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The Cherenkov Telescope Array (CTA) will be the major global observatory forVHE gamma-ray astronomy over the next decade and beyond. It will be an explorerof the extreme universe, with a broad scientific potential: from understandingthe role of relativistic cosmic particles, to the search for dark matter.Covering photon energies from 20 GeV to 300 TeV, and with an angular resolutionunique in the field, of about 1 arc min, CTA will improve on all aspects of theperformance with respect to current instruments, surveying the high energy skyhundreds of times faster than previous TeV telescopes, and with a much deeperview. The very large collection area of CTA makes it an important probe oftransient phenomena. The first CTA telescope has just been inaugurated in theCanary Islands, Spain, and as more telescopes are added in the coming years,scientific operation will start. It is evident that CTA will have importantsynergies with many of the new generation astronomical and astroparticleobservatories. In this talk we will review the CTA science case from the pointof view of its synergies with other instruments and facilities, highlightingthe CTA needs in terms of external data, as well as the opportunities andstrategies for cooperation to achieve the basic CTA science goals.

Cherenkov Telescope Array Science: Multi-wavelength and multi-messenger perspectives