The ASTERICS project (Astronomy ESFRI and Research Infrastructure Cluster) is a collaborative cluster for the next generation ESFRI telescope facilities (ELT, CTA, SKA, KM3NeT, EST, see Figure 1) and other relevant research infrastructure initiatives in the area of astronomy, astrophysics and astroparticle physics. The ASTERICS Consortium consists of 26 partners, universities and research institutes, linked to one or more of these ESFRI facilities.
Each of the facilities is a mega-scale Research Infrastructure, endorsed and prioritised by the European Strategy Forum on Research Infrastructures (ESFRI). These ESFRI projects and their pathfinders significantly extend our astronomical observational capabilities; they also open new windows on the universe through the detection of neutrinos, high-energy particle showers and gravitational waves. Moreover, multi-messenger astronomy provides an unprecedented chance to probe the combined observational parameter space.
The purpose of ASTERICS was to enhance the ESFRI facilities’ impact in the future. ASTERICS brought together developers of all facilities to more efficiently develop tools and standards and to lay the foundation for true multi-messenger astroparticle physics.
Ensuring that Europe, and the world, fully exploits the impact of the ESFRI facilities, demands close integration through operations, (data) processing, analysis and data interoperability. Before the ASTERICS project, interactions between the communities had been limited. As each of these new facilities will generate vast amounts of data, ASTERICS focused on aspects of data handling (generation, transport, preservation, retrieval and analysis), interoperability between facilities (linked to smart analysis, scheduling for simultaneous observations) and fast response.
The project realised close collaboration between the diverse astronomy and astroparticle physics domains. The project partners developed several tools for data handling including new algorithms and standards, with the objective of future use on data from large astronomical facilities. Since many of these tools can be used already on the precursor or pathfinder data, the use and further development is guaranteed and will have a huge impact on the data handling of these facilities.