The Astronomical Observatory of the Jagiellonian University (OA UJ) conducts a wide range of research in the fields of astronomy and astrophysics. Scientific activity is carried out within several departments, each focusing on specific research areas:
- learning about the processes of stellar evolution based on observations of physically variable stars and eclipsing stars,
- research on comet nuclei, including comets and asteroids originating from outside the Solar System,
- studies on the evolution of galaxies and the large-scale structure of the Universe,
- research on the spectroscopic properties and dynamics of radio-galaxies, including the mechanism of multiple radio activity of active galaxies.
- research on various mathematical formulations of gravitational physics and their applications in relativistic astrophysics,
- relativistic theory of the formation of structures (clusters of matter) in the early Universe,
- applications of gravitational lensing in cosmology,
- chaotic and critical phenomena in the general theory of relativity,
- applications of computer algebra systems in the General Theory of Relativity and relativistic astrophysics.
- contemporary astronomy of the highest energy gamma rays – the world projects High Energy Stereoscopic System (H.E.S.S.), Cherenkov Telescope Array (CTA), and Fermi Large Area Telescope (LAT),
- research on the astrophysics of accretion disks and relativistic jets,
- cosmological evolution of supermassive black holes and active galaxies,
- heliophysics – research on the Sun, including coronal ejections of matter,
- research on geophysical phenomena and the influence of the heliosphere on the Earth using measurements of extremely low frequency electromagnetic waves (ELF),
- theory of acceleration and propagation of cosmic rays at high energies.
- studies of the properties of magnetic fields in galaxies, in groups and galactic clusters conducted using the largest radio interferometers (JVLA, LOFAR, GMRT, WSRT, ATCA) and space observatories (XMM-Newton, Herschel),
- computer modeling of the evolution of cosmic magnetic fields and gravitational interactions between galaxies,
- determination of the cosmological evolution of radio spectra and star-forming properties of galaxies,
- studies of the morphology of blazars and determination of the properties of giant radio sources,
- explanation of the multi-range variability of blazars on scales from minutes to decades,
- determination of the properties of the interstellar medium by studying the effects of propagation of radio signals coming from pulsars,
- participation in a number of international studies as part of the implementation of the International LOFAR Telescope project.