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The design of the new space-based gamma-ray telescope GAMMA-400 is presented.GAMMA-400 is optimized for the energy 100 GeV with the best parameters: theangular resolution ~0.01 deg, the energy resolution ~1%, and the protonrejection factor ~10E6, but is able to measure gamma-ray and electron +positron fluxes in the energy range from 100 MeV to 10 TeV. GAMMA-400 is aimedto a broad range of science topics, such as search for signatures of darkmatter, studies of Galactic and extragalactic gamma-ray sources, Galactic andextragalactic diffuse emission, gamma-ray bursts, as well as high-precisionmeasurements of spectra of cosmic-ray electrons + positrons, and nuclei.

The Space-Based Gamma-Ray Telescope GAMMA-400 and Its Scientific Goals