Thanks to its active optics and adaptive optics technologies, it enables scientific work at the international level.
It enables scientific observations in the visible region of the electromagnetic spectrum.
It is important for monitoring and analyzing atmospheric conditions, observatory site selection, and performance testing of the telescope optics.
High-resolution astrometric, photometric and spectroscopic observations are carried out.
Thanks to its wide field of view, photometry in crowded star fields and exoplanet and small-body research are conducted.
Photometry projects of long-period variable stars are conducted with this telescope.
