Dark Matter is one of the outstanding problems in modern physics. The possibility of annihilation or decay of Dark matter particles to standard model particles, in particular gamma-rays, in celestial bodies has given rise to the discipline of "Indirect detection of Dark matter". With the launch of the Fermi Gamma-ray Space Telescope in 2008 the indirect search for traces of dark matter in cosmological sources has entered a new exciting phase. In my talk I review the status of indirect detection of dark matter with gamma-rays, including results of the Fermi Gamma-ray Space Telescope as well as Imaging Air Cherenkov Telescopes (IACT), like H.E.S.S., MAGIC and VERITAS. I will also briefly address the perspectives for the next generation IACT, the Cherenkov Telescope Array