GIOTTO 560 Smart Flat Field Generator (PrimaLuceLab, SKU: PLLGIOTTO560) PrimaLuceLab opinie

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GIOTTO 560 Smart Flat Field Generator (PrimaLuceLab, SKU: PLLGIOTTO560 ) is the largest in the family of intelligent calibration panels, designed for telescopes with an aperture of up to 560 mm . The use of many white LEDs with a color similar to sunlight and a special diffuser guarantees uniform field illumination even for large instruments. The built-in electronics allow for brightness adjustment in 100 steps (0 - 100 %), and operation is provided by a USB-C connector, built-in Wi-Fi (Virtual HandPad) and a 12 V DC power socket. After adding the optional ALTO engine, the panel can act as a remote-controlled telescope cover.

Key Features of GIOTTO 560

• maximum diameter of the illuminated field: 560 mm – for telescopes with an aperture of ≤ 560 mm
• LEDs with a color close to 5500 K - neutral white balance of flat frames
• a special diffuser ensuring uniform lighting of the entire surface
• brightness adjustment in 100 steps (0 - 100%) from PLAY, ASCOM or Virtual HandPad
• integrated controller: USB-C port, 2.4 GHz Wi-Fi, 12 V DC power socket (2.5 A)
• cooperation with PLAY software (Windows) and ASCOM driver
• possibility of expansion with ALTO-3L cover motor – remote opening and closing of the telescope
• panel weight: 4.0 kg

Set components

• GIOTTO 560 Smart Flat Field Generator calibration panel
• 12V DC power cord
• USB-C → USB-A cable
• quick start guide

Technical parameters

• Diameter of illuminated field: 560 mm
• brightness adjustment: 0 – 100% (100 steps)
• LED color temperature: ≈ 5500 K
• interfaces: USB-C, Wi-Fi 2.4 GHz
• power supply: 12 V DC / ≤ 2.5 A (5.5 × 2.5 mm socket, + in the center)
• weight: 4.0 kg
• ALTO compatibility: 3L model
• manufacturer: PrimaLuceLab – Italy

With GIOTTO 560 you can make perfect flat frames even for very large reflector telescopes. Remote control via USB or Wi-Fi makes it easy to automate calibration, and the optional ALTO engine turns the panel into a robotic cover, increasing the convenience of work in observatories and remote sets.