Launch of Europe's largest astronomy network
Monday 29 March 2021

The entire arc of Milky Way, full of gas and dust, star clusters and emission nebulae, is a luminous background for the ESO-operated Very Large Telescope (VLT). Credit: M. Claro/ESO. Until now, Europe has had two major collaborative networks for
ground-based astronomy, one in the optical wavelength domain and the
other in the radio-wave domain. OPTICON and RadioNet have now come
together to form Europe's largest ground-based astronomy collaborative
network. Launched with funding to the tune of €15 million under the
H2020 programme, the project aims to harmonise observational methods and
tools, and provide access to a wider range of astronomy facilities. As
our knowledge of the Universe advances, astronomers increasingly need a
range of complementary techniques in order to analyse and understand
astronomical phenomena. As a result, the European Union has decided to
bring together the optical and radio networks OPTICON and RadioNet, who
have successfully served their respective communities over the past
twenty years. With €15 million in funding from the European
Commission's H2020 programme, the European astronomical community will
now benefit from the formation of Europe's largest ground-based
astronomy network: the OPTICON-RadioNet PILOT (ORP), which brings
together some twenty telescopes and telescope arrays. The ORP
network is intended to harmonise observational methods and tools for
ground-based optical and radio astronomy instruments, and provide
researchers with access to a wider range of facilities, building on the
success and experience of the OPTICON and RadioNet networks. The
new programme will make it easier for the astronomy community to access
these infrastructures, as well as provide training for new generations
of astronomers. According to the management team, « it is very
exciting to have this opportunity to further develop European
integration in astronomy, and develop new scientific opportunities for
astronomy research across Europe and globally. » The ORP will in
particular foster the development of the booming field of what is known
as multi-messenger astronomy, which makes use of a wide range of
wavelengths as well as gravitational waves, cosmic rays and neutrinos.
Removing barriers between communities by harmonising observation
protocols and analysis methods in the optical and radio domains will
enable astronomers to work better together when observing and monitoring
transient and variable astronomical events. Astronomers from 15
European countries, Australia and South Africa, as well as from 37
institutions, have already joined the ORP consortium. It will be
coordinated by the French Centre National de la Recherche Scientifique
(CNRS), which runs and contributes to several optical and radio
telescopes, the University of Cambridge (UK), and the Max Planck
Institute for Radio Astronomy (Germany). In Belgium, the network
involves the Institute of Astronomy at KU Leuven in charge of developing
new instrumentation for the Very Large Telescope Interferometer (VLTI,
Chile) and coordinating one of the seven European VLTI expertise
centers. The VLTI is a major European observatory at the forefront of
astronomical research. With the new ORP funding, the Institute of
Astronomy will develop a new VLTI observing mode dedicated to exoplanet
research, support the VLTI expertise centres network's activities, and
gather the whole VLTI community in Leuven in 2023. "We are excited to be
part of this new ORP network and to contribute to the development of
astronomical research and community in Europe" says Denis Defrère,
associate professor at the Institute of Astronomy. The management
team includes Jean-Gabriel Cuby, ORP project coordinator at the CNRS
National Institute for Earth Sciences and Astronomy, and Gerry Gilmore,
Professor at the University of Cambridge (UK) and Anton Zensus, Director
of the Max-Planck Institute for Radio Astronomy (Germany), as ORP
scientific coordinators for OPTICON and RadioNet respectively. This
project has received funding from the European Union's Horizon 2020
research and innovation programme under grant agreement No 101004719.
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