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Welcome to Skynet

Skynet is a global observing network for astronomical research, education, and automated observations. It connects observatories around the world so a heterogeneous fleet of optical and radio telescopes can be operated as a single, coordinated instrument.

These docs are organized for the three audiences who use Skynet most:

  • Telescope Owners


    Bring an observatory online, wire up devices through SkyNode, and run a queue.

    Start here

  • Observers


    Submit observations, organize them into projects, and work with results.

    Start here

  • Developers


    Authenticate to the public API, browse endpoints, and reference schemas.

    Start here


What is Skynet?

Skynet provides seamless access to remote telescopes, enabling:

  • Rapid response observations — capture transients like supernovae, gamma-ray bursts, and exoplanet transits.
  • Long-term monitoring — sustain campaigns on variable stars, AGN, and other periodic targets.
  • Educational engagement — give students and researchers hands-on astrophotography and data analysis.
  • Automated scheduling — allocate telescope time by scientific priority and resource availability.

How Skynet works

Skynet serves three overlapping roles — observers, observatory owners and managers, and consortiums — on a unified platform, while ensuring each observatory retains complete ownership and control of its telescopes.

  • Observers define the science: request observations through the web app or API, and Skynet matches each request to telescopes capable of fulfilling it. Results are processed and delivered automatically.
  • Observatory owners retain full authority over how their telescopes are used, who can access them, and when. SkyNode connects their hardware to the network without giving up local control.
  • Consortiums let partner institutions pool telescope time and coordinate multi-observatory campaigns while each member retains ownership of its own facilities.

For the conceptual model behind the network, see The AILA standard.