iPhone Screenshots
Description
This software requires an external camera with UVC universal protocol, 4000*3000 resolution, specified hardware name, and tpyc communication. The camera is mounted via threaded installation at the telescope eyepiece position.
Users can activate the camera through the software interface and adjust auxiliary markers' size, position, as well as camera focus, brightness, and other parameters. This facilitates the alignment of the telescope's optical axis to achieve optical leveling between the primary mirror, secondary mirror, and eyepiece observation point.