor of the Atik 4120EX is the ideal solution for capturing stunning high resolution images. Exclusively available as one-shot colour (OSC), this is an ideal match for Hyperstar systems and short focal length telescopes. The small 3,1 µm pixels are able to faithfully record the colour of stars and nebulae, even in the fastest imaging systems. The high resolution means you can print your images to A3 and beyond, while the famed sensitivity of the Sony EXview sensor ensures those images are brimming with detail.

Features of the 4-Series

Our 4-Series is designed in such way as to combine power and control with flexibility and ease of use. The narrow body makes them ideal for use on Hyperstar and Fastar systems whilst maintaining suitability with a huge range of other telescopes. They feature fully regulated set-point cooling which makes for easy and consistent image calibration, though they feature such low noise that dark frames are no longer even a requirement, meaning you can spend more time imaging the things that matter.

The slim, ergonomic design of these cameras naturally comes in at a low weight to help minimize stress on the corrector plate. The desiccant port is readily accessible from outside the camera for easy maintenance , and a simple 12V power requirement is complimented by low power use to help you get the most out of your imaging sessions, whether in the observatory or out in the field.

EXview

All of our 4-EX series cameras use sensors embedded with Sony EXview HAD CCD II™ technology which results in outstanding Quantum Efficiency, incredibly low read noise and excellent thermal management. These high Quantum Efficiencies make for impressive sensitivity across a vast range of wavelengths, but become particularly outstanding when imaging in narrowband, capturing stunning levels of detail in even the faintest of objects.

Atik Infinity Mono

Technical Specification

• Sensor Type: CCD - Sony ICX825
• Horizontal Resolution: 1392 pixels
• Vertical Resolution: 1040 pixels
• Pixel Size: 6.45 µm x 6.45 µm
• ADC: 16 bit
• Readout Noise: 6e- typical value
• Gain Factor: 0.37e-/ADU
• Full Well: ~24,000e-
• Speed: 2-3 frames per second
• Interface: USB 2.0 High Speed and ST4 compatible guide port
• Power: 12v DC 1A
• Maximum Exposure Length: 120 s
• Minimum Exposure Length: 1/1000 s
• Cooling: Passive
• Weight: approx. 340 gr
• Backfocus: 13mm

Link to Video from the Atik You tube channel below:

https://www.youtube.com/watch?v=28nuK8X6xbw

The One 9.0 mono is Atik's latest and greatest Sony based camera. It features a 9MP ICX814AL with the incredibly sensitive EXview HAD II technology, ultra-low read noise, a mechanically indexed 5 position filter wheel, and boosted cooling performance.

It also features a new CCD chamber design, purged with high purity Argon, and an integral USB 2.0 hub and a power port for accessories. You can now use just two cables to operate your entire system!