With the advantage of low readout noise and high-speed readout, CMOS technology has revolutionized astronomical imaging. A monochrome, back-illuminated, high-sensitivity, astronomical imaging camera is the ideal choice for astro-imagers. The QHY600M-L uses the latest SONY back-illuminated sensor, the IMX455, a full frame (35mm format) sensor with 3.76um pixels and native 16-bit A/D. This sensor is available in both monochrome and color versions. The QHY600M-PH ends the days of non-16bit CMOS cameras and it ends the days non-full frame (and larger) monochrome CMOS cameras.

The QHY600M-L has extremely low dark current (0.002e/p/s@-20C) using SONY’s Exmor BSI CMOS technology. QHY600M-PH is also a zero amplifer glow camera. The QHY600M-PH has only one electron of read noise at high gain and full resolution and 4FPS readout speed. One electron of read noise means the camera can achieve a SNR>3 at only 4 to 6 photons. This is perfect performance when conditions are photon limited, i.e., short exposures, narrow band imaging, etc., making this large area sensor ideal for sky surveys, time domain astronomy, fluorescence imaging, DNA sequencing and microscopy.

Models

QHY600 Series have mutiple models which covers both photographic and scientific using. Below list different types of QHY600 PH (photographic) series:

QHY600PH : Standard version for amateur astrographers;

QHY600PH-SBFL (Short back-focal length version) ：specially designed for DSLR lens users or those who has special requirment of short back focal length. This version has a special front part version which has 14mm B.F.L only (The B.F.L consumed equals 12.5mm when connecting QHYCFW. About the defination of “BFL Comsumed” and our adapter system please view: https://www.qhyccd.com/astronomical-camera-adapter-bfl-solution/). QHY600SBFL can easily match Canon/Nikon lens even with filter wheel. On the side of this adapter there is a 4mm hole to connect air pump through plastic pipe in case of the dewing glass when necessary.

QHY600L : a lite, shorter and cheaper version. Compared with QHY600PH, QHY600PH-Lite has the following features compared with previous models: QHY600L only has mono version; The body length becomes shorter, which is about 112mm, and its price is lowered compared with QHY600PH; The Built-in DDR3 Buffer (memory storage) is adjusted to 1GB compared to 2GB of QHY600PH/Pro. Other specifications of QHY600L keep the same with QHY600PH except the body length and weight.

The Helium ME400 Red Tripod is ideal for portable Paramount use and is available for the Paramount MEII and ME6 models:

• Provides a stable platform for all your equipment
  • Helium ME400 has a maximum payload capacity of 180 kg when the legs are fully extended, or up to 227 kg capacity when the legs are fully retracted
  • Allows eyepiece placement at a convenient height with an adjustable height range Helium ME400 from 61cm to 100 cm.
• The ultra-portable and lightweight design weighs in at 14kg

Helium MX400 Features

• Simple and intelligent mechanics permit the legs to be expanded or collapsed in seconds and produce exceptional stability at all heights
• The top plate rotates 360 degrees for hassle-free polar alignment in azimuth.
• A wide range of coarse leveling adjustments can accommodate gently sloping surfaces.
• Fine-level adjustments help achieve the optimal level
• Swiveling feet can be fit with spikes or other third-party commercial tripod feet based on your observing site (grass, wood, concrete, gravel, etc.)
• Built-in bubble level helps quickly get the top plate horizontal.
• The 6061 aluminum tripod legs are red anodized with black anodized aluminum structural components (top plate, feet, etc.)
• Large tray between the legs conveniently stows your eyepieces and other equipment
• Legs accept many off-the-shelf tripod feet (including spikes, and wide rubber pads) to optimize coupling to the observing surface

The result of these innovative features is an exceptionally stable and readily portable imaging platform that can be quickly set up on any surface, leveled and aligned with the celestial pole, and easily taken down each night.

The Helium MX400 Red Tripod is ideal for portable Paramount use and is available for the Paramount MX+ and MX6 models:

• Provides a stable platform for all your equipment
  • Helium MX400 has a maximum payload capacity of 180 kg when the legs are fully extended, or up to 227 kg capacity when the legs are fully retracted
  • Allows eyepiece placement at a convenient height with an adjustable height range Helium MX400 from 61cm to 100 cm.
• The ultra-portable and lightweight design weighs in at 14kg

Helium MX400 Features

• Simple and intelligent mechanics permit the legs to be expanded or collapsed in seconds and produce exceptional stability at all heights
• The top plate rotates 360 degrees for hassle-free polar alignment in azimuth.
• A wide range of coarse leveling adjustments can accommodate gently sloping surfaces.
• Fine-level adjustments help achieve the optimal level
• Swiveling feet can be fit with spikes or other third-party commercial tripod feet based on your observing site (grass, wood, concrete, gravel, etc.)
• Built-in bubble level helps quickly get the top plate horizontal.
• The 6061 aluminum tripod legs are red anodized with black anodized aluminum structural components (top plate, feet, etc.)
• Large tray between the legs conveniently stows your eyepieces and other equipment
• Legs accept many off-the-shelf tripod feet (including spikes, and wide rubber pads) to optimize coupling to the observing surface

The result of these innovative features is an exceptionally stable and readily portable imaging platform that can be quickly set up on any surface, leveled and aligned with the celestial pole, and easily taken down each night.

Specifications

• CCD: Sony ICX825AL ExView2 monochrome CCD
• Pixel count: 1392(H) x 1040(V)
• Pixel size: 6.45 x 6.45uM
• Optical size: 8.98 x 6.71 mm
• Read noise: Typically 5.0 electrons
• QE: Peak QE 75% (yellow light)
• Gain: 0.3 e/ADU
• Barrel size: 31.75mm dia. x 85mm long (1.25 inch eyepiece push fit size)
• Barrel thread: 25.4mm x 0.75mm ‘CS’ mount lens thread
• Input connection: ‘Mini B’ USB socket for USB2.0
• Output connection: Standard RJ12 autoguider socket
• Output type: Opto-isolated 4 lines (N,S,E & W) pull down with common return line
• Download rate: Approx. 2 frames per second in binned 1×1 mode

Specifications

• CCD type: ICX267AL Sony SuperHAD interline CCD with low dark current and vertical anti-blooming.
• CCD Full resolution pixel data: Pixel size: 4.65uM x 4.65uM, Image format: 1392 x 1040 pixels
• CCD Image area: 6.4mm (Horizontal) x 4.75mm (Vertical).
• CCD quality: Grade 1
• Spectral Response: QE max at 520nM (~50%), 30% at 420nM and 670nM.
• Readout Noise: Less than 10 electrons RMS – typically only 7 electrons.
• Full-well capacity: Greater than 15,000 e- (unbinned)
• Anti-blooming: Overload margin greater than 1000x.
• Dark current: Less than 0.1 electrons/second @ + 10C ambient.
• Data format: 16 bits.
• System gain: 0.3 electrons per ADU
• Lens details: 1.55mm FL F/2 180 degree ‘Fish Eye’
• Computer Interface: Built-in USB 2.0 compatible interface.
• Image download time: Typically 0.6 seconds at full resolution using USB 2.0.
• Power requirements: Camera is USB powered, dew heater requires 12v at 1 amp max.
• Input connection: ‘Mini B’ USB socket for USB2.0 and a 2.1mm jack for +12v heater supply.
• Cooling system: Ambient air cooling.
• Viewing dome: High quality polycarbonate hemisphere (replaceable)
• Overall size: 150mm tall x 95mm diameter

PRODUCT MANUAL Handbook-for-the-Oculus

Introducing the Starlight Xpress TRIUS PRO Series of cooled CCD cameras to our product portfolio.

The TRIUS range of cameras was introduced in 2014. These were the first cameras on the market to incorporate a powered USB 2.0 hub in the rear of the camera to enable the user to connect their USB filter wheel and guide camera directly to the camera rather than multiple cables back to the computer - simplicity and convenience.

The new TRIUS PRO Blue series follows on from that success. We have redesigned the electronics to give even lower read-noise figures and faster downloads. With the Sony CCD cameras, we are now getting read-noise figures that are better than most CMOS cameras (when used at unity gain), along with 16bit data and significantly better dark-noise figure thanks to the impressive cooling. Dark frames really are a thing of the past, making calibration frames optional rather than compulsory, giving you more time to capture data and process your images.

There's lots of advantages of using a CCD chip for deep-sky imaging compared to CMOS cameras.

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

Specifications

• CCD type: Sony ICX825AQ EXview II HAD CCD with ultra low dark current, extended IR response and vertical anti-blooming.
• CCD quality: Grade 1 or better – No bad columns, no dead pixels, no more than 6 ‘hot’ pixels (saturated in <10 seconds).
• CCD Full resolution Pixel data: Pixel size: 6.45uM x 6.45uM, Image format: 1392 x 1040 pixels
• CCD Image area: 8.98mm (Horizontal) x 6.7mm (Vertical).
• Spectral Response: QE max at 540nM (~65%), 50% roll-off at 400nM and 750nM.
• Readout Noise: Typically ONLY 3.5 electrons.
• Full-well capacity: Greater than 23,000 e- (unbinned)
• Anti-blooming: Overload margin greater than 800x.
• Dark current: Dark frame saturation time greater than 100 hours. Less than 0.002 electrons/second @ -10C.
• Data format: 16 bits.
• System gain: 0.3 electrons per ADU
• Computer Interface: Built-in USB 2.0 compatible interface with 3 port USB 2 hub for peripheral devices.
• Image download time: Typically 0.6 seconds full resolution using USB 2.0, approximately 2 seconds with USB 1.1.
• Power requirements: 115VAC / 240VAC @ 12VA, or 12VDC @ 1.5 A max.
• Cooling system: Regulated set-point cooling supply with two stage thermoelectric cooler to give a CCD temperature of better than -40C below ambient. Dry Argon fill.
• Size: 75 x 70mm black anodised aluminium barrel with 42mm ‘T2’ thread at the CCD window end & input/output plugs at rear.
• Weight: approx. 450g

PRODUCT MANUAL Trius-PRO-825C-handbook

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

The iOptron® CEM40 mount is the next generation of center-balanced equatorial mounts. This mount is incredibly eye-pleasing, and its beauty is found in more than its appearance. The functionality of the mount is superb. Weighing in at only 17.4lbs., this mount can support a payload of up to 40lbs.! That's incredible!

Innovative iOptron Technology
Make way for an innovative mount! This mount has an integrated electronic polar finder scope known as the iPolar. This tool ensures the accurate alignment of a telescope, even when the pole star is obscured. There are large levers on the quick-lock drive engagement system; these large levers make it easy to snap the gears into place.

This iOptron CEM40G mount has a dual saddle that accommodates Losmandy and Vixen-style dovetail plates. The CEM40 also uses iOptron's ultra-quiet, low-power consumption stepper motor drive system, aiding the mount in providing precise tracking.

Computerized Mount Features
The iOptron CEM40 mount uses the Go2Nova® 8407 hand controller to navigate the night sky. This incredible technology helps observers find celestial objects with the aid of the mount's 212,000+ object database! For those looking for a telescope that has the capability of tracking and finding beautiful night sky objects, this mount is a must have tool.

With the included tripod, 11lbs counterweight, and the mount's computerized technology, observers are just an OTA away from a spectacular viewing experience!

(This mount uses #8027 counterweight)

Features

• Unique design, Center-Balanced equatorial mount (CEM) for maximum payload and minimum mount weight
• Idea for both visual observation and astrophotography
• Maximum payload of 40 lbs (18 kg) with the mount weight of only 17.4 lbs (7.9 kg)
• All metal, CNC machined with red/black anodized
• Easy to use quick-lock gear clutches
• Integrated iPolar^TM electronic polar finder
• Low periodic error (< ± 7 arc seconds)
• Permanent periodic error correction (PPEC)
• Precision stepper motor for precise GOTO and accurate tracking
• Go2Nova® 8407+ controller with Advanced GOTONOVA® GOTO Technology with built-in heater
• Integrated ST-4 autoguiding port
• 32-channel Global Positioning System (GPS)
• USB communication port
• Cable management system
• 6" Losmandy D & Vixen dual dovetail saddle
• Standard 1.5 inch heavy-duty stainless steel tripod (5kg)
• Optional WiFi for mount control via SmartPhone/Tablet/Computer

Supplied with an American power supply from factory

Like their predecessors, the C262A3 is designed with portability in mind, weighing in at only 4.5kg it can support up to a 12kg payload an incredible 2.6 mount weight to payload ratio. The key to enable such ratios is the CEM design focuses the mount and payload weight directly on the center of the tripod rendering “natural stability”.

Building on the legacy of earlier CEM models we have added features for convenience and functionality. A positive lock gear engagement system (easy to use even when wearing gloves), Built-in Wi-Fi enabling unparallel connectivity and recordable permanent periodic error correction (PPEC) to repeat optimal PEC training sessions. Regarding functionality the C262A3 delivers precise pointing and accurate tracking. The CEM26 sets the new standard for compact equatorial mounts.

The center-balanced design mount puts the weight of the payload at the center of gravity allowing for greater natural stability. Other features include an adjustable counterweight bar to prevent obstruction with the tripod. And polar aligning is quick and accessible all the time since the polar scope is not blocked by the declination shaft.

The C262A3 is equipped with the latest advanced GOTONOVA® GOTO technology, making it one of the most powerful and accurate GOTO mounts available. Its database includes over 212,000+ objects. The Go2Nova® Hand Controller is intuitive to use and its large 4-line LCD screen simplifies the process of setting telescopes and locating objects.

The CEM26A mount has an integrated electronic polar finder scope known as the iPolar. This tool ensures the accurate alignment of a telescope, even when the pole star is obscured. It comes with a 1.5" heavy duty stainless steel tripod and an aluminum carrying case.

Features

• Unique design, center-balanced equatorial mount (CEM)for maximum payload and minimum mount weight
• Ideal for both visual observation and astrophotography
• Low periodic error (< ± 10 arc seconds)
• Payload of 12 kg (26 lbs) with the mount-only weight of 4.5 kg (10 lbs)
• CNC machined and cast metal body
• Spring loaded gear system
• Large easy to use quick-lock gear clutches
• 0º latitude operation with optional adapter
• Stepper motor with low power consumption
• Integrated iOptron iPolar^TM electronic polar scope
• Polar alignment routine for those who can’t see the Pole Star
• Go2Nova® 8409 controller with Advanced GOTONOVA® GOTO Technology
• Integrated ST-4 autoguiding port
• Built-in Wi-Fi
• USB port for firmware upgrade and computer control
• LiteRoc heavy-duty stainless steel tripod w/ vibration suppression pads (7.5kg)
• Die-cast metal tripod spreader with accessory tray
• Hard carrying case
• Optional 32-channel Global Positioning System (GPS)
• Optional iGuider^TM autoguiding system #3360

Supplied with an American power supply from factory

The CDK400 Observatory System from PlaneWave Instruments is designed for the sophisticated astrophotographer and dedicated astronomy researcher. This premium package combines the high-performing CDK17 optical tube with the advanced L-500 direct-drive mount to provide a superior observational platform that excels in a range of applications, from detailed celestial research to high-end astrophotography.

Key Features of the CDK400 Observatory System

CDK17 Optical Tube Assembly

• Aperture and Focal Length: Features a 17-inch aperture and a 2939 mm focal length at an f/6.8 focal ratio, optimizing it for deep-sky imaging with excellent depth and clarity.
• Advanced Optical Design: Utilizes a Corrected Dall-Kirkham optical design, delivering a field free of off-axis coma and astigmatism and achieving a perfectly flat field across a 70 mm image circle, resulting in critically sharp images across the entire viewing area.
• High-Quality Construction: Made with lightweight yet robust carbon fiber, reducing thermal expansion and allowing for rapid thermal equilibration, which helps maintain precise optical alignment under fluctuating temperatures.
• Superior Mirrors and Coatings: Equipped with high-stability fused silica mirrors known for minimal thermal expansion, paired with high-performance coatings that maximize light throughput while minimizing stray light for optimal imaging quality.
• Thermal Management: Features an advanced cooling system with strategically placed fans that promote rapid thermal stabilization, essential for maintaining consistent high-quality imaging and minimizing focus shifts caused by temperature changes.

L-500 Direct Drive Mount

• Direct Drive Motors: Employs state-of-the-art direct-drive motors on each axis, ensuring smooth, fast, and virtually silent movement of the telescope with zero backlash and zero periodic error, perfect for precise tracking and swift repositioning of celestial objects.
• High-Resolution Encoders: Outfitted with high-resolution optical encoders on both axes, providing exacting positioning and movement, crucial for top-tier astrophotography and detailed astronomical studies.
• Azimuth Dovetail Balance System: Incorporates a finely adjustable balance system that improves the stability and performance of the setup in both alt-azimuth and equatorial configurations, essential for prolonged accurate tracking and reducing stress on the mount during extended observations.
• Rapid Target Acquisition: Achieves impressive slew speeds up to 50 degrees per second, allowing for quick and efficient targeting of celestial bodies and satellites, vital for dynamic observations and responsive astrophotography.

Application-Specific Advantages

Astrophotography

The CDK400 stands out as a formidable system for astrophotographers, offering unmatched tracking accuracy and image stability which facilitate capturing spectacular celestial images with detailed resolution and vibrant colors.

Astronomy Research

Researchers will appreciate the CDK400 for its consistent performance and precise data collection capabilities. It serves as a robust platform for sophisticated photometry, spectroscopy, and minor planet tracking, offering a solid foundation for scientific discovery and exploration.

Visual Observations

For enthusiasts of visual astronomy, the CDK400 delivers vibrant and detailed views of the universe. Its significant aperture and high-quality optical components ensure exceptional viewing of planetary, lunar, and deep-sky objects, enriching every observational experience.

Space Situational Awareness (SSA) and Space Domain Awareness (SDA)

With its swift and precise repositioning capabilities, the L-500 mount in the CDK400 system is capable of tracking satellites and space debris. However, it's important to note that while the L-series mounts are highly effective for astrophotography and research applications, they might not meet the optimal performance standards required for dedicated SSA/SDA operations. For those needs, we recommend exploring our T-600 Direct-Drive Gimbal, specifically engineered to exceed the demanding requirements for SSA/SDA applications, ensuring superior tracking and responsiveness in monitoring and cataloging space objects.

Mount System 

Control System

Optical Systems

Mechanical Structure

Motion control

System Performance 

Included items

IRDK17’s Key Features

Large Aperture and Optimized Focal Ratio

The IRDK17 features a considerable 432 mm aperture and an f/6.8 focal ratio, enhancing its ability to capture infrared light effectively. This configuration is ideal for precise infrared observations and long-exposure imaging, offering superior light-gathering capabilities.

Specialized Optical Design for Infrared

The Dall-Kirkham optical design of the IRDK17 is finely tuned for infrared wavelengths. There are no refractive lenses, only reflective components made from fused silica. The reflective coatings are a protected gold with better than 98% reflectivity from .65 microns (650nm) to 5 microns (5000nm), making it optimal for infrared astronomy or LIDAR applications. UV-optimized coatings can also be provided, enhancing the telescope's versatility—please contact our technical sales team to discuss UV optimization.

Robust Mechanical Structure

Constructed using carbon fiber, the optical tube of the IRDK17 ensures durability and stability with minimal thermal expansion. This feature guarantees consistent performance across various conditions and is suitable for intensive scientific and research applications.

Advanced Thermal Management

The IRDK17 has cooling fans and a system ready for Delta-T applications, promoting rapid thermal equilibrium. This system is essential for minimizing air turbulence within the tube, reducing potential image distortion, and improving overall imaging quality.

Integrated Dew Control

Given that infrared observations are prone to condensation, the IRDK17 incorporates advanced dew-prevention technology. Heater pads, controlled via PlaneWave’s software, ensure the optical surfaces remain clear from dew, maintaining consistent and sharp imaging performance.

Application-Specific Benefits

Infrared Astronomy

The IRDK17 excels in infrared astronomy, where its large aperture and infrared-optimized optics allow for detailed observation of celestial objects in infrared light. This capability is vital for uncovering astrophysical phenomena invisible to the naked eye or conventional optical wavelengths.

Advanced Research and LIDAR Applications

With its specialized design and infrared optimization, the IRDK17 is a robust platform for advanced scientific research, including applications in LIDAR, leveraging its specialized optical capabilities.

Optical Systems

Secondary Mirror

Primary Mirror

The All NEW iOptron CEM120EC

An extraordinary innovation in mount design...Now with a new payload!

Recognizing the growing demand for an accurate and stable, equatorial mount with the versatility to carry larger instruments and more complex imaging arrays, we created the iOptron CEM120EC. It offers the benefits of our revolutionary “center balance” design: stability, accuracy, and smooth mechanical operation, while capable of carrying a payload up to 52 kg. The “center balance” design’s natural stability is due to its focusing the mount along with payloads weight directly over the center of the pier or tripod.

The CEM120EC's performance is demonstrated by its low periodic tracking error of <0.15 arcsec RMS. Along with the stability aspect, the CEM120EC features an advanced cable management system consisting of more ports in more locations preventing tangle ups and reducing the chance of fractured cables. It also adds some new features to the CEM family like Wi-Fi and LAN for remote operation and easy to use, reliable clutches on both axes.

Optional Extra's

Optional heavy duty Tri-Pier 360 and Permanent Pier are available for order.

/product/ioptron-tri-pier-360

Optional Tri-Pier adapter for light weight payload ( 8036-120) is also available for $239. It can be modified for permanent pier mounting.

Features

• A new design, center-balanced equatorial mount (CEM) for maximum payload with natural stability
• Observatory astrophotography mount ideal for both visual and Astro-photographers
• Payload of 52 kg with the mount weight of 26 kg
• Easy to use and reliable gear clutches
• Precision altitude and azimuth adjustment.
• Precision stepper motor with 0.07 arcsec accuracy for precise GOTO and accurate tracking
• Polar alignment routine for those who can't see the Pole Star
• Go2Nova® 8407 V2 controller with Advanced GOTONOVA® GOTO Technology with built in heater
• High precision tracking with low periodic error (PE)<0.15 arcsec RMS
• Real time periodic error correction (RPEC)
• 32-channel Global Positioning System (GPS)
• Built-in WiFi and LAN for remote operation
• Integrated ST-4 autoguiding port
• Advanced cable management system with more choices
• Spring loaded, individual adjustable Losmandy saddle

Specifications

Supplied with an American power supply from factory

Manuals and Instructions

Quick Start Guide

Instruction Manual

AUX port plug (DIN-422) assembly

Latest Firmware

SKU: 7301

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

Enhance your viewing experience with the Tele Vue TV 101is Accessory Kit. This package includes all the necessary add-ons for your Tele Vue 101is telescope, providing a more versatile and efficient use. Enjoy accurate and clear observations with the expertise and precision of Tele Vue products.

Package Components

PlaneWave CDK 14" Fused Silica

The CDK (Corrected Dall-Kirkham) Optical Design is an innovative solution for unsurpassed astroimaging quality at an affordable price. The CDK telescope design provides excellent imaging with large format CCD cameras while remaining superb for visual use. The CDK design far exceeds the off-axis performance of most commercial telescope designs including the Ritchey-Chrétien design.

FUSED SILICA

Fused Silica is a synthetic amorphous silica glass of the highest purity and one of the most transparent glasses made.

The optical and thermal properties of fused silica are superior to other types of glass due to its purity. Its transmission and homogeneity exceed those of crystalline quartz without the problems of temperature instability inherent in the crystalline form.

Fused Silica has a coefficient of thermal six times lower than Borosilicate glass, which means that as fused silica cools down, it preserves its shape to a high degree of accuracy. This translates into consistent optical performance and unchanging focus over temperature changes.

With high melting temperature (~1,600 degrees Celsius), a very low coefficient of thermal expansion and resistance to thermal shock, fused silica is the material of choice for professional observatories as well as various scientific applications.

This no-compromise design is unique in making the optical alignment forgiving and collimation very easy. This guarantees the user the best possible performance from the telescope. The end result at the image plane of the CDK design is no off-axis coma, no off-axis astigmatism, perfectly flat field (no off-axis defocus). The CDK design will give you pinpoint stars from the center to the corner of the field of view.

More about our Optical Design

Features:

PlaneWave CDK 14" Fused Silica Specifications

OPTICAL SYSTEM

SECONDARY MIRROR

PRIMARY MIRROR

LENS GROUP

STANDARD FEATURES

SHIPPING

NOTE: This product has a lengthy lead time. Please contact education@bintel.com.au for further information.

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.

Specifications

The Atik 490EX fully supports 1.25" filters down to f/2, so you won't need to replace any of your current investment in wheel or filters. This is an added advantage when looking to invest in a CCD camera that may go through multiple telescopes.

The Atik-4 Series cameras are a development of the renowned 3-Series cameras, featuring better cooling and narrower body. They benefit from setpoint cooling to make taking matching dark frames a snap, and simple 12V power requirement to facilitate field operation. The impressive sensitivity, great cooling and narrow profile, make the Atik Series 4 outstanding CCD cameras to use on modern telescopes, including Hyperstar/Fastar systems.

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.

The EFA PC Port Kit allows connecting the PWI Software to the PC port on the EFA Box. Each kit contains:

• a USB to Serial Converter
• an Ethernet to 9-pin Adapter and
• a short Ethernet cable

• Feathertouch 2″ Diameter Dual Speed Focuser with 2.5″ of Travel.
• Great choice for refractors and Ritchey Chretien and CDK telescopes.
• It is precision engineered to deliver smooth operation and no image shift.

Now, one person can easily balance a CDK on the L-Series mounts using the Ascend accessory! The Ascend can attach to either the front or rear of the #200919 Dovetail Clamp and precisely slide the CDK forward or back for accurate balance. Ascend uses a long pushrod to safely balance in the mount’s declination/altitude axis with the turn of a bolt.

Description

Advanced Kowa XD optical performance in a rugged compact body.

These binoculars offer high optical performance comprising bright and clear images, high resolution, and high contrast. They are easy to use and are perfect for outdoor observation. The high quality models are perfect for beginners to experienced users who want to enjoy sharp and accurately reproduced colour and contrast when viewing the natural world. Even for a large objective 56mm binocular - the BDXD are lightweight and compact, perfect for low light applications without compromising on image quality. The XD lenses and bright wide field of view delivers sharp images without chromatic aberration. A multi-coating processing is applied to all lenses and prism surfaces delivering a bright and clear field of view. Close focus performance is exceptional on all models. A tough fully waterproof and nitrogen filled magnesium alloy body makes these binocualrs suited for even the harshest of outdoor environments. Large bright 56mm objective lenses increase light transmission even further for excellent low light performance.

Techn. Details

The ATS 80 is a lightweight and handy spotting scope that offers high optical quality, despite its compact dimensions. With its angled view the ATS 80 enables comfortable observation for hours. The 80 mm objective lens diameter provides higher detail recognition, while a wider exit pupil ensures brighter images and comfortable viewing even in poor lighting conditions.

The Swarovski ATS Objective Module is an essential component for the ATS/STS spotting scope system, delivering premium optical performance for nature enthusiasts, birdwatchers, and outdoor adventurers. Designed with Swarovski Optik’s renowned precision engineering, this objective module offers crystal-clear images, outstanding edge-to-edge sharpness, and exceptional light transmission, ensuring vibrant colors and high contrast even in challenging lighting conditions.

Key Features:

• Premium Optics: Features high-quality fluoride-containing HD lenses to minimize chromatic aberration and enhance color fidelity.
• Rugged & Weatherproof: Built with a durable, lightweight aluminum housing that is waterproof and nitrogen-purged, making it ideal for harsh environments.
• Versatile Compatibility: Pairs seamlessly with the Swarovski ATS and STS eyepiece modules, allowing for customized magnification and viewing angles.
• Easy Handling: The ergonomic design and smooth focusing mechanism ensure comfortable, effortless operation in the field.

Whether you're observing distant wildlife, scanning landscapes, or engaging in digiscoping, the Swarovski ATS Objective Module delivers a superior viewing experience with the clarity and precision that Swarovski Optik is known for.

The 25-50x Wide-Angle Eyepiece for the Swarovski ATS spotting scope offers exceptional optical performance with a versatile zoom range and crystal-clear image quality. Featuring a wide field of view ranging from 42 to 27 meters at 1000 meters, this eyepiece allows for comfortable long-range observation, whether you're birdwatching, digiscoping, or surveying landscapes.

With high-quality SWAROVISION optics, this eyepiece ensures superior edge-to-edge sharpness, true color fidelity, and excellent contrast, even in low-light conditions. Its 17 mm eye relief provides comfortable viewing, making it ideal for extended use, even for eyeglass wearers.

The 2.4° to 1.55° field of view enhances situational awareness, while the smooth magnification adjustment allows you to easily zoom in on distant subjects without losing detail. Engineered for rugged outdoor use, this eyepiece is waterproof, fog-proof, and built to withstand harsh conditions.

Perfectly compatible with the Swarovski ATS/STS spotting scopes, this lightweight yet durable eyepiece is a must-have for nature enthusiasts, hunters, and professional observers who demand unparalleled optical performance.

LEICA GEOVID PRO SE 8x42

Leading high-end optics plus powerful ballistics calculator.

The Geovid Pro SE 8x42 was developed for hunting at all distances, during the day and into the twilight hours. This universal glass smartly combines everything a hunter needs for an ethical and successful hunt: premium binoculars plus a leading ballistics rangefinder. Over 30 years of experience are incorporated in these rangefinder binoculars. Their optical performance is achieved by the unique Perger-Porro prism system. High light transmission, color neutrality, excellent contrast and image sharpness are indispensable when observing and identifying game. In addition, the rangefinder with its class 1 laser delivers precise measurements up to 2000 m within fractions of a second, and provides vertical hold correction values for up to 800 m at the touch of a button. The ergonomic design with the practical reach-through bridge enables long and fatigue-free observation, while the large exit pupil ensures comfortable handling for rapid detection of game. The Geovid Pro SE 8x42 offers excellent image stability and a large field of view for an excellent overview, well into twilight. Whether stalking in the local forest, hunting in the vast savannah or in the mountains, and whether with a rifle or with a bow – the Geovid Pro SE models are utterly reliable companions for the ethical hunt.

The essentials:

• All-rounder for any hunting situation
• Leica High Definition optics for maximum image brightness and high contrast
• Rapid and precise laser rangefinding up to 2000 m
• Vertical hold correction up to max. 800 m via integrated Applied Ballistics calculator
• LPTTM (Leica ProTrack) tracking assistant for finding game after the shot

IN THE BOX

• Geovid Pro SE 8x42, Carrying Case, Carrying Strap, Lens Cleaning Cloth, Quick Start Guide.

saxon Fluorescent Biological Microscope 40x-1600x

The saxon Fluorescent Biological Microscope is specifically designed for educational and laboratory use. Built with a die-cast base for enhanced stability and an ergonomic design, this microscope features a transmitted light and fluorescence reflective lighting system for versatile applications.

Key Features:

• Magnification: 40x/ 64x/ 100x/ 160x/ 400x/ 640x/ 1000x/ 1600x for high-detail observations
• Large Dual-Layer Mechanical Stage: Offers smooth and precise movement.
• Coarse & Fine Focusing: Ensures detailed observation.
• Illumination: In-built adjustable brightness LED Light

Applications:

• Biological Research: Study cell biology, protein localization, and live cell imaging.
• Pharmaceutical and Drug Development: Drug target validation and toxicology studies
• Education:  Used in schools and universities to teach students about cellular structures and processes

Large Aperture and Optimized Focal Ratio

The IRDK24 features a generous 610 mm aperture paired with an f/6.5 focal ratio, enhancing its ability to capture light effectively. This combination is ideal for detailed infrared observations and long-exposure imaging, providing superb light-gathering capabilities.

Specialized Optical Design for Infrared

The Dall-Kirkham optical design of the IRDK24 is optimized for infrared wavelengths. There are no refractive lenses, only reflective fused silica mirrors. Reflective coatings are a protected gold with better than 98% reflectivity from .65 microns (650nm) to 5 microns (5000nm), ideal for infrared astronomy or LIDAR applications. UV-optimized coatings can also be provided, so please contact our technical sales team to discuss UV optimization.

Robust Mechanical Structure

Constructed using carbon fiber, the optical tube of the IRDK24 offers durability and stability with minimal thermal expansion. This design ensures consistent performance under varying environmental conditions, making it suitable for intensive scientific applications.

Advanced Thermal Management

The IRDK24 incorporates cooling fans and a system ready for Delta-T applications, facilitating rapid thermal equilibrium. This setup is crucial for minimizing air turbulence within the tube, thus reducing potential image distortion and enhancing overall imaging quality.

Integrated Dew Control

Infrared observations can be susceptible to condensation, but the IRDK24 addresses this with sophisticated dew prevention technology. Heater pads, controlled via PlaneWave’s software, ensure the optical surfaces remain clear from dew, thereby maintaining consistent and clear imaging performance.

Application-Specific Benefits

Infrared Astronomy: The IRDK24 is especially effective for infrared astronomy, where its large aperture and infrared-optimized optics allow for detailed observation of celestial objects in infrared light. This capability is essential for studying astrophysical phenomena invisible to the naked eye or standard optical wavelengths.

Advanced Research and LIDAR Applications: With its specialized design and infrared optimization, the IRDK24 is a robust platform for advanced scientific research, including LIDAR.

Optical Systems

Primary Mirror

Secondary Mirror

CDK24’s Key Features

Large Aperture and Moderate Focal Ratio

The CDK24 features a substantial 610 mm aperture and a moderate f/6.5 focal ratio. This setup enhances its capability to capture deep-sky objects with remarkable detail, providing excellent light-gathering efficiency and a broad field of view for research and imaging.

Advanced Optical Design

Equipped with a state-of-the-art Corrected Dall-Kirkham optical system, the CDK24 offers exceptional image clarity. Its design eliminates off-axis coma and astigmatism and delivers a perfectly flat field, ensuring images are sharp and detailed across the entire field of view with minimal post-processing adjustments.

Robust Mechanical Structure

Constructed with a carbon fiber optical tube, the CDK24 is lightweight and durable. Its thermal expansion coefficient ensures minimal focus shift as temperatures change, making it ideal for prolonged observing sessions under varying environmental conditions.

High-Performance Mirrors and Coatings

Utilizing fused silica mirrors, the CDK24 maintains precise optical alignment and surface accuracy, even with temperature fluctuations. Its high-quality coatings enhance light transmission and reduce stray light, optimizing performance for specialized observational tasks.

Thermal Management

The CDK24 is equipped with cooling fans and a Delta-T ready system to achieve thermal equilibrium swiftly. These features help to minimize air turbulence within the tube, thus reducing image distortion and maintaining consistent imaging quality.

Integrated Dew Control

The telescope incorporates advanced dew prevention technology with heater pads controlled by PlaneWave’s software. This ensures that optical surfaces remain clear of condensation during humid conditions, thus maintaining clear and consistent imaging performance.

Application-Specific Benefits

Astrophotography

With its large image circle and exquisite field flatness, the CDK24 allows astrophotographers to capture expansive and breathtaking views of the cosmos with incredible detail and clarity.

Astronomy Research

The precise and stable imaging capabilities of the CDK24 make it an invaluable tool for academic institutions and observatories engaged in complex astronomical research, including deep-sky surveys and detailed photometric studies.

Visual Observations

The CDK24 excels in visual observation, offering bright and crisp views ideal for star parties and serious visual astronomy. The telescope's large aperture and superior optical quality provide stunning views of planetary, lunar, and deep-sky objects, making every viewing session a remarkable experience.

Space Situational Awareness (SSA) and Space Domain Awareness (SDA)

The CDK24 also lend itself to applications in Space Situational Awareness and Space Domain Awareness. Its capability to provide detailed observations can be essential for tracking and monitoring satellites and other space debris, contributing valuable data for space traffic management and safety initiatives.

Optical Systems

Secondary Mirror

Lens Group

Primary Mirror

The BTX combines the visual power of both eyes with a revolutionary viewing experience. Crucial subtleties can be seen with the crystal clear optics, with every detail now fully on show. A forehead rest and angled view guarantee comfortable viewing for hours on end.

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 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
• 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.

The left image shows a flat field image taken with a camera using an iris type shutter. The right image is a flat field image taken under the same conditions using our even-illumination shutter.

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.

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 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:

• MaxIm LT software 
• 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 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.