This camera adaptor is designed to connect SBIG STL-11000 CCD cameras to a TMB-designed FLT field flattener. It provides a secure and precise interface, ensuring proper alignment and stable performance for astrophotography setups. Made from durable aluminium, the adaptor offers long-lasting reliability and a professional black finish.

A field flattener is a lens designed to correct the natural field curvature produced by primary telescope optics. This curvature can make stars at the edge of an image appear less sharp. By using a flattener, also known as a field flattener, this effect is corrected, resulting in astrophotography images where stars are sharp all the way to the edge. The flattener is positioned between the telescope and the camera.

A field flattener is a lens that corrects the natural field curvature created by a telescope's primary optics. Without this correction, stars near the edge of your image may appear less sharp. The flattener is placed between the telescope and the camera, allowing astrophotographers to capture images with consistently sharp stars across the entire field. This particular field flattener is specially designed for the William Optics Fluorostar FLT 91. 

This guidescope is designed to be mounted parallel to your main telescope tube, ideally using guide scope rings for easy adjustment and alignment. A compatible camera can be attached to the end of the guidescope to control the mount's tracking, enabling accurate long-exposure night sky photography. Cameras suitable for guiding typically use a 1.25" socket, allowing for a straightforward connection to the guidescope.

This guidescope is mounted parallel to the main telescope tube, ideally using guide scope rings for easy positioning and adjustment. You can attach a compatible camera to the end of the guidescope to enable automated tracking, which is essential for long-exposure astrophotography. Guiding cameras usually have a 1.25" socket for straightforward connection to the guidescope.

If astrophotography is your passion and you are searching for the perfect telescope for your astronomical observatory, Ritchey-Chretien telescopes are made for you. Two hyperbolic mirrors create nearly perfect images, providing a large, well-illuminated field of view free from coma, all within a compact design. The result is perfect stars right up to the edge of the field. This is why countless professional observatories and institutes rely on this system.

This filter set provides an affordable alternative to the more expensive filter sets offered by other manufacturers. Despite the lower price, these are high-quality, multi-coated interference filters. The set is specially optimized for use with ZW Optical’s ASI cameras. By combining exposures from the three color filters (red, green, blue) and the luminance filter (which also acts as an IR cut filter), you can create full-color images on your computer.

The ZWO Duo-Band Filter is a dual narrowband filter designed especially for use with color ASI cameras. It is ideal for astronomers who already own a color camera and want to try narrowband imaging or capture emission nebulae, without needing to buy a monochrome camera, filter wheel, and multiple narrowband filters. This filter provides an affordable way to explore narrowband imaging and is also a practical solution for astrophotography in light-polluted urban environments.

The ASI 2600 MC-Air is an advanced astrophotography camera that combines both imaging and guiding sensors in a single compact unit. The main imaging sensor is the Sony IMX571, featuring a native 16-bit ADC, a dynamic range of 14 stops, and square pixels sized at 3.76 micrometers. Readout noise is as low as 1.0 e, and the full well capacity is an impressive 80,000 e—achieved with no amplifier glow. The built-in ASI Air astrophotography computer, previously sold separately, is now integrated. 

The ASI2600MM Duo Mono brings both imaging and guiding sensors together in a single, compact body. The primary sensor is the Sony IMX571, featuring a native 16-bit ADC, a dynamic range of 14 stops, and 3.76 micrometer square pixels. Readout noise is as low as 1.0 e, and the full well capacity reaches an impressive 80,000 e, all with no amplifier glow. The guiding sensor is the SC2210, offering excellent near-infrared sensitivity and matching the performance of the ZWO ASI 220MM mini camera. 

The ASI 294MM is the first uncooled CMOS camera to feature the new Sony IMX492 sensor. This camera is ideal for imaging the Sun, Moon, and planets, as well as deep sky objects such as nebulae and galaxies. It uses Sony’s advanced back-illuminated sensor technology to deliver outstanding sensitivity. With 4.6 µm pixels, the ASI 294MM is a true all-rounder, offering excellent sensitivity even with very short exposure times. For even higher resolution, the camera can be used in "unlocked mode," reducing the pixel size to 2.3 µm.

The ZWO ASI 585MM Mono camera features a large sensor with high sensitivity, excellent resolution, and a fast frame rate. This makes it ideal for planetary imaging, as well as for capturing detailed images of the Sun and Moon, and even for deep sky objects. Equipped with the modern Sony IMX585 sensor, the camera delivers high resolution with 2.9µm pixels, a high frame rate, and zero amplifier glow. This combination makes the camera suitable not just for planets, the Sun, and the Moon, but also for long-exposure deep sky photography. 

This motherboard is designed to replace the built-in motherboard of the ZWO ASI662MC camera if the original part becomes defective. If needed, you can also contact the workshop for professional assistance.