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KM3NeT blog posts

First KM3NeT group in China

08 November 2019 – We are happy to welcome the Sun Yat-sen University (SYSU), China, in our collaboration!

The HEP group at the School of Physics in SYSU is involved in various aspects of the intensity frontier, cosmic frontier and energy frontier, being involved in the Daya Bay reactor neutrino experiment, the Jiangmen Underground Neutrino Observatory, and the Large High Altitude Air Shower Observatory experiment among others.
The high-energy astrophysics group at the School of Physics and Astronomy focuses on theoretical study and data analysis of extreme high-energy phenomena, such as GRB, SNR and AGN. Together with the Tianqin Research Center at SPA, which is devoted to Tianqin project – a LISA-like space gravitational wave project, the group is focusing on the multi-messenger study, combining information from various messengers from space, such as electromagnetic radiation, neutrinos and gravitational waves.

“In short, the team at SYSU has a broad endeavor in neutrino physics and multi-messenger studies. With the help of KM3NeT, we will be able to further reach the neutrino spectrum in the cosmic frontier, crossing-over with other interesting sciences.” says Lily Yang, PI of the new KM3NeT group.

Workshop on simulation and data analysis

23 January 2019 – An internal KM3NeT workshop on ‘Simulation and Data Analysis’ was organised at INFN – Istitutio Nazionale di Fisica Nucleare in Genova, Italy. In the last two years the ARCA and ORCA sites were equipped with the first detection units which allowed for obtaining the first calibration data. The data comprises many measurements of muons created in the atmosphere. These measurements, although background to the neutrino signal, are extremely useful for the understanding of the detector performance and improving detector calibration and simulations of the detector response. The aim of the workshop was to review the currently existing simulation software tools and tuning them to reach agreement with the collected data on a new precision level.

Simulation of background events comprises very computationally intensive tasks, which must be run on the GRID and cloud infrastructures. For this, automatic workflows for the software deployment and running on different computer infrastructures were discussed and tests have been started. The simulation workflows also should keep provenance of the data to allow for repetition  and tracing of each simulated event. Automisation of the quality control of the data and simulation is yet another key task addressed at the workshop.

Launch of ESCAPE cluster for Open Science

20 November 2018 – As an ESFRI research infrastructure for neutrino astronomy and particle physics, KM3NeT actively participates in the new ESCAPE science cluster that will address Open Science data challenges shared by the participating European large research infrastructures for astronomy and particle physics. Early 2019, ESCAPE will be launched officially. Read the press release and the project summary.

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New KM3NeT management team elected

23 October 2018 – KM3NeT proudly presents its new management team!

In a few months from now, at 1 February 2019, the new management team will take over from the current one for a term of two years. Mauro Taiuti chairs the team as the Spokesperson (Director) of the KM3NeT Collaboration. He shares the tasks with Aart Heijboer, who is the Deputy Spokesperson. Miles Lindsey Clark is the Technical Project Manager and Paschal Coyle the Physics and Software Manager. Together they will lead the KM3NeT Collaboration of researchers and engineers in their endeavour of building the ARCA and ORCA neutrino detectors, taking data and searching with deep learning techniques and complex algorithms for signatures of neutrinos.

The KM3NeT Collaboration has great confidence in the team and congratulates all four members with their election!