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Paramount ME Series 6 - The Binocular and Telescope Shop

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From $36,350.00

Introducing the new Paramount ME Series 6 observatory workhorse.

The Paramount ME Series 6 represents the latest in gear-driven GEM performance.

Its new features include a state-of-the-art MKS 6000 telescope control system that lets you connect via USB C, Ethernet, and Wi-Fi. Its two-port USB 2.0 hub is conveniently located on the instrument panel

The Paramount ME Series 6 remains an observatory favorite among professional and advanced-amateur astronomers.

On-axis Absolute Encoders vs. Motor-based Encoders.

Paramount's equipped with on-axis absolute encoders know where they are at all times. Paramount's with incremental encoders (or motor-based encoders) know only how far they have moved since they were initialized using a nightly process called homing.

The crucial additional difference is that the on-axis absolute encoders are fitted directly to the mount axes themselves, bypassing the worm drives. Paramount's with incremental encoders are fitted to the worms instead, which means that with incremental encoders alone, periodic errors in the worm drive show up in the tracking. These mounts must be calibrated and corrected using a process called periodic error correction (PEC), which measures and records the repeatable gear train errors and removes them. (TheSky features advanced, multi-harmonic PE detection and PEC calibration that minimizes periodic error in mounts with incremental encoders.)

For mounts with incremental encoders, homing re-zeros the encoders when precise sensors on each of the axes are reached. From then on, the incremental encoders are in effect delivering absolute readings.

However, the crucial additional difference remains, namely that the incremental encoder system is behind the worm drive, and periodic error correction is still required to get the best out of the RA tracking.

High-resolution on-axis absolute encoder technology is significantly more expensive than incremental encoders.

Are on-axis absolute encoders right for me ?

The short answer is, “it depends.”

Gear-driven Paramounts equipped with on-axis absolute encoders do not have periodic error, require no mechanical initialization (or homing), and the number of TPoint pointing samples needed for precision calibration is reduced.

These advantages expedite nightly setup, negate one-time periodic error training, and shorten the calibration process require to achieve spectacular pointing and tracking performance. However, the Paramount worm gear's uncorrected periodic error is low (below 7 arc seconds peak to peak), and, after a one-time PE training, periodic error correction (PEC) generally make it negligible. The Paramount without on-axis absolute encoders requires a nightly Find Home process that usually takes a minute or less to complete.

So, at least with Paramounts, periodic error is effectively in the noise, and homing straightforward.

What about pointing and tracking?

Without on-axis absolute encoders, Paramounts routinely produce 5-to-10-minute unguided exposures; many have reported 20 minutes. Also without on-axis absolute encoders, Paramount’s produce all-sky pointing accuracies at or below 30 arcseconds RMS (usually less than 15 arcseconds on fixed mirror telescopes).

Paramount’s exceptional software makes the above performance possible. TheSky Professional edition, in conjunction with TPoint™ and ProTrack™ the mount’s position is continually updated in both axes to correct system-wide pointing and tracking errors caused by tube flexure, atmospheric refraction, polar misalignment, harmonic errors from mis-centered encoders and/or worm gears, and more.

On-axis absolute encoders alone cannot correct these errors which exist with all telescopes. A properly applied telescope model is necessary to achieve superior pointing and tracking.

So are on-axis absolute encoders right for you? Perhaps if you want to enjoy the conveniences mentioned above. And for many, that’s enough. With that said, the optional on-axis 26-bit Renishaw absolute encoders with 0.02 arc second precision are the finest available and they operate in temperatures between +80°C and –40°C.

Hardware Specifications

109 kg instrument capacity; 218 kg maximum payload capacity (instruments + counterweights)
All sky pointing accuracies at or below 30 arcseconds RMS
Unibody mount design weighs 38 kg without counterweights or counterweight shaft
Maximum seven (7) arcseconds peak-to-peak periodic error before correction
After a one-time training, periodic error is 1 arcsecond, peak-to-peak or less
Optional 26-bit Renishaw encoders eliminate periodic error and the need for homing; operates in temps as low as –40° C
If you skip encoders now and later decide you want them, they can be retrofitted on the Paramounts ME Series 6
As there’s some confusion about what encoders can and cannot do, there’s an FAQ below that elaborates on that and whether they’re right for you
Its encoder cables are located inside the mount to help prevent snags.
All electronics and through-the-mount cables are housed inside the mount with ample room for additional cables
Its state-of-the-art MKS 6000 telescope control system (TCS) lets you connect via USB C, Ethernet, and Wi-Fi
Two-port USB 2.0 hub located on instrument panel
Included Versa-Plate™ conveniently accepts most telescopes
48V DC power supply and PC-to-mount USB and Ethernet cables included
Two 14 kg counterweights included. You may need more if your imaging system weighs more than 28 kg.
Belt-driven gears with spring loaded worm gears produce virtually zero backlash
Durable and fade-resistant red powder coating and black anodized finish; components are aluminum
Clutch-free design helps maintain its TPoint™ assisted pointing accuracy
AutoHome™ homing capability ensures the mount always knows its orientation (after performing an initializing process called “homing” that typically takes less than a minute)
Calibrated azimuth and elevation polar alignment adjustments speed polar alignment

Software Specifications

Paramount’s unequaled pointing and tracking wouldn’t be possible without its TPoint™ and ProTrack™ software.
By employing TPoint’s calibration and telescope modeling tools, you’ll enjoy all sky pointing accuracies at or below 30 arcseconds RMS. Nothing outperforms that
Operating in conjunction with TPoint ™, ProTrack™ continuously updates the mount’s position across both axes to correct system-wide tracking errors including tube flexures, atmospheric refraction, polar misalignment, harmonic errors from mis-centered encoders, and more.
On-axis absolute encoders alone cannot correct these errors which exist with all telescopes. A properly applied telescope model is necessary to achieve superior tracking.
Without encoders, the Paramount ME Series 6 can deliver uncommonly long unguided exposures (one customer reported 20 minutes).
For more information about what encoders can and cannot do, please see the FAQ below.
All the included software is integrated into a single, easy-to-use, application consisting of TheSky™ Professional, TPoint™, Cameras+, Domes, Multi-OS+, and Weather modules.
You can control all your astrophotography-related cameras and devices with this one app.
It runs on macOS™, Windows™, Ubuntu™, and Linux (x86_64 and ARM64 architectures).
Regardless of the operating system you run it on, it appears and operates identically. You can even switch between operating systems and its license allows up to six computers. Why paint yourself or your institution into a corner?
Absent ProTrack™ which is unique to Paramount, the included software is sold separately as TheSky™ Universal Bundle and represents a US$1,095 value.

SKU: SB10616

Optional Black Anodised mounts available on request

Available to order

ZEISS Victory HT 10x54 T* LotuTec black - The Binocular and Telescope Shop

ZEISS Victory HT 10x54 T* LotuTec black

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$4,299.00

The Victory® HT premium binoculars allow you to experience nature in a whole new dimension. Thanks to the revolutionary optical concept, they offer transmission levels of 95%+. This outstanding value is achieved through the perfect combination of SCHOTT HT lenses, ZEISS T* multi-layer coating and Abbe König prism system. You can enjoy unrivalled brightness and an extraordinary level of detail – even in the deepest twilight. The ergonomic design is equally innovative. The impressive new Comfort Focus concept has a large focusing wheel embedded in the double-link bridge. It makes the binoculars extremely robust and very easy to use. Experience cutting-edge optics of the highest level – with the brightest premium binoculars in the world.

The 10x magnification provides an incredibly detailed view. Highlights of the 10x54 include the extreme brightness and the exceptionally high contrast. With the robust and compact construction, they offer nature lovers the highest level of optics even in challenging light conditions.

95% Light Transmission

High Transmission SCHOTT glasses for optimum identification and resolution of targets in low light. The bright, high-contrast images provide you with the extra few minutes you need on a hunt. After all, it is often the first or last light of the day that is vital for those magic hunting moments that will always remain in your memory.

Optimised lens diameter

Optimised objective lens diameter for reduced weight. This ensures smooth imaging in any situation, however they are held. In this way, the design supports the highest standards of perfect visual experiences.

ComfortFocus concept

The conspicuously large focusing wheel and extra long translation enable you to focus with extreme precision to obtain the perfect focus, even when wearing gloves.

A clear view, whatever the weather

There are always exciting things to be seen in the world of nature – even in wet weather. This is why ZEISS developed LotuTec®. A coating for the lenses of binoculars and spotting scopes that enables a clear and unhindered view in all weather conditions.

ZEISS T* Coating

ZEISS T* coating is a guarantee of the brilliant, high-contrast images which you will experience above all in adverse light conditions and in the twilight. Behind it, however, there is no specific formula for building up the layers. Instead, it is a technology that is constantly adjusted to suit new glass materials and requirements, which varies from lens to lens.

Specifications

Magnification	10 ×
Effective lens diameter	54 mm
Light transmission	95%
Exit pupil diameter	5.4 mm
Twilight factor	23.2
Field of view at 1,000 m (yds)	110 m (330 ft)
Subjective viewing angle	63° Ww
Close focusing distance	3.5 m (11.5 ft)
Diopter adjustment range	− 3.0 \| + 3.0 dpt
Exit pupil distance	16 mm
Pupil distance	58 – 76 mm
Lens type	FL/HT-Type
Prism system	Abbe-König

Features

LotuTec \| Nitrogen filled	+ \| +
Water resistance	500 mbar

Specifications

Operating temperature	− 30°C \| + 63°C
Length	193 mm
Width at an interpupillary distance of 65 mm	142 mm
Weight	1.05kg

Available to order

Sky-Watcher 130 Black Diamond Reflector OTA

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$599.00

Out of stock

SBIG Aluma AC2020BSI

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From $15,889.00

SBIG Aluma AC2020BSI

Extreme sensitivity back-illuminated Scientific CMOS camera. 4-megapixel sensor with 6.5-micron pixels, Adaptive Optics capable, StarChaser Guider compatible.

SBIG Aluma AC2020BSI features a Class 1 sensor.

A fused silica chamber window is available with VIS-NIR and UV-VIS optical coating options.

Coming soon – available for preorder.

The SBIG Aluma AC Series represents the state-of-the-art in Advanced Scientific CMOS cameras for astronomical imaging systems. The camera’s advanced design permits high-speed download via the USB 3.0 connection to the control computer. The SBIG Aluma AC2020BSI uses the Gpixel GSENSE2020BSI-H CMOS sensor with 4 million pixels at 6.5 microns in a 2048 x 2048 array. The sensor measures just over 13.3mm square. The Aluma AC series has powerful two-stage cooling and supports optional water cooling. Aluma AC cameras can be operated directly from a 12VDC 8A power supply.

Design features include:

Back-Illuminated Sensor

Incredible sensitivity! High-performance back-illuminated sensors are flipped over and thinned during manufacture, so incoming light does not encounter any circuitry before hitting the sensitive pixel area. This provides optimum sensitivity across the entire visible spectrum – and beyond.

The sensor in the GSENSE2020BSI-H has a peak quantum efficiency of 91%, with a broad peak in the visible spectrum. For near UV and IR applications, it features good sensitivity all the way from 200 nm to 1000 nm.

Chamber Window Coating Options

The GSENSE2020BSI-H sensor is windowless, which provides the optimum sensitivity across the sensor. For windowless sensors we recommend recharging the desiccant plug annually, to avoid any risk of moisture contamination on the sensor.

The fused silica optical window on the sealed sensor chamber is available with two standard coating options, depending on your application. VIS-NIR provides optimal sensitivity from 400 nm through 1000 nm. UV-VIS provides optimal transmission from 250 nm through 700 nm.

StackPro™

The SBIG Aluma AC2020BSI scientific CMOS camera features StackPro™, a revolutionary feature that performs image stacking inside the camera.

CMOS sensors often have more limited well depth and bit depth than their CCD predecessors. At the same time, the modern CMOS sensors have much lower read noise than the equivalent CCD. This low read noise can be used to advantage, by stacking many shorter exposures to achieve the same final result. This does however result in a lot of extra disk usage and post-processing.

StackPro™ performs the stacking automatically, inside the camera. It automatically subdivides your exposure into up to 16 individual subexposures, and stacks them inside the camera prior to download. This eliminates the excessive amounts of data cluttering up your hard drive. Stacking can also be used as an alternative to High Dynamic Range (HDR) mode.

HDR Mode

The sensor in the AC2020BSI is capable of operating in HDR mode, where high-gain and low-gain images are read out simultaneously. Our included MaxIm LT software features an HDR merge feature, which greatly simplifies the process of producing clean, highly linear images.

Superior Cooling

Proven pin heatsink design shared with industry-leading STX series cameras gets the heat out while providing low vibration. Includes SmartCooling™ intelligent thermoelectric cooling and fan operation.

Water Circulation Ready

For high ambient temperature environments, the liquid cooling option improves thermal performance and helps minimize dark current.

User Rechargeable Desiccant

SBIG pioneered including a high-tech user-replaceable cartridge with a ceramic filter and molecular sieve desiccant. Unlike competing cameras, which require factory service when their chamber desiccant eventually saturates out, the user can easily recharge the desiccant. This eliminates the need for costly service – not to mention the associated downtime and shipping costs. This feature is especially important in high-humidity locations.

Electronic and Mechanical Shutters

The GSENSE CMOS sensor has an electronic rolling shutter. In addition, the Aluma AC series cameras include a mechanical shutter to enable convenient dark-frame subtraction for optimal performance and sensitivity. This is essential for remote/robotic operation.

Optional 12 Position Filter Wheel

The SBIG Aluma AC2020BSI is compatible with the new 12 position SBIG AFW-12-50R filter wheel, utilizing 50 mm round filters.

It is also compatible with the 7 position FW7-STX filter wheel, utilizing 50 mm square filters.

Self-Guiding and Adaptive Optics Options Available

The available SBIG StarChaser SC-3 is an excellent low-cost option for integrated autoguiding in front of the filters, and it supports our SBIG AO-X Adaptive Optics accessory.

The AO-X uses a tip-tilt window to quickly and precisely adjust the image position in response to autoguider feedback. With Adaptive Optics there is no backlash, stiction, or lag, and the movements are precise and accurate. This allows the AO-X to not only remove the effects of periodic error, drift, and wind gusts but also reduce the effects of atmospheric seeing. When used with an Aluma AC camera, the AO-X requires the StarChaser SC-3.

For more information please see AO-X.

USB 3.0 Interface

The Aluma AC includes a USB 3.0 interface port for high-speed downloads. For installations where longer cable lengths are required, the port is also compatible with USB 2.0.

I2C AUX Port

The STX cameras have a convenient auxiliary control port (also known as an I2C AUX port), which controls the filter wheel and provides optional external trigger interfaces. Unlike older SBIG models, the AUX port is not used for AO-X control, as this function is now handled by the optional SBIG StarChaser SC-3 off-axis guiding camera.

MaxIm LT Software

All SBIG cameras come with our MaxIm LT software – a $200 value! MaxIm LT is a special version of our venerable MaxIm DL software that provides complete control of your camera, filter wheel, and auto guider, plus advanced image processing capabilities. If you wish you can upgrade to MaxIm DL Pro to get complete observatory integration and even more processing and analysis capabilities.

Included Accessories

All Aluma AC cameras include a deluxe carrying case, universal power supply, Aluma AC power extension cable, USB 3.0 cable, and MaxIm LT software.

Specifications

Exposure	0.001-3600 sec
OS Compatibility	Windows 7, 8, 10 x86/x64, MacOS 10.14 "Mojave" x86 binaries, Ubuntu 18.04 LTS x64, Raspbian Buster armhf, Ubuntu MATE arm64
Full Frame Download	0.1 sec
Weight	3.5 lbs / 1.6 kG
Filter Size	50mm Square
Read Noise (typ)	1.2 e- in 2-CMS Readout Mode, 1.6 e- Regular Mode
Temperature Regulation	Yes
Computer Interface	USB 3.0
Power	12 VDC 8A
Cooling Delta	~ 40 °C typical, water cooling option included
Adaptive Optics Option	AO-X with StarChaser SC-3
A/D Converter	Dual 12 bit with HDR capability
Dark Current e-/p/s	0.16 e-/p/sec @ -20C
Full Well Capacity	55,000 e-
Sensor Size	13.3 mm x 13.3 mm
Imaging / Pixel Array	2048 x 2048
Shutter	Rolling electronic, Mechanical dark shutter
Self-Guiding In Front of Filters	Yes with StarChaser
Pixel Size	6.5 um
Total Pixels	4 million
Filter Wheel Option	FW7-STX
OAG Option	StarChaser
Imaging Sensor	Gpixel GSENSE2020BSI
Chamber Window	VIS-NIR, UV-VIS

Available to order

Optec Temperature Compensating Focuser-S3i

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$2,799.00

Available to order

Atik One 9.0 Cooled CCD Camera + Atik GP + OAG Kit

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$5,899.00

Out of stock

Planewave Electronic Focus Accessory (EFA) Kit

Planewave Electronic Focus Accessory (EFA) Kit

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From $1,730.00

Out of stock

Planewave Adapter to Feather Touch Focuser

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From $440.00

Out of stock

Planewave Counterweight for 1.5″ Shaft

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From $1,040.00

Out of stock

Planewave T-600 Direct-Drive Gimbal Mount

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$124,480.00

The PlaneWave T-600 Direct Drive Gimbal is engineered to meet the rigorous demands of advanced astrophotography, complex astronomical research, SSA/SDA, and FSOC applications. Leveraging cutting-edge technology, this gimbal provides a robust, precise, versatile observational platform suitable for demanding environments.

Core Features of the T-600 Gimbal

High-Torque Direct-Drive Motors

The T-600 Gimbal has high-torque, double-stacked direct-drive motors, ensuring smooth, fast, and virtually silent operation. This feature is critical for tracking celestial objects with minimal vibration and supreme accuracy, accommodating substantial payloads effectively.

High-Resolution Absolute Encoders

With high-resolution absolute encoders on each axis, it offers incredibly precise pointing and tracking capabilities, crucial for capturing sharp, detailed celestial images and conducting rigorous scientific observations.

Zero Backlash and Periodic Error

The design of the T-600 Gimbal eliminates backlash and periodic error, facilitating consistent and reliable tracking that enhances astrophotography and supports precise applications in research and space surveillance.

Advanced Customization Options

The T-600 includes optional contact gasket seals for full weatherization and supports limitless Az rotation, making it adaptable for specific research observational requirements across various environments.

Rugged and Environment-ready

Designed with rugged environments in mind, the gimbal features electronics enclosed within the mount and weatherproof cable pass-throughs, ensuring durability and reliability in light-to-moderate rain and preventing debris entry.

Application-Specific Advantages

Astrophotography

With its robust load capacity and exceptional slew speeds, it allows astrophotographers to reposition heavy equipment quickly and smoothly, capturing breathtaking images of the cosmos with ease and efficiency.

Research

Researchers will find the gimbal’s precise tracking and advanced software ideal for detailed celestial observations and data collection, particularly in demanding environments where equipment adaptability and operational reliability are paramount.

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

Professionals in SSA/SDA will benefit from the T-600 Gimbal’s high-precision tracking and configurable features, which are perfect for monitoring space debris and tracking satellites, ensuring accurate surveillance and data collection in space domain awareness initiatives.

System Performance

Acceleration (Azimuth and Altitude)	Acceleration up to 100°/second² *Depending upon installed payload-induced moment of inertia
Velocity	Up to 100 degrees per second *Depending upon acceleration and distance traveled
Pointing Accuracy	<5-arcsecond RMS* with PointXP Model *Under stable environmental conditions
Pointing Precision	2 arcseconds at sidereal velocity
Open Loop Tracking Accuracy	0.2 arcseconds RMS over 300 second exposure at siderial rate
Open Loop Axis Following Error	<0.15 arcseconds RMS at sidereal rate, <0.3 arcseconds RMS at 1 degree per second* <2 arcseconds RMS at 10 degrees per second* *Dependent on Payload
Internal Servo-Loop (Drive to Motor)	10 kHz cascaded velocity/position controller, PID + Filters
Software Command Round-Trip	5 – 25 msec (depending on application)
System Natural Frequency	20 Hz or greater (for gimbal only)

Mount system

Type	Alt-Azimuth / Equatorial Direct-Drive Mount
Weight	605 lbs
Max. Load Capacity	600 lbs (with payload limited to 100 kg-m² moment per port with center of gravity ≤ 15 inches from mounting surface and an lowest eigenmode frequency of 20 Hz. i.e. dual mounted CDK24 telescopes are compatible)
Dimensions	34” x 20” x 23.5” (H/D/W)
Latitude Range	0 to 90 degrees, Northern and Southern hemispheres
Motor Torque (Azimuth and Altitude)	127 ft-lbs (peak)
Azimuth Axis Range of Motion (Optional)

Cable Management	Through-the-mount cabling
Coudé Path (Optional)	Limits elevation axis range of motion to 180º
Power Requirement	100 to 240 VAC (50-60 Hz), 20 amp service at 120 VAC, 10 amp service at 240 VAC
Operating Temperature Range	-30 C to +50 C
Storage Temperature Range	-50 C to +70 C

Mechanical structure

Gimbal Assembly	Fully CNC machined construction (Surface finish treated with UV resistant coating on all exposed metal surfaces)
Default Weatherization	2-Layer non-contact labrynth sealing at each motion-surface to prevent water (light-to-moderate rain) and debris entry. *Optional rubber seals may be added for further ruggedization.
Azimuth Bearing	4-way loaded radial ball bearings
Altitude Bearing	4-way loaded radial ball bearings
Instrument Mounting	Breadboard plate on both mounting surfaces (see interface document for complete mounting information)
Lifting Points	Present for lifting in “any orientation”

Motion control

Drive Electronics (Azimuth and Altitude)	Elmo Motion Control Systems industrial grade off-the-shelf brushless motor drives
Motors (Azimuth and Altitude)	Each axis includes a double stacked direct-drive 3 phase axial-flux torque motor
Encoders (Azimuth and Altitude)	26-bit absolute encoder ring with readhead
User Interface	PlaneWave Interface 4 (PWI4) Control Software with integrated PointXP mount modeling software by Dave Rowe. Includes ASCOM driver.
Advanced Timing Features (Optional)	Timestamped using GPS Reciever, or PTP/NPT Server <100-microseconds accuracy

Included items

Included Items	Hardware- Six 1/2-13 x 1 1/4″ socket head cap screws to bolt the mount to the pier or wedge; Six 1/2-13 washers; One extended length shoulder bolt for RA axis to EQ wedge alignment
	One 16' USB cable - Too connect the mount to the observatory control computer
	One 120VAC power cable- to provide power to the mount
	Flashdrive - Contains PWI4 software for mount control , instructions for installation, software, and instructions for collimation and spacing the primary to secondary mirror
	3/8 Socket - Used for operating the RA balance leadscrew on the mount
	Gamepad - Used for control of the mount tracking speeds for visual observing

Out of stock

Planewave CDK450Q Observatory System

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$99,310.00

The CDK450 Observatory System from PlaneWave Instruments is a sophisticated solution designed for the serious astrophotographer and dedicated astronomy researcher. This high-end system combines the powerful CDK17 optical tube with the precise L-550 direct-drive mount, creating an exceptional observational platform that excels in a variety of scientific and imaging applications.

Key Features of the CDK450 Observatory System

CDK17 Optical Tube Assembly

Advanced Optical Design: Employs a Corrected Dall-Kirkham optical design, achieving a field free of off-axis coma and astigmatism and a perfectly flat field across a 52 mm image circle, resulting in critically sharp images over the entire viewing area.
High-Quality Construction: Constructed with robust carbon fiber, reducing thermal expansion and enabling quick 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: Incorporates an advanced cooling system with strategically placed fans that ensure rapid thermal stabilization, essential for maintaining consistent, high-quality imaging and minimizing focus shifts caused by temperature changes.

CDK17 f/6.8 OTA

Aperture and Focal Length: Features a 17-inch aperture, a shorter 3454 mm focal length at a faster f/6.8 focal ratio, and a shorter back focus of 262 mm.

L-550 Direct Drive Mount

Direct Drive Motors: Features state-of-the-art direct-drive motors on each axis, providing smooth, fast, and virtually silent movement of the telescope with zero backlash and zero periodic error, perfect for precise tracking and rapid repositioning of celestial objects.
High-Resolution Encoders: Outfitted with high-resolution optical encoders on both axes, offering precise positioning and movement, which is crucial for elite astrophotography and detailed astronomical studies.
Azimuth Dovetail Balance System: Includes a finely adjustable balance system that enhances 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: Capable of 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 CDK450 is a formidable system for astrophotographers, offering unmatched tracking accuracy and image stability, which facilitate capturing spectacular celestial images with detailed resolution and vibrant colors. The L-550 carries a greater payload capacity – perfect for holding a second telescope on the outside hub.

Astronomy Research

Researchers will find the CDK450 invaluable 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 CDK450 provides 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-550 mount in the CDK450 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

Mount Weight	338 lbs (153 kg)
Max. Load Capacity	300 lbs (136 kg)
Latitude Range	0 to 90 degrees, Northern and Southern hemispheres
Cable Management	Equipment cables can be wired through mount

Control system

Control Electronics	PlaneWave Interface dual axis telescope control
User Interface	PlaneWave Interface 4 (PWI4) Control Software with integrated PointXP mount modeling software
Homing Sensors	Home position sensors are included allowing the mount can find its home position on power up.
Slew Rate	20 degrees per second (standard); 50 degrees per second (maximum), both axes
Power Requirement	Accepts 120 to 240 VAC. Supplied with 120 VAC 15A IEC Type B Regulated Power Adapter.

Optical systems

Aperture	17 inch (432 mm)
Focal Length	2939 mm (115.71 inch)
Focal Ratio	f/6.8
Central Obstruction	23.7% by surface area; 48.6% of the primary mirror diameter
Backfocus from Mounting Surface	10.32 inch (262.33 mm)
Backfocus from Racked in Focuser	7.24 inch (184 mm)
Weight	106 lbs (48 kg)
Optimal Field of View	70mm image circle

Motion control

Motor – Azimuth and Altitude	Direct Drive 3 Phase Axial-Flux Torque Motors
Encoder – Azimuth and Altitude	152mm stainless steel encoder ring with reader built into the azimuth and altitude axes. 18,880,000 counts per revolution (0.069 arcsecond resolution).
Motor Torque	Approximately 20 ft-lbs continuous; 50 ft-lbs peak
Drive Electronics	Industrial grade, off-the-shelf brushless motor drives for each axis with custom designed interface card
Telescope Control Software	Uses PWI4. Incorporates PointXP mount modeling software by Dave Rowe. All ASCOM compatible.

System Performance

Pointing Accuracy	<10 arcsecond RMS with PointXP Model
Pointing Precision	2 arcseconds at sidereal velocity
Tracking Accuracy	0.3 arcseconds over a 5-minute period at sidereal velocity
System Natural Frequency	10 Hz or greater

Included Items

Included Items	Heating elements for dew prevention - The heating pads on the primary and secondary mirror require the 600195 Delta-T controller sold separately
	OTA Cover - To protect the primary mirror and inside of the optical tube
	Flash drive - Contains PWI4 software for mount control , instructions for installation, software, and instructions for collimation and spacing the primary to secondary mirror
	Hardware - Six 1/2-13 x 1 1/4″ socket head cap screws to bolt the mount to the pier, or wedge; Six 1/2-13 washers; One extended length shoulder bolt for RA axis to EQ wedge alignment
	One 16′ USB cable - To connect the mount to the observatory control computer
	One 120VAC power cable - To provide power to the mount
	Standard Allen Key set - For tightening bolts used on the mount
	Gamepad - Used for control of the mount tracking speeds for visual observing
	Dovetail Saddle (200919) - The PW wide saddle comes standard with the L-550 mount

Out of stock

Planewave DRL350 Observatory System

(0)

$63,800.00

The DeltaRho 350 Telescope System from PlaneWave Instruments is crafted for elite astronomers and astrophotographers who demand the best. Created with a passion for excellence, the DeltaRho 350 Telescope System brings groundbreaking features to advanced imaging, offering unmatched versatility across a spectrum of scientific and communicative applications. The DeltaRho 350 Telescope System from PlaneWave Instruments features a 350mm wide-field, f/3 aperture. This premium CDK optical tube combines a DeltaRho 350 with a L-350 direct drive mount.

DeltaRho 350 Telescope System’s Key Features

Large Aperture and Fast Focal Ratio

The DeltRho 350 has a 350 mm aperture and an impressively fast f/3 focal ratio. This combination allows significant light-gathering capability and rapid image capture, perfect for detailed SSA/SDA object capture and deep-sky photography.

Advanced Optical Design

Featuring a corrected Cassegrain focus optical system, the DeltaRho 350 ensures top-tier image clarity. Achieve sharp, flat fields across the entire field of view with no curvature, capturing stellar images that require minimal post-processing.

Mechanical Structure

Constructed with a lightweight yet sturdy carbon fiber tube. This Offers enhanced durability and stability while minimizing thermal expansion and maintaining optimal image quality under various environmental conditions.

High-Performance Coatings

Equipped with high-quality mirror coatings that can be customized to meet specific observational requirements. It enhances light transmission and reduces stray light, optimizing the telescope for specialized applications such as SSA/SDA and FSO.

Collimation Software

The DeltaRho 350 is equipped with user-friendly collimation software designed to ensure optimal alignment of optical elements quickly and accurately. This feature is crucial for maintaining the high resolution and sharpness needed for professional-level imaging and research, allowing users to adjust collimation on the fly easily.

Dew Control

Integrated dew control systems in the DeltaRho 350 utilize advanced heater technology to prevent condensation on optical surfaces. This system ensures that dew does not interrupt observations and imaging sessions, providing consistent clarity and performance in various environmental conditions.

Application-Specific Benefits

Astrophotography

The DeltaRho 350’s fast exposures and expansive field view allow astrophotographers to capture breathtaking night sky images with exceptional detail and clarity.

Astronomy Research

With its robust build and advanced optics, the DeltaRho 350 is an excellent tool for universities and research institutions engaged in long-term astronomical studies.

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

The Delta Rho's fast focal ratio and large image circle allow you to take shorter exposures and use larger Sensors. Making it perfect for surveying larger areas of the sky for quicker monitoring and cataloging of space debris and satellites.

Mount Systems

Mount Weight	110 lbs (50 kg)
Max. Load Capacity	100 lbs (45 kg)
Latitude Range	0 to 90 degrees, Northern and Southern hemispheres
Cable Management	Equipment cables can be wired through mount

Control systems

Control Electronics	PlaneWave Interface dual axis telescope control
User Interface	PlaneWave Interface 4 (PWI4) Control Software with integrated PointXP mount modeling software
Homing Sensors	Home position sensors are included allowing the mount can find its home position on power up.
Slew Rate	20 degrees per second (standard); 50 degrees per second (maximum), both axes
Power Requirement	Accepts 120 to 240 VAC. Supplied with 120 VAC 15A IEC Type B Regulated Power Adapter.

Optical Systems

Aperture	350 mm
Focal Length	1050 mm (41.34 in.)
Focal Ratio	f/3
Central Obstruction	56 % by diameter
Backfocus from Mounting Surface	5.6 in. (142.24 mm). This distance includes refraction from filters.
Weight	46 lbs (21 kg)

Motion control

Motor – Azimuth and Altitude	Direct Drive 3 Phase Axial-Flux Torque Motors
Encoder – Azimuth and Altitude	152mm stainless steel encoder ring with reader built into the azimuth and altitude axes. 18,880,000 counts per revolution (0.069 arcsecond resolution).
Motor Torque	Approximately 20 ft-lbs continuous; 50 ft-lbs peak
Drive Electronics	Industrial grade, off-the-shelf brushless motor drives for each axis with custom designed interface card
Telescope Control Software	Uses PWI4. Incorporates PointXP mount modeling software by Dave Rowe. All ASCOM compatible.

System Performance

Pointing Accuracy	<10 arcsecond RMS with PointXP Model
Pointing Precision	2 arcseconds at sidereal velocity
Tracking Accuracy	0.3 arcseconds over a 5-minute period at sidereal velocity
System Natural Frequency	10 Hz or greater

Included items

Included Items	Heating Elements for Dew Prevention - The heating pads on the primary and secondary mirror require the 600195 Delta-T controller sold separately
	OTA Cover - To protect the primary mirror and inside of the optical tube
	Flashdrive - Contains software and instructions for collimation and spacing the primary to secondary mirror

Out of stock

FSSP floating shoulder strap pro

(0)

$142.00

In stock

iOptron HAE29-EC Strain Wave AZ/EQ

(0)

$5,299.00

Introducing the new members of iOptron strain wave gear mount family - AZ/EQ dual mount HAE29 and HAE29EC! These light weight, high payload little titans will deliver an astronomy experience like never before. Imagine a mount head weighing in at 8 lbs with a payload capability 29.7lbs, without needing a cumbersome counterweight or shaft. Applying iOptron’s multi-decade experience creating precision mounts, the HAE29 brings this vision to reality.

Utilizing state of the art strain wave gear technology for the both RA and DEC movement, the HAE29s deliver unparalleled weight to payload efficiency. Its black anodized all metal CNC machined body is not only appealing to the eye, it’s a rugged platform that will perform at the highest level for many years to come. Unique features such as an electronic friction brake and power down memory allow the mount safely stop and resume a GoTo slew or continue tracking even after an abrupt power loss (No need to realign and start from the beginning).

An HAE29 mount can be controlled by a computer, either via ASCOM/Commander for a Windows PC or a third party INDI driver for a MacOS software; a SmartPhone/Tablet via iOptron Commander Lite or an App like SkySafari; or a Raspberry Pi device via INDI driver.

The HAE29EC features a high precision RA axis encoder that delivers incredible tracking accuracy, enough that many will choose to image “sans” guiding.

Features

Advanced strain wave gear system technology
Payload capacity of 13.5 kg (29.7 lbs) with the mount weight of 3.7 kg (8.15 lbs, include dovetail saddle)
CNC machined
Unique friction brake on both RA and DEC to safely stop movement during a planned or unplanned power interruption
360 second gear period
High precision encoder with realtime PEC (RPEC)
Go2Nova® hand controller with ~212,000 object database
iPolar electronic polar scope for easy and accurate polar alignment
Customer cable management system ready
Dual saddle (Vixen and Losmandy-D styles)
Built in zero position search and locator
Power down position and location memory
Integrated ST-4 autoguiding port
Built-in Wi-Fi (via hand controller)
USB port for firmware upgrade and computer control
Carrying case
Two year warranty

Specifications

Mount	Strain Wave Altazimuth/Equatorial Mount
RA gear system	Strain Wave Gear
DEC gear system	Strain Wave Gear
Reduction ratio	RA 480:1, DEC 360:1
Payload w/o CW *	29.7 lbs (13.5 kg)
Mount weight	8.15 lbs (3.7 kg) with dovetail saddle
Payload/Mount weight	3.65
Payload with CW*	40 lbs (18kg)
High precision encoder	Yes (RA)
PEC	Realtime PEC (RPEC)
Period	360 second
Drive motor	Stepper motor
Structure Material	All metal, CNC machined
Exterior finish	Anodized black
Polar Scope	iPolar electronic polar scope (external)
Level indicator	Level bubble
Control system	GOTONOVA/Commander
Hand Controller	Go2Nova® 8409 with ~212,000 objects database
Tracking	Automatic
Maximum slew speed	6º/sec
Power consumption	0.6A(Tracking), 1A(GOTO)
Power	DC12V-5A (5.5/2.5mm DC plug)
AC adapter	100V ~ 240V (included, indoor use only)
Cable management	Ready for DIY
Power off brake	Electronic friction brake
Power-down memory	Yes
Wi-Fi	Built-in
Communication port	Yes (Wi-Fi and USB, via HC)
Autoguide port	Yes (ST-4 compatible)
Firmware upgrade	Yes
Dovetail saddle	Vixen & Losmandy
Tripod	Optional
Counterweight Shaft	SS Φ20X200mm, 3/8"-16 thread (Optional)
Counterweight	10 lbs (4.5kg)(Optional)
Operation temperature	-20ºC ~ 40ºC (hand controller -10ºC ~ 40ºC)
Warranty	Two year limited

* 200mm, with payload center of gravity to the RA rotation axis. Or an OTA size of ~220mm.

Available to order

Pixfra M2 Series Thermal Monocular 15mm

(0)

$899.00

Pixfra Mile 2 Thermal Monocular: creating new pathways for birding and conservation

Thermal imaging is changing the way we observe and count birds in their natural environment - at all times of the day or night, without intrusive lighting or disturbance.

Any birder knows there's often times when birds are hidden from view, either by foliage or the time of day. It becomes even more frustrating when bird counts are needed to estimate population or species locations for conservation efforts and protection and they simply can't be properly seen.

In situations like this, no matter how powerful the binoculars you're using, the birds will remain hidden.

Thermal imaging devices lets you "see" birds via the heat their bodies produce - revealing them in bushes and trees or when there's simply not enough natural light otherwise.

Have a chat to the experts at BINTEL about how new generation devices like the Pixfra Mile 2 can help how you discover new ways to view nature.

Includes:

15mm lens
2.33x-18.64x magnification
View wildlife up to 800m away
8 Hours Battery Life
Share your live views with up to up 4 people nearby
Vanadium oxide uncooled focal plane detector.
Ultra-low power consumption.
Connects to the mobile app through Wi-Fi.
Six colour palettes.
Built-in EMMC (16 GB).
Electronic compass for quick direction identification.
Lightweight and portable.
IP67 rated.

A design wonder
Hidden Power Switch, Non-Slip Silicone Texture, and a Smooth, Continuous Exterior for Unmatched Ergonomics.

Compact size that sits easily in your hand
Truly pocked sized, the PixFra Mile 2 Series monoculars fit the palm of your hand and can be used for extended periods of time without fatigue.

Despite the compact design, the Mile 2 also produces 640x512 resolution images on your devices.

Logical, Easy to Use Button Layout
Perfect for night-time use or low light conditions, the control button layout is thoughtfully laid out and can be easily used one-handed without a second thought .

Main Features

Thermal
Thermal Detector Type	Vanadium oxide uncooled focal plane detector
Effective Pixels	256 (H) × 192 (V)
Pixel Pitch	12 μm
Spectral Range	8 μm–14 μm
Sensitivity (NETD)	≤35 mK@f/1.0, 25 °C
Focal Length	15mm
Aperture	2.6m
Detection Distance	800m
Magnification	2.33x
Frame Rate	50 Hz
Display
Screen	800 × 600, 0.32 inch, OLED
Colour Palettes	6 (white hot/black hot/iron red/alarm/emerald/amber)
Video Compression	–3 D to +1 D
Eye Relief	13mm
Exit Pupil	5mm
Functions
Digital Zoom	1×, 2×, 4×, 8×
Video Recorder	Yes
Snapshot	Yes
Wi-Fi Hotspot	Yes
Hot Spot Track	Yes
Video Distance Measurement	Yes
FFC Calibration	Auto, Manual, External Correction
Standby Mode	Yes
DPC (Defective Pixel Correction)	Yes
Storage Built-in	16 Gb
Power
Battery Type	Rechargeable Lithium battery
Battery Life	Battery Life 8.5 hrs @25 °C
Power Supply	5 VDC/2A
Port	USB Type-C
Overvoltage Protection	Yes
General
Operating Temperature	–30 °C to +55 °C
Operating Humidity	≤95%
Packaging Dimensions	180.0 mm × 123.0 mm × 96.0 mm
Product Dimensions	149.0 mm × 56.6 mm × 50.3 mm (
Gross Weight	760g
Net Weight	270g

Available to order

LEICA GEOVID R SE 8x42

(0)

$2,550.00

Available to order

Nexcope NIB620 Inverted Laboratory Phase Contrast Microscope

(0)

$8,999.00

Nexcope NIB620 Inverted Laboratory Phase Contrast Microscope

The Nexcope NIB620 Inverted Laboratory Phase Contrast Microscope is a high-performance imaging solution designed for advanced applications in life sciences, cell culture, and research. Its robust design, advanced optical features, and user-friendly operation make it an essential tool for professionals in clinical and laboratory settings.

Key Features:

Optical Excellence: Equipped with high-quality infinity-corrected optical systems, including phase contrast objectives, the NIB620 ensures sharp, clear images with enhanced contrast.
Magnification Range: Offers a magnification range of 40x to 400x with 10x eyepieces and Plan Phase objectives (10x, 20x, 40x) and an infinity Plan 4x objective.
Eyepieces: Widefield 10x/22mm eyepieces for a broad and comfortable field of view.
Illumination: Powerful LED illumination with adjustable brightness for even lighting and reduced eye strain.
Stage: Spacious 250mm x 170mm mechanical stage with smooth X/Y control and a 110mm x 74mm movement range.
Condenser: Long working distance condenser with phase sliders for optimized light control during observation.
Ergonomic Design: Features a comfortable viewing angle and intuitive controls for prolonged use in lab settings.
Camera Compatibility: Includes a trinocular port for digital imaging, making it ideal for documentation and image analysis.

Applications:

Cell Culture Studies: Perfect for analyzing live cells and monitoring cell cultures in life science research.
Clinical Diagnostics: Ideal for laboratory research in microbiology, pathology, and cytology.
Educational Use: Suitable for teaching advanced microscopy techniques in universities and research institutions.

The Nexcope NIB620 Inverted Laboratory Phase Contrast Microscope combines high-quality optics, ergonomic design, and advanced features to deliver precision and reliability for demanding applications.

Warranty Information	3-Years Limited Warranty
Eyepiece	Extra Wide Field 10x/ 22mm
Magnification Range	10x, 40x, 200x, 400x
Objectives	Infinity Plan 4x, Phrase Contrast 10x, 20x, 40x
Field of View	22mm
Working Distance	75mm
Illumination	LED
Head Type	Inverted Binoculars
Focus	Coarse and Fine, Coaxial
Condenser	NA 0.3, WD 75
Stage Type	Fixed with Attached Mechnical Slide Holder (250 x 170mm)
Stand	Inverted
Power Supply	250v 10A Power cord

Available to order

Nexcope NE620 Trinocular Professional Microscope 40x-1000x

(0)

$3,899.00

Nexcope NE620 Trinocular Professional Microscope 40x-1000x

The Nexcope NE620 Trinocular Professional Microscope is a premium optical instrument designed for advanced research and professional applications. Combining precision engineering with user-friendly features, the NE620 delivers exceptional image clarity and versatility, making it an excellent choice for a variety of fields, including biology, materials science, and industrial research.

Key Features:

Optics: High-contrast NIS infinity plan objectives for outstanding resolution and image quality.
Magnification: Wide range of magnifications for detailed observation.
Viewing Comfort: Ergonomically designed viewing head for prolonged usage without discomfort.
Condenser: Multifunctional condensers support bright field, dark field, and phase contrast observation methods. (Dark field, and phase contrast slider to be purchased separately)
Illumination: Intelligent brightness control with even, bright illumination to ensure optimal viewing conditions.

Applications:

Biological Research: Ideal for cellular studies, tissue examination, and live cell imaging.
Industrial Inspection: Suitable for material analysis, quality control, and failure diagnostics.
Educational Use: Perfect for advanced teaching in universities and research institutions.

The Nexcope NE620 microscope combines innovative design, superior optics, and versatility, making it a reliable and high-performing solution for professionals and researchers.

Warranty Information	3-Years Limited Warranty
Eyepiece	Extra Wide Field 10x/ 22mm
Magnification Range	40x, 100x, 400x, 1000x
Objectives	NIS Inifnite Plan Achromatic 4x, 10x, 40x, 100x (Oil)
Field of View	22mm
Working Distance	28mm
Illumination	3W LED
Head Type	Trinocular
Focus	Coarse and Fine, Coaxial
Condenser	NA 1.25
Stage Type	Fixed with Attached Mechnical Slide Holder (185 x 142mm)
Stand	Curved Arm
Power Supply	250v 10A Power cord

Available to order

Saxon SmartOne Biological Microscope 40x-1600x

(0)

$649.00

saxon SmartOne Biological Microscope 40x-1600x

The SmartOne Biological Microscope is a reliable and versatile equipment for educational, home schooling, and hobby applications. With its impressive magnification range and precision engineering, this microscope offers exceptional clarity and functionality for various biological studies.

Key Features:

Magnification: 40x, 64x, 100x, 160x, 400x, 640x, 1000x,1600x
Binocular Viewing Head: Provides a comfortable, ergonomic experience during prolonged use.
Eyepieces: Includes 10x and 16x wide-field eyepieces for enhanced viewing flexibility.
Quadruple Nosepiece: Smoothly rotating nosepiece to easily switch between objectives.
Achromatic Objectives: 4x, 10x, 40x, and 100x oil immersion for sharp, high-contrast images.
Stage: Precision mechanical stage measuring 110x125mm for smooth sample positioning.
Condenser: NA 1.25 Abbe condenser with an iris diaphragm for optimal light control.
Coarse & Fine Focusing: Ensures detailed observation.
Illumination: Bright and even LED illumination for detailed observation.

Applications:

Education: Ideal for home schooling, schools, and universities for teaching cellular biology and microbiology.
Research: Suitable for biological, medical, and environmental studies requiring high precision.

The saxon SmartOne Biological Microscope combines quality optics, a robust design, and ease of use, making it an excellent choice for both professionals and enthusiasts.

Warranty Information	3-Years Limited Warranty
Eyepiece	WF 10x/18mm, WF 16x
Magnification Range	40x, 64x, 100x, 160x, 400x, 640x, 1000x, 1600x
Objectives	4x, 10x, 40xR, 100xR
Field of View	18mm
Working Distance	4x @ 37.5mm, 10x @ 6.5mm, 40x @ 0.63mm, 100x @ 0.195mm
Illumination	LED
Head Type	Binoculars
Focus	Coarse and Fine, Coaxial
Condenser	1.25 Abbe
Stage Type	Fixed with Attached Mechanical Slide Holder (115 x 125mm)
Stand	Arm
Power Supply	250v 10A Power cord
Weight	4kgs
Shipping Dimensions	41 x 34 x 26 cm3
Shipping Weight	5.2kgs

Available to order

Planewave IRDK 14 OTA

(0)

$39,000.00

The IRDK14 from PlaneWave Instruments is a precisely engineered optical system designed for high performance in infrared wavelengths. It is an excellent tool for advanced astronomical research and remote sensing applications, offering superior performance for infrared imaging.

IRDK14’s Key Features

Large Aperture and Optimized Focal Ratio

The IRDK14 features a 356 mm aperture and an f/7.2 focal ratio, enhancing its capacity to gather infrared light effectively. This setup is ideal for detailed infrared observations and long-exposure imaging, providing exceptional light-gathering capabilities.

Specialized Optical Design for Infrared

The Dall-Kirkham optical design of the IRDK14 is optimized for infrared wavelengths. There are no refractive lenses, only reflective fused silica mirrors. The reflective coatings are a protected gold with better than 98% reflectivity from .65 microns (650nm) to 5 microns (5000nm), making it well-suited for infrared astronomy or LIDAR applications. UV-optimized coatings can also be provided, and potential customers are encouraged to contact our technical sales team to discuss UV optimization.

Robust Mechanical Structure

Constructed using carbon fiber, the optical tube of the IRDK14 offers durability and stability with minimal thermal expansion. This design ensures consistent performance under various environmental conditions, making it suitable for intensive scientific applications.

Advanced Thermal Management

The IRDK14 includes cooling fans and a system prepared for Delta-T applications, promoting rapid thermal equilibrium. This feature is critical for minimizing air turbulence within the tube, thus reducing potential image distortion and enhancing overall imaging quality.

Integrated Dew Control

Infrared observations are prone to condensation, but the IRDK14 tackles this with advanced dew prevention technology. Heater pads, controlled via PlaneWave’s software, ensure the optical surfaces stay clear from dew, maintaining consistent and clear imaging performance.

Application-Specific Benefits

Infrared Astronomy

The IRDK14 excels in infrared astronomy, where its significant aperture and infrared-optimized optics allow for precise 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 IRDK14 is a robust platform for advanced scientific research, including LIDAR and other remote sensing applications.

Key Features Overview

The IRDK14 comes with impressive specifications tailored for infrared optimization:

Gold-coated mirrors optimized for high reflectivity in infrared wavelengths (ultraviolet optimization available)
14-inch (356 mm) aperture
2563 mm focal length
f/7.2 focal ratio
282mm back focus from mounting surface
70mm image circle
Rock-solid fused silica mirrors with low thermal expansion
Lightweight and rigid carbon fiber optical tube assembly

Optical Systems

Aperture	356mm (14 in)
Focal Length	2563mm (101 in)
Focal Ratio	F/7.2
Central Obstruction	23.5% by Surface Area: 48.5% by Diameter
Back Focus From Mounting Surface	282mm (11.09 in)
Weight	22kg (48lbs)
OTA Length	889mm (35 in)
Upper Cage	Carbon Fiber Truss
Lower Cage	Carbon Fiber Truss And Light Shroud

Secondary Mirror

Diameter	165mm (6.5 in)
Material	Fused Silica (Quartz)
Shape	Spherical
Coating	Protected Gold

Primary Mirror

Optical Diameter	355.6mm (14 in)
Outer Diameter	468.3mm (14.5 in)
Shape	Prolated Ellipsoid
Material	Fused Silica (Quartz)

Included Items	Heating Elements for Dew Prevention - The heating pads on the primary and secondary mirror require the 600195 Delta-T controller sold separately
	OTA Cover - To protect the primary mirror and inside of the optical tube
	Flashdrive - Contains software and instructions for collimation and spacing the primary to secondary mirror
	Wrench Set (5812A35) - Standard hex wrenches (European orders only)

Out of stock

Swarovski STX 30-70 x 115 Spotting Scope

(0)

$7,930.00

Clarity right up to the edge - SWAROVISION Field Flattener

This type of image definition has never been achieved before in any other spotting scope, thanks to the field flattener lenses creating a virtually flat image. Even the finest structures are reproduced with razor-sharp clarity right up to the edge with no need for constant refocusing.

The result: every detail is instantly captured, producing a perfect image without any distortions.

Maximum contrast - Including HD optics

A highly innovative optics design combined with fluoride- containing HD lenses minimise interfering colour fringing. This enables maximum
colour fidelity and leads to a significant improvement in resolution and contrast.

The result: an even more lifelike, contrast-rich image.

A complete view - Large field of view and high zoom range

Nothing escapes you. Thanks to their wide field of view, the ATX/STX spotting scopes provide you with a broader, more exciting platform for your viewing experience.

In spite of their high zoom range, the new generation of spotting scopes offers a large field of view. This allows you to achieve optimum magnification and detail recognition and also makes it extremely easy for you to search for and find objects, especially if they are in motion.

Eye relief plus - Large field of view even for spectacle wearers

SWAROVISION features a long eye relief and the removable twist-in eyecup is individually adjustable.

The result: even spectacle wearers can enjoy a large field of view, not to mention the inimitable edge sharpness. An additional eyecup has been specially developed for spectacle wearers to further increase viewing comfort.

Maximum colour fidelity - Optimised coatings

The enhanced lens and prism coatings (SWARODUR & SWAROTOP) give noticeably better colour reproduction combined with even greater transmission. SWAROCLEAN coatings on the outer lens surfaces create a non-stick effect, making it easier to clean.

The result: even more impressive observing experiences, even in low light.

Ingenious System

The new modular design offers previously unimagined flexibility and you are free to choose the perfect solution as the situation dictates. In collaboration with experts we have developed digiscoping adapters that open up a new realm of ways in which to observe and share the most beautiful moments.

Perfectly designed down to the smallest detail making you equipped for any situation.

Just one hand

When every second counts. Imagine a plover flitting over the shore one minute and taking off into the sky the next. The ATX/STX spotting scopes ensure that you are prepared for moments like this. This is because the new position of the zoom ring, which is now directly behind the focusing ring, makes it easier to handle. It means that you can zoom and focus with one hand, while steering the spotting scopes direction with the other.

This completely new ergonomic design offers a crucial benefit for digiscopers in particular. They can now use the camera quickly, easily and accurately with one hand, while the other concentrates on zoom and focus.

Easy to transport

Not a gram too heavy for top optical performance. Size and weight is the name of the game for all those who like to travel or spend long days in the field. The ATX/STX series means that bulky spotting scopes that are difficult to pack and heavy to carry are a thing of the past.

The modular design enables you to store the objective and eyepiece modules separately and the smaller dimensions also mean that you can easily and safely store individual modules in your luggage.

Available to order

Swarovski STX 30-70 x 95 Spotting Scope

(0)

$6,650.00

Clarity right up to the edge - SWAROVISION Field Flattener

This type of image definition has never been achieved before in any other spotting scope, thanks to the field flattener lenses creating a virtually flat image. Even the finest structures are reproduced with razor-sharp clarity right up to the edge with no need for constant refocusing.

The result: every detail is instantly captured, producing a perfect image without any distortions.

Maximum contrast - Including HD optics

A highly innovative optics design combined with fluoride- containing HD lenses minimise interfering colour fringing. This enables maximum
colour fidelity and leads to a significant improvement in resolution and contrast.

The result: an even more lifelike, contrast-rich image.

A complete view - Large field of view and high zoom range

Nothing escapes you. Thanks to their wide field of view, the ATX/STX spotting scopes provide you with a broader, more exciting platform for your viewing experience.

In spite of their high zoom range, the new generation of spotting scopes offers a large field of view. This allows you to achieve optimum magnification and detail recognition and also makes it extremely easy for you to search for and find objects, especially if they are in motion.

Eye relief plus - Large field of view even for spectacle wearers

SWAROVISION features a long eye relief and the removable twist-in eyecup is individually adjustable.

The result: even spectacle wearers can enjoy a large field of view, not to mention the inimitable edge sharpness. An additional eyecup has been specially developed for spectacle wearers to further increase viewing comfort.

Maximum colour fidelity - Optimised coatings

The enhanced lens and prism coatings (SWARODUR & SWAROTOP) give noticeably better colour reproduction combined with even greater transmission. SWAROCLEAN coatings on the outer lens surfaces create a non-stick effect, making it easier to clean.

The result: even more impressive observing experiences, even in low light.

Ingenious System

The new modular design offers previously unimagined flexibility and you are free to choose the perfect solution as the situation dictates. In collaboration with experts we have developed digiscoping adapters that open up a new realm of ways in which to observe and share the most beautiful moments.

Perfectly designed down to the smallest detail making you equipped for any situation.

Just one hand

When every second counts. Imagine a plover flitting over the shore one minute and taking off into the sky the next. The ATX/STX spotting scopes ensure that you are prepared for moments like this. This is because the new position of the zoom ring, which is now directly behind the focusing ring, makes it easier to handle. It means that you can zoom and focus with one hand, while steering the spotting scopes direction with the other.

This completely new ergonomic design offers a crucial benefit for digiscopers in particular. They can now use the camera quickly, easily and accurately with one hand, while the other concentrates on zoom and focus.

Easy to transport

Not a gram too heavy for top optical performance. Size and weight is the name of the game for all those who like to travel or spend long days in the field. The ATX/STX series means that bulky spotting scopes that are difficult to pack and heavy to carry are a thing of the past.

The modular design enables you to store the objective and eyepiece modules separately and the smaller dimensions also mean that you can easily and safely store individual modules in your luggage.

Available to order

Swarovski STX 25-60 x 65 Spotting Scope

(0)

$4,950.00

Clarity right up to the edge - SWAROVISION Field Flattener

This type of image definition has never been achieved before in any other spotting scope, thanks to the field flattener lenses creating a virtually flat image. Even the finest structures are reproduced with razor-sharp clarity right up to the edge with no need for constant refocusing.

The result: every detail is instantly captured, producing a perfect image without any distortions.

Maximum contrast - Including HD optics

A highly innovative optics design combined with fluoride- containing HD lenses minimise interfering colour fringing. This enables maximum
colour fidelity and leads to a significant improvement in resolution and contrast.

The result: an even more lifelike, contrast-rich image.

A complete view - Large field of view and high zoom range

Nothing escapes you. Thanks to their wide field of view, the ATX/STX spotting scopes provide you with a broader, more exciting platform for your viewing experience.

In spite of their high zoom range, the new generation of spotting scopes offers a large field of view. This allows you to achieve optimum magnification and detail recognition and also makes it extremely easy for you to search for and find objects, especially if they are in motion.

Eye relief plus - Large field of view even for spectacle wearers

SWAROVISION features a long eye relief and the removable twist-in eyecup is individually adjustable.

The result: even spectacle wearers can enjoy a large field of view, not to mention the inimitable edge sharpness. An additional eyecup has been specially developed for spectacle wearers to further increase viewing comfort.

Maximum colour fidelity - Optimised coatings

The enhanced lens and prism coatings (SWARODUR & SWAROTOP) give noticeably better colour reproduction combined with even greater transmission. SWAROCLEAN coatings on the outer lens surfaces create a non-stick effect, making it easier to clean.

The result: even more impressive observing experiences, even in low light.

Ingenious System

The new modular design offers previously unimagined flexibility and you are free to choose the perfect solution as the situation dictates. In collaboration with experts we have developed digiscoping adapters that open up a new realm of ways in which to observe and share the most beautiful moments.

Perfectly designed down to the smallest detail making you equipped for any situation.

Just one hand

When every second counts. Imagine a plover flitting over the shore one minute and taking off into the sky the next. The ATX/STX spotting scopes ensure that you are prepared for moments like this. This is because the new position of the zoom ring, which is now directly behind the focusing ring, makes it easier to handle. It means that you can zoom and focus with one hand, while steering the spotting scopes direction with the other.

This completely new ergonomic design offers a crucial benefit for digiscopers in particular. They can now use the camera quickly, easily and accurately with one hand, while the other concentrates on zoom and focus.

Easy to transport

Not a gram too heavy for top optical performance. Size and weight is the name of the game for all those who like to travel or spend long days in the field. The ATX/STX series means that bulky spotting scopes that are difficult to pack and heavy to carry are a thing of the past.

The modular design enables you to store the objective and eyepiece modules separately and the smaller dimensions also mean that you can easily and safely store individual modules in your luggage.

Available to order

CHROMA TECHNOLOGY Sii (8nm) Filter

(0)

From $520.00

Available to order

CHROMA TECHNOLOGY Sii (5nm) Filter

(0)

From $840.00

Available to order

Chroma Technology H-BETA (5nm) Filter

(0)

From $840.00

Available to order

Chroma Technology H-BETA (3nm) Filter

(0)

From $1,040.00

Available to order

Paramount Large Dovetail Rails

(0)

$1,799.00

Available to order

iOptron HAE29 Strain Wave AZ/EQ With iPolar

(0)

$3,670.00

Introducing the new members of iOptron strain wave gear mount family - AZ/EQ dual mount HAE29 and HAE29EC! These light weight, high payload little titans will deliver an astronomy experience like never before. Imagine a mount head weighing in at 8 lbs with a payload capability 29.7lbs, without needing a cumbersome counterweight or shaft. Applying iOptron’s multi-decade experience creating precision mounts, the HAE29 brings this vision to reality.

Utilizing state of the art strain wave gear technology for the both RA and DEC movement, the HAE29s deliver unparalleled weight to payload efficiency. Its black anodized all metal CNC machined body is not only appealing to the eye, it’s a rugged platform that will perform at the highest level for many years to come. Unique features such as an electronic friction brake and power down memory allow the mount safely stop and resume a GoTo slew or continue tracking even after an abrupt power loss (No need to realign and start from the beginning).

An HAE29 mount can be controlled by a computer, either via ASCOM/Commander for a Windows PC or a third party INDI driver for a MacOS software; a SmartPhone/Tablet via iOptron Commander Lite or an App like SkySafari; or a Raspberry Pi device via INDI driver.

Features

Advanced strain wave gear system technology
Payload capacity of 13.5 kg (29.7 lbs) with the mount weight of 3.7 kg (8.15 lbs, include dovetail saddle)
CNC machined
Unique friction brake on both RA and DEC to safely stop movement during a planned or unplanned power interruption
360 second gear period
Go2Nova® hand controller with ~212,000 object database
iPolar electronic polar scope for easy and accurate polar alignment
Customer cable management system ready
Dual saddle (Vixen and Losmandy-D styles)
Built in zero position search and locator
Power down position and location memory
Integrated ST-4 autoguiding port
Built-in Wi-Fi (via hand controller)
USB port for firmware upgrade and computer control
Carrying case
Two year warranty

Specifications

Mount	Strain Wave Altazimuth/Equatorial Mount
RA gear system	Strain Wave Gear
DEC gear system	Strain Wave Gear
Reduction ratio	RA 480:1, DEC 360:1
Payload w/o CW *	29.7 lbs (13.5 kg)
Mount weight	8.15 lbs (3.7 kg) with dovetail saddle
Payload/Mount weight	3.65
Payload with CW*	40 lbs (18kg)
Period	360 second
Drive motor	Stepper motor
Structure Material	All metal, CNC machined
Exterior finish	Anodized black
Polar Scope	iPolar electronic polar scope (external)
Level indicator	Level bubble
Control system	GOTONOVA/Commander
Hand Controller	Go2Nova® 8409 with ~212,000 objects database
Tracking	Automatic
Maximum slew speed	6º/sec
Power consumption	0.6A(Tracking), 1A(GOTO)
Power	DC12V-5A (5.5/2.5mm DC plug)
AC adapter	100V ~ 240V (included, indoor use only)
Cable management	Ready for DIY
Power off brake	Electronic friction brake
Power-down memory	Yes
Wi-Fi	Built-in
Communication port	Yes (Wi-Fi and USB, via HC)
Autoguide port	Yes (ST-4 compatible)
Firmware upgrade	Yes
Dovetail saddle	Vixen & Losmandy
Tripod	Optional
Counterweight Shaft	SS Φ20X200mm, 3/8"-16 thread (Optional)
Counterweight	10 lbs (4.5kg)(Optional)
Operation temperature	-20ºC ~ 40ºC (hand controller -10ºC ~ 40ºC)
Warranty	Two year limited

Available to order

iOptron HAE43 Strain Wave AZ/EQ with iPolar

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$5,020.00

Introducing the new members of iOptron strain wave gear mount family - AZ/EQ dual mount HAE43 and HAE43EC! These light weight, compact, medium payload titans will deliver an astronomy experience like never before. Imagine a mount head weighing in at less than 13lbs with a payload capability 44lbs, without needing a cumbersome counterweight or shaft. Applying iOptron’s multi-decade experience creating precision mounts, the HAE43 brings this vision to reality.

Utilizing state of the art strain wave gear technology for the both RA and DEC movement, the HAE43s deliver unparalleled weight to payload efficiency. Its black anodized all metal CNC machined body is not only appealing to the eye, it’s a rugged platform that will perform at the highest level for many years to come. Unique features such as an electronic friction brake and power down memory allow the mount safely stop and resume a GoTo slew or continue tracking even after an abrupt power loss (No need to realign and start from the beginning).

An HAE43 mount can be controlled by a computer, either via ASCOM/Commander for a Windows PC or a third party INDI driver for a MacOS software; a SmartPhone/Tablet via iOptron Commander Lite or an App like SkySafari; or a Raspberry Pi device via INDI driver.

Features

Advanced strain wave gear system technology
Payload capacity of 20 kg (44 lbs) with the mount weight of 5.8 kg (12.8 lbs, include dovetail saddle)
CNC machined
Unique friction brake on both RA and DEC to safely stop movement during a planned or unplanned power interruption
270 second gear period
Go2Nova® hand controller with ~212,000 object database
iPolar electronic polar scope for easy and accurate polar alignment
Customer cable management system ready
Dual saddle (Vixen and Losmandy-D styles)
Built in zero position search and locator
Power down position and location memory
Integrated ST-4 autoguiding port
Built-in Wi-Fi (via hand controller)
USB port for firmware upgrade and computer control
Aluminum carrying case
Two year warranty

Mount	Strain Wave Altazimuth/Equatorial Mount
RA gear system	Strain Wave Gear
DEC gear system	Strain Wave Gear
Reduction ratio	RA 640:1, DEC 480:1
Payload w/o CW *	44 lbs (20 kg)
Mount weight	12.8lbs (5.8kg) with dovetail saddle
Payload/Mount weight	3.45
Payload with CW*	55 lbs (25kg)
Period	270 second
Drive motor	Stepper motor
Structure Material	All metal, CNC machined
Exterior finish	Anodized black
Polar Scope	iPolar electronic polar scope (external)
Level indicator	Level bubble
Control system	GOTONOVA/Commander
Hand Controller	Go2Nova® 8409 with ~212,000 objects database
Tracking	Automatic
Maximum slew speed	6º/sec
Power consumption	0.7A(Tracking), 1.2A(GOTO)
Power	DC12V-5A (5.5/2.5mm DC plug)
AC adapter	100V ~ 240V (included, indoor use only)
Cable management	Ready for DIY
Power off brake	Electronic friction brake
Power-down memory	Yes
Wi-Fi	Built-in
Communication port	Yes (Wi-Fi and USB, via HC)
Autoguide port	Yes (ST-4 compatible)
Firmware upgrade	Yes
Dovetail saddle	Vixen & Losmandy
Tripod	Optional
Counterweight Shaft	SS Φ20X200mm, 3/8"-16 thread (Optional)
Counterweight	10 lbs (4.5kg)(Optional)
Operation temperature	-20ºC ~ 40ºC (hand controller -10ºC ~ 40ºC)
Warranty	Two year limited

* 200mm, with payload center of gravity to the RA rotation axis. Or an OTA size of ~220mm.

Available to order

Optical Design	Newtonian (Parabolic)
Diameter/Aperure	130mm
Focal Length	650mm
Focal Ratio	f/5
Finder Scope	6x30mm
Eyepiece	LET 28mm 2"
Focuser	2" Crayford 10:1 Dual Speed

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