At the Astronomical Observatory in Belgrade, out of the 9 telescopes still operate five: Large refractor, Solar spectrograph, Zeiss Astrograph, Photovisual Refractor Askania and Meade reflector (D=40 cm). Large Refractor - equatorial Zeiss 650/10550 mm is equipped with CCD cameras for binary stars observations (position angle and angular distance), for occultation observation (solar system bodies with stars or other objects). Solar Spectrograph of Littrow type, collimator lens 200/9000 mm, attached to the Zeiss equatorial 200/3020 mm, two astro-cameras Tessar and Petzval 100/800 mm for guiding and projecting. Dispersion element is a Bausch and Lomb grating with 600 l/mm, achieving a spectral resolution 130000 in the fourth order. This instrument is equipped with an Apogee Alta 47 CCD camera (chip size: 1024x1024 pixels, pixel size:15x15 micro m). The spectrograph is capable to observe solar spectrum from about 480 nm 690 nm, covering about 0.3 nm spectral interval per chip. It works in two regimes: integrated solar flux (sun as a star) and in low special resolution (approximately about 20 arc seconds along the dispersion. Zeiss Astrograph, Photovisual Refractor Askania and Meade reflector are using for CCD observation of positions of solar system bodies and their occultations. Currently, the new Astronomical Station (AS) is equipped with the Astro Optik (D=60 cm) reflector, with BVRI and Stromgren photometrical devices and with a stellar spectrograph with six different grating (from 150 l/mm to 2400 l/m), which will be linked to the telescope by fiber optic device. We plan to start with observations at AS during next year, with 60 cm diameter telescope. It will be used for photometric measurements of celestial bodies (mainly variable stars) in two photometric systems: BVRI and Stromgren. We also plan to equip AS with a 1.5 m class telescope in next few years for photometric observations of faint objects and spectroscopic observations too.