Variable stars, RR Lyrae, transients, supernovae, microlensing events.
By studying high redshift galaxies, we can learn about the evolution of galaxies throughout the history of the Universe.
Gaia is the ESA cornerstone mission set to revolutionise our understanding of the Milky Way.
Clusters of galaxies are the largest objects in the Universe that are held together by their own gravity, and provide great tools for studying the processes that govern AGN feedback.
A major area of research in X-ray astronomy is the accretion of matter on to black holes and neutron stars in the context of AGN and galactic X-ray binaries. Accretion is an energetic process and can give high luminosities.
During the epoch of reionization the first stars and black holes in the Universe (re-) ionized the Intergalactic Medium. Studying the epoch of reionization will tell us about the first galaxies.
Observations of tiny fluctuations in the cosmic microwave background radiation give powerful constraints on cosmological parameters and theories of the early universe.
Gravitational lensing is used to determine the masses of lensing galaxies and clusters and to study more distant galaxies that can be magnified by a factor of more than 20.
Quasars are the most luminous objects in the Universe and powered by accreting supermassive black holes in the centres of galaxies.