KM3NeT - News Archive

Archive of news items

Neutrino emission from our Galaxy! New observations by the IceCube Collaboration

29 June 2023 – The KM3NeT Collaboration congratulates the IceCube Collaboration after today’s announcement of an evidence in IceCube of high-energy neutrinos originating from our own Galaxy.

“Congratulations to the IceCube Collaboration for this great result. For the KM3NeT Collaboration it is a very important observation” says Paschal Coyle, the KM3NeT Spokesperson.

While IceCube has previously reported evidence for several sources of extragalactic neutrinos, the detection of neutrinos from the Milky Way has proved difficult,  due to the IceCube’s location at the South Pole, where a signal from within our Galaxy is observed as downgoing events and is therefore subject to a large background of atmospheric muons. Furthermore, as the signal was observed in the cascade channel, which has a limited angular resolution, it was not possible to determine if the signal is due to a diffuse source or a collection of unresolved point sources.

A telescope located in the Northern hemisphere, such as KM3NeT, observes our Galaxy using upgoing events, which have significantly less background than downgoing events and are therefore easier to detect. This in fact allowed ANTARES to report the first hint of a neutrino emission from the Galaxy (see the news item on the ANTARES web-site).

Moreover, the KM3NeT telescope will be able to observe the signal in the muon neutrino channel in addition to the electron neutrino channel and both with a much better angular resolution than IceCube.

“IceCube has confirmed our Galaxy is a guaranteed source of high-energy neutrinos. KM3NeT looks forward to unravelling the origins of this Galactic signal with unprecedented precision” concludes Paschal Coyle.

A cheerful Collaboration meeting in Salerno

14 June 2023 – The KM3NeT Collaboration met in Salerno last week.

It was quite a busy week, during which the status of data taking and data analysis of ARCA and ORCA as well as the contributions to the ICRC 2023 were reviewed, the progress in detector construction was discussed (celebrating the remarkable result of the 1,100th built DOM!) and the plans for next sea campaigns were refined.

The Collaboration continues to grow, with a research team joining as observer from Institute of Experimental Physics in Kosice, Slovakia (team leader: Blahoslav Pastircak).

Many thanks to the organizing team in Salerno!

The next Collaboration meeting will be in October in Paris and will include a day dedicated to celebrating the success of ANTARES, the first-undersea neutrino telescope ever built, progenitor of KM3NeT.

Three more detection units for KM3NeT/ORCA

1 May 2023 – During a two days sea operation, 27-28 April 2023, three detection units were successfully connected to the ORCA detector of KM3NeT in a record time of just over 24 hours. In addition, an acoustic beacon was recovered for battery replacement. The total number of deployed ORCA units is now 18, as visible in the sonar scan above.

As usual, the operation was performed with two ships: the Castor of Foselev, for deployment of the detection units, and the Janus II of SAAS (formerly Comex), equipped with a deep-sea remotely operated vehicle, for submarine operations.

Many thanks to the crews offshore as well as to the team who performed the functional tests of the new detection units from the shore station!

New marine science sensors coming online

24 April 2023 – Following a successful sea operation, the 16-19 April 2023, a collection of new marine science instrumentation is now connected to the Laboratoire Sous-marin Provence Mediterranee (LSPM)) sea floor infrastructure at the KM3NeT/ORCA site, near Toulon, France.

During the three day sea operation the so-called ‘pre-SJB’, developed by CPPM Marseille, was connected into the seafloor network. The pre-SJB is a passive junction box housing an AC power transformer and a sea return electrode. During the same operation a remotely operated vehicle (ROV) connected an interlink cable between the pre-SJB and the previously deployed SJB.

The SJB (Scientific Junction Box), developed by Ifremer, is a junction box with six output dedicated to marine science instrumentation. The Pre-SJB/SJB are located about 3.7 km west of the main KM3NeT/ORCA detector. The SJB with its associated instrumentation had already been deployed about a year ago and was waiting for the pre-SJB installation to come online. An earlier incarnation of the SJB was previously installed on the ANTARES junction box.

The instrumentation currently connected to the SJB includes the BathyBot seafloor crawler, its docking station BathyDock (MIO/DT-INSU-Marseille) and BathyReef (an artificial reef), a broad-band seismograph (GeoAzur-Nice), a germanium gamma spectrometer (CPPM-Marseille,) and a stereo biocamera (IP2I-Lyon).

Two ships were involved in the sea operation: the Raymond Croze of Orange Marine and the Janus II of SAAS.

The ROV being deployed from Janus II.
The ROV being deployed from Janus II.
The Raymond Croze.
The Raymond Croze of Orange Marine.
Deployment of the Pre-SJB.
Deployment of the Pre-SJB from the Raymond Croze.
Layout of the LSPM instrumentation connected to the SJB.
Layout of the LSPM instrumentation connected to the SJB.

The KM3NeT-INFRADEV2 project is launched

27 March 2023 – The kick-off Meeting of the KM3NeT-INFRADEV2 project, funded by the European Union, marked the official start of a new step toward the full implementation of the KM3NeT Research Infrastructure.

Involving institutes, laboratories and universities from France, Italy, Germany, Greece, The Netherlands, and Spain, this three-year European project aims to support the creation of a KM3NeT legal entity, accelerates the implementation of the detectors, develops the data management and open science practices of the collaboration as well as ensures a sustainable future for the infrastructure.

During the online meeting, each work package was presented to all partners involved and to Ioannis Andredakis, the Project Officer for the INFRADEV2 project from the European Research Executive Agency.

The leaders of the working groups and their team members also had the opportunity to further discuss their work together, giving a very positive start to the project.

For the next three years and thanks to the European funding, the consortium will continue firmly with the development and successful operation of the KM3NeT neutrino observatory.

 

 

 

The KM3NeT Collaboration met online

14 March 2023 – The KM3NeT Collaboration met online last week for the spring Collaboration meeting.

During the meeting we reviewed the status of data taking and data analysis of ARCA and ORCA, and discussed the progress in detector construction and the plans for next sea campaigns.

The Collaboration continues to grow: a research team has joined as full member of the Collaboration from University of Hull in UK (team leader: Brad Gibson) and a team from Ariel University in Israel (team leader: Dafne Guetta) has been welcomed as observer; furthermore, Marco Miceli of University of Palermo, Italy, has been accepted as associated member.

During the meeting the first-ever winners of the Giorgos Androulakis Prize, Tamás Gál and Edward Berbee, were announced.

The plan for next Collaboration meetings was also finalized. A decision of the KM3NeT Collaboration, meant to reduce the carboon footprint on the planet, is that at least one of the general Collaboration meetings is organized online per year. The next Collaboration meetings will take place in person, in early June in Salerno and in mid-October in Paris.

Tamás Gál and Edward Berbee awarded the Giorgos Androulakis Prize

9 March 2023 – During the Spring KM3NeT collaboration meeting, the first-ever winners of the Giorgos Androulakis Prize were announced.

With the prize, KM3NeT recognises “exceptional contribution to the KM3NeT project that has a particularly high impact on the success or progress of KM3NeT”.

The prize is named after Giorgos Androulakis, the late KM3NeT Quality Manager, in order to commemorate Giorgos’ dedication to the project. The prize is awarded in two categories: Early-Career Scientists and Technicians & Engineers.

The winners of the KM3NeT Giorgos Androulakis Prize are:

  • in the category Early Career Scientists: Tamás Gál of ECAP, “for his prominent role and numerous contributions in the development and maintenance of essential software tools for the Collaboration, like the KM3NeT GitLab server, wiki, elog and online monitoring system,  allowing the transformation of the KM3NeT software infrastructure into a modern software system; and for his continued dedication to provide documentation and support whenever  needed in the most helpful way”
  • in the category Technicians and Engineers: Edward Berbee of Nikhef, “for his incredible set of contributions to all mechanical aspects of KM3NeT, including design, construction and testing of DOMs, DUs, LOMs, his never ending work and tireless dedication to the experiment”

Congratulations to Tamás and Edward! With many thanks for your dedication to KM3NeT.

 

The winners of the Giorgos Androulakis Prize: Tamás Gál (left) and Edward Berbee (right).

New publication: The KM3NeT broadcast optical system

1 February 2023 – Via a long-distance electro-optical network the more than 6000 optical modules of KM3NeT in the deep sea are provided with a point-to-point connection to the control station on shore. The optical layer is presented in full details:

S. Aiello et al. 2023 JINST 18 T02001 DOI 10.1088/1748-0221/18/02/T02001

Abstract:

The optical data transport system of the KM3NeT neutrino telescope at the bottom of the Mediterranean Sea will provide more than 6000 optical modules in the detector arrays with a point-to-point optical connection to the control stations onshore. The ARCA and ORCA detectors of KM3NeT are being installed at a depth of about 3500 m and 2500 m, respectively and their distance to the control stations is about 100 kilometers and 40 kilometers. In particular, the two detectors are optimised for the detection of cosmic neutrinos with energies above about 1 TeV (ARCA) and for the detection of atmospheric neutrinos with energies in the range 1 GeV–1 TeV (ORCA). The expected maximum data rate is 200 Mbps per optical module. The implemented optical data transport system matches the layouts of the networks of electro-optical cables and junction boxes in the deep sea. For efficient use of the fibres in the system the technology of Dense Wavelength Division Multiplexing is applied. The performance of the optical system in terms of measured bit error rates, optical budget are presented. The next steps in the implementation of the system are also discussed.

The architecture of the KM3NeT broadcast optical system
The architecture of the optical layer connecting the ARCA detector of KM3NeT in the deep sea with the control station on shore.

ORCA enlarged with 4 new detection units

12 December 2022 – During a sea campaign performed last week, ORCA has been enlarged by means of 4 new detection units. This brings the total of detection units deployed in ORCA to 15, comprising more than 7,500 photomultipliers.

The operation was performed with the Castor ship of Foselev, for deployment of the detection units, and with the Janus II of SAAS (formerly Comex), equipped with a deep-sea remotely operated vehicle, for submarine operations.

The KM3NeT Collaboration congratulates the crews on the two ships, the team who performed careful checks from the shore station during the campaign, and all the teams who contributed to the construction of the detection units, for the success of the operation.

One of the ORCA detection units starting its journey from the Castor to the sea floor, 2500 m below. In the background is the Janus II.

 

Sonar map of ORCA, showing 14 detection units (the 15th one is beyond the boundary of the map). The 4 in the bottom part of the picture are the new ones installed.

Major upgrade of ARCA’s seafloor network

22 November 2022 – After 4 years of  activities carried out by the Italian funding agency INFN and Alcatel Submarine Networks, part of Nokia, the new subsea network for KM3NeT ARCA, funded under the Idmar regional project in Italy, is now complete.

The new system comprises a 100 km long electro-optical cable, equipped with 48 optical fibres for detector control and data communication and two electrical conductors for power distribution, connected to the shore station control and power feeding equipment, that can deliver up to 80 kW offshore. The cable is bifurcated in order to serve the two building blocks foreseen in ARCA.

During a 10 days long sea operation, which ended on November 17th, a cable termination frame (CTF) was installed on the northern branch of the cable. To this purpose the end of the cable, which was deployed already in 2020, was recovered from the sea floor and connected to the CTF onboard the deployment ship – the Ile d’Ouessant of Alcatel Submarine Networks. Then the CTF was carefully deployed to the target position on the sea floor. Extensive tests were done before and after the deployment to ensure its nominal behaviour.

The CTF is a large-size, 12-ton component which is equipped with four medium voltage converters and a total of 16 electrical and optical subsea connectors for connecting a set of submarine junction boxes to which the detection units will be in turn connected.

With this installation the connectivity and power transmission capabilities of the network have been increased by a factor four compared to the first part of the network, used to run the set of junction boxes and the first 30 detection units of ARCA Phase 1. This will allow for the completion of the construction of the first building block of ARCA and prepares the field for the installation of a second CTF on the other branch of the cable for the second building block.

The CTF at the end of the integration.
CTF onboard Ile d’Ouessant.
Overboarding of the CTF.