The small ToupTek 678M offers optimal performance for planetary imaging and driving. Low readout noise, high dynamic range, peak QE >83%, AR protection window and much more!
This camera weighs only 90g and has a 31.8mm barrel! 3840x2160 pixels while the pixel size is 2 μm.

• 16- times magnification in a compact format
• Vibration correction on land, water and in the air
• Automatic switch-off function after 10 minutes
• Sharp and high-contrast image
• Comfortable and lightweight construction
• Precise focusing ring for fast interaction

The new TECHNO STABI 12X28 Compact Binoculars provide outstanding performance while combining high power, stabilization and exceptional views with durability, all in a compact body.

FUJINON TECHNO STABI 12X28 Key Features:

• Equipped with vibration canceler; vibration correction range of ±3° delivers stable images with 12x magnification.
• Fully multi-coated optics and phase-coated prisms provide sharp, high contrast images and bright view.
• Battery can run for up to 12 hours; auto off function turns power off after 10 minutes 
• Precise center focus wheel for easily bringing details into sharp focus
• Made of fiberglass-reinforced, high durability plastic 
• Lightweight, compact and ergonomic weighing only 0.93lb

5/8 λ ground plane omnidirectional 26 to 28 MHz Tunable Antenna. Height (approx): 6700 mm / 21.98 ft.
Additional nylon ring to reduce the wind noise of the radials included.

There’s no need to introduce this classic of CB marine communication. This antenna has become a standard for professionals, thanks to an excellent quality and an outstanding reliability. The special paint with anti-UV filter avoids the deterioration of the colouring and keeps the whip shining white.

The new vinyl plastic cap, navy blue, provides a quality, finished appearance to the antenna and it’s extremely resistant to high temperatures. 100% WATERPROOF

• 100% WATERPROOF Antenna
• Anti – UV high gloss finish
• 5 m coaxial cable RG 58 CU MIL

Using a new large aperture lens and CMOS, under the same ambient brightness, the exposure time of the OCAL3.0 electronic collimator is only 1/20 of that of the second-generation electronic collimator. If the light source is too strong, it is recommended to reduce the gain rather than simply reducing the exposure time. Now, new collimators can adjust the telescope's collimation in darker environments.

The clarity of the OCAL3.0 electronic collimator image has been greatly improved. Now you can see clearer primary mirror marks and more reflection information, and it still performs well when equipped with a correction mirror. 

Controller bracket for use with MBF-1

The MBA-5 bracket is for the control head of the IC-2730E. The MBA-5 does have holes for direct mounting to a surface. Alternatively, the MBA-5 can be held by the MBF-1 base.

Please note that the MBF-1 suction mounting base is sold separately.

Compact Desktop 36A|13.8V Power Supply sets the new standard for high quality.

• Safety: The Intelligent Protection System protects your devices from damage
• Quiet Operation: The low EMI and acoustic noise minimize distractions
• Flexibility: The flexible orientation and multiple connectivity options make it easy to use
• Convenience: The touchscreen display and USB interface make it easy to control and monitor the power supply
• Power: The 500 watts continuous power output is enough for demanding tasks
• Durability: The sleek design and sturdy construction make it a reliable investment

D-Star dual band 144/430 MHz Analog/Digital Transceiver.
Following in the footsteps of the previous TH-D74 model, the TH-D75E adds many useful features such as simultaneous reception of 2 D-STAR frequencies, Terminal Reflector mode to access the D-STAR Reflectors, improved voice guidance and a Standalone APRS digipeater function . Usability has been improved with the adoption of a USB Type-C socket, PTT support for Bluetooth headphones and a fully ergonomic design. These long-awaited new functions make this super-evolved version the definitive solution to the needs of a wide range of radio amateurs.