Neutrinos
The CPPM Neutrinos Astroparticle team is heavily involved in the ANTARES and KM3NeT neutrino telescopes deployed in the abyss of the Mediterranean Sea, used for cosmic neutrino research and fundamental neutrino properties studies.
As part of its research of high-energy neutrinos coming from transient astrophysical sources, the team is also participating in the development and operation of the COLIBRI robotic telescope, associated with the SVOM space detector optimised for the research of Gamma Ray Bursts.
The team also searches for new physics with the SuperNEMO experiment. This is realized through the study of a very rare radioactive decay, the double desintegration beta without neutrino .
Researchers and Research professors
- Vincent Bertin (ANTARES, KM3NeT, SVOM, team leader)
- Jose Busto (ANTARES, KM3NeT, SuperNEMO scientific coordinator)
- Paschal Coyle (ANTARES, Spokesman Collaboration KM3NeT)
- Damien Dornic (ANTARES, KM3NeT, SVOM scientific coordinator)
- Eric Kajfasz (SVOM)
- Mathieu Perrin-Terrin (ANTARES, KM3NeT national coordinator, neutrino tagging ANR ENTER)
Engineers and Technicians
- Thomas Auphan, Detectors and Data department (KM3NeT, SVOM)
- Stéphan Beurthey, mechanics department (KM3NeT)
- Jürgen Brunner, Detectors and Data department (ANTARES technical coordinator, KM3NeT, ANR LACTEL)
- Laurence Caillat, quality engineer (KM3NeT)
- Victoria Ciarlet-Thaon, CDD administration department (KM3NeT)
- Marie-Ange Cordier, Detectors and Data department (KM3NeT)
- Alain Cosquer, mechanics department (KM3NeT)
- Christian Curtil, IGE (SuperNEMO)
- Alexander Enzenhöfer, Detectors and Data department (ANTARES, KM3NeT, Detector operation manager)
- Feifei Huang, Detectors and Data department (KM3NeT)
- Evelyne Garçon, electronics department (KM3NeT)
- Sylvain Henry, Detectors and Data department (KM3NeT)
- Pascale Keller, Detectors and Data department (KM3NeT)
- Paul Lacroix, apprentice quality (KM3NeT)
- Philippe Lagier, mechanics department (KM3NeT)
- Sarah Lancelin, CDD administration department (KM3NeT)
- Jérôme Laurence, mechanics department (KM3NeT)
- Pierre Lebon, CDD mechanics department (KM3NeT)
- Emmanuel Le Guirriec, Detectors and Data department (KM3NeT)
- Christophe Lerouvillois, mechanics department (KM3NeT)
- Nick Lumb, Detectors and Data department (KM3NeT)
- Aurélien Marini, mechanics department (KM3NeT)
- Jérôme Royon, electronics department (KM3NeT)
- Stéphane Théraube, electronics department (KM3NeT)
Post-doctoral fellows
- Mohammed Bouta (2024-2026) (KM3NeT, ANR LACTEL)
- Mischa Breuhaus (2023-2025) (KM3NeT, SVOM)
- Jean-Grégoire Ducoin (2023-2025) (KM3NeT, SVOM)
- Hichem Tedjditi (2023-2025) (SuperNEMO, Plateau Radon)
PHD students
- Diane Joly (2023-2026) (KM3NeT)
- Francesco Magnani (2023-2026) (KM3NeT)
- Lucie Petit (2023-2026) (Neutrino tagging)
- Paul Deguire (2024-2027) (KM3NeT)
- Sharif El Mentawi (2024-2027) (KM3NeT)
- Odhongo Schephatia (2024-2027) (Plateau Radon)
The ANTARES detector was the largest neutrino telescope in the Northern Hemisphere and the first one built in a marine environment. From 2006 to 2022, it was installed by 2500 m depth in the bottom of the Mediterranean Sea off the coast of Toulon (France).
The main goal of ANTARES was the search for cosmic neutrinos coming from the violent phenomena of the Universe. The ANTARES underwater infrastructure also constituted a real multidisciplinary platform for experimentation enabling numerous studies in the fields of Marine, Earth and Environmental Sciences.
At CPPM, the team plays a leading role in the operation of this detector and data analysis. In particular, it is heavily involved in:
- searches for cosmic neutrinos from transient or variable sources ;
- multi-messenger analyses of astrophysical sources ;
- the indirect search for Dark Matter towards the Sun and the galactic centre ;
- measurement of neutrino oscillation parameters and constraints on sterile neutrino models.
The CPPM team is also responsible for the operation and maintenance of the detector and its control room, as the laboratory hosting the experiment. It is also heavily involved in the calibration and the Collaboration governance.
Presentation of the ANTARES project, by Antoine Kouchner, Researcher at APC | Production CPPM 2023
The origins of the ANTARES project, by Patrick Lamare, Technical Manager of ANTARES at CEA | Production CPPM 2023
Why an underwater detector offshore from La Seyne-sur-Mer? By Vincent Bertin, Researcher at CPPM | Production CPPM 2023
Detecting neutrinos with ANTARES, by José Busto, Researcher at CPPM | Production CPPM 2023
How is an ANTARES detection line built? By Jérôme Laurence, Assistant Engineer at CPPM | Production CPPM 2023
How can ANTARES sensors be synchronised? By Frédéric Rhétoré, Engineer at CPPM | Production CPPM 2023
How to position the detection lines of the ANTARES telescope? By an Engineer at CPPM | Production CPPM 2023
How do you interface a detector at the bottom of the sea? By Michel Ageron, Engineer at CPPM | Production CPPM 2023
Why was the Michel Pacha Institute the control room for ANTARES? By Paschal Coyle, Researcher at CPPM | Production CPPM 2023
The main results of the ANTARES experiment, by Antoine Kouchner, Researcher at APC | Production CPPM 2023
The KM3NeT detector is a second generation neutrino telescope installed in the abyss of the Mediterranean Sea, designed based on the return of experience of the ANTARES detector.
A first version of detector, called ARCA, installed off Sicily, is dedicated to the search for high energy neutrinos from cataclysms of the Universe such as supernovæ or the formation and evolution of black holes. A second detector, called ORCA, is under construction off Toulon. It will allow a determination of the mass hierarchy of neutrinos, by precisely studying the flux of atmospheric neutrinos crossing the Earth. The MEUST-NUMerEnv underwater infrastructure of the ORCA detector also constitutes a multidisciplinary experimental platform hosting numerous studies in the fields of Marine, Earth and Environmental Sciences within the framework of the EMSO seabed observatory.
This project is financed with the support of the European Union with the European Regional Development Fund.
At CPPM, the team plays a leading role in the design, construction and operation of the KM3NeT-ORCA detector and KM3NeT data analyses. In particular, it is heavily involved in:
- the determination of the mass hierarchy of neutrinos ;
- multi-messenger analyses of astrophysical sources ;
- searches for cosmic neutrinos from transient or variable sources ;
- the indirect search for Dark Matter.
The CPPM team is also responsible for the construction and operation of the KM3NeT-ORCA detector, as well as the MEUST-NUMerEnv underwater infrastructure, and of the control room, as host laboratory of the French KM3NeT site. It is also heavily involved in the governance of the KM3NeT Collaboration.
What is the KM3NeT project? By Paschal Coyle, Researcher at CPPM | Production CPPM 2023
How to finance an international collaboration? By Victoria Ciarlet, Project Manager at CPPM | Production CPPM 2023
How is the KM3NeT detector being built? By Nick Lumb, Engineer at CPPM | Production CPPM 2023
The construction of a KM3NeT detection line, by Aurélien Marini, Head of KM3NeT line integration at CPPM | Production CPPM 2023
Deployment of KM3NeT lines at sea, by Sylvain Henry, Engineer at CPPM | Production CPPM 2023
Data transmission from the KM3NeT detector, by Evelyne Garçon, Engineer at CPPM | Production CPPM 2023
The power supply system of the KM3NeT detector, by Stéphane Théraube, Engineer at CPPM | Production CPPM 2023| Production CPPM 2023
How can data be recovered from the seabed? By Thomas Auphan, Engineer at CPPM
How to analyse the data flow from the KM3NeT detector in real time? By Emmanuel Le Guirriec, Engineer at the CPPM | Production CPPM 2023
The space mission SVOM (Space based multi-band astronomical Variable Objects Monitor) is a Sino-French project dedicated to the detection and study of gamma-ray bursts whose launch is planned for June 2024. The duration of operation is planned for 3 years with a 2-year extension.
Fortuitously discovered in the 1970s, gamma-ray bursts are intense flashes of high-energy photons whose origin seems to be linked to the explosion of hyper massive stars or the fusion of two neutron stars. These bursts are the brightest phenomena ever observed since the Big Bang. These sources could also be at the origin of cosmic rays of very high energy. As a result, they are also the most favourable candidates as counterparts for high energy neutrinos. This synergy with neutrinos is one of the strong themes of the CPPM’s ANTARES/KM3NeT team. Research conducted with SVOM will provide additional information to the information collected by ANTARES and KM3NeT.
The CPPM team is involved in the construction and operation of the COLIBRI robotic telescope that will be installed in San Pedro Martir, Mexico and dedicated to optical and infrared monitoring of SVOM satellite alerts. The CPPM is mainly involved in the telescope software, in particular on the development of the instrument's instrumental centre and all the analysis tools of visible and near infrared images.
The SuperNEMO detector is a modular tracko-calorimetric detector, allowing to study the kinematics of the double bêta disintegration (simultaneous emission of two electrons coming from the same nucleus and whose sum energy is fixed). For that, the SuperNEMO detector, is constituted by a central module, source surrounded by two tracking modules where the trajectory of the two electrons is reconstructed and finally two modules of plastic scintillators for the calculation of the energy of the electrons.
The SuperNEMO project is part of experiments to discover the nature of neutrino and thus determine whether or not it is identical to its antiparticle. This research, which explores a new physics beyond the Standard Model, is realized through the study of a very rare radioactive decay, the double disintegration bêta without Neutrino . Beyond the study of the Dirac or Majorana nature of neutrino, the allows us to characterize the mass hierarchy of neutrinos and explore several fundamental aspects related to the non conservation of lepton numbers.
Responsabilités de l’équipe :
During the SuperNEMO construction phase the CPPM team works on the following tasks:
- Purification of tracer gas to keep radon concentration below 150 µBq/m3 ;
- Reconditioning and circulation of tracker gas ;
- Study of SuperNEMO background noise using gamma tracking.
Publications Astronomie neutrino
Articles
2025: 8 articles
- Acoustic Positioning for Deep Sea Neutrino Telescopes with a System of Piezo Sensors Integrated into Glass Spheres, A. Albert et al. , ANTARES Collaboration, Exper. Astron. 59 (2025) 6
- JUNO Sensitivity to Invisible Decay Modes of Neutrons, A. Abusleme et al. , JUNO Collaboration, Eur. Phys. J. C 85 (2025) 5
- Prediction of Energy Resolution in the JUNO Experiment, A. Abusleme et al. , JUNO Collaboration, Chin. Phys. C 49 (2025) 013003
- Potential to Identify the Neutrino Mass Ordering with Reactor Antineutrinos in JUNO, A. Abusleme et al. , JUNO Collaboration, Chin. Phys. C 49 (2025) 033104
- Observation of an ultra-high-energy cosmic neutrino with KM3NeT, S. Aiello et al. , KM3NeT Collaboration, Nature 638 (2025) 376-382
- First detection of a tagged neutrino in the NA62 experiment, E. Cortina Gil et al. , NA62 Collaboration, Phys. Lett. B 863 (2025) 139345
- First detection of a tagged neutrino in the NA62 experiment, E. Cortina Gil et al. , NA62 Collaboration, Phys. Lett. B 863 (2025) 139345
- Observation of the decay and measurement of its branching ratio, E. Cortina Gil et al. , NA62 Collaboration, J. High Energy Phys. 02 (2025) 191
2024: 22 articles
- Model Independent Approach of the JUNO B Solar Neutrino Program, J. Zhao et al. , JUNO Collaboration, Astrophys. J 965 (2024) 122
- Embedded software of the KM3NeT central logic board, S. Aiello et al. , KM3NeT Collaboration, Comput. Phys. Commun. 296 (2024) 109036
- Prospects for combined analyses of hadronic emission from -ray sources in the Milky Way with CTA and KM3NeT, T. Unbehaun et al. , CTA Consortium, KM3NeT Collaboration, Eur. Phys. J. C 84 (2024) 112
- Real-time monitoring for the next core-collapse supernova in JUNO, A. Abusleme et al. , JUNO Collaboration, J. Cosmol. Astropart. P 01 (2024) 057
- Searches for Neutrinos in the Direction of Radio-bright Blazars with the ANTARES Telescope, A. Albert et al. , ANTARES Collaboration, OVRO Collaboration, Astrophys. J 964 (2024) 3
- Multi-band analyses of the bright GRB~230812B and the associated SN2023pel, T. Hussenot-Desenonges et al. , GRANDMA Collaboration, Mon. Not. Roy. Astron. Soc 530 (2024) 1-19
- Ready for O4 II: GRANDMA Observations of Swift GRBs during eight-weeks of Spring 2022, I. Tosta e Melo et al. , GRANDMA Collaboration, Astron. Astrophys. 682 (2024) A141
- Measurement of the K+ → π+γγ decay, Cortina Gil, Eduardo et al. , Phys. Lett. B 850 (2024) 138513
- Searches for neutrino counterparts of gravitational waves from the LIGO/Virgo third observing run with KM3NeT, S. Aiello et al. , KM3NeT Collaboration, J. Cosmol. Astropart. P 04 (2024) 026
- The Design and Technology Development of the JUNO Central Detector, A. Abusleme et al. , JUNO Collaboration, Eur. Phys. J. Plus 139 (2024) 1128
- Search for leptonic decays of the dark photon at NA62, E. Cortina Gil et al. , NA62 Collaboration, Phys. Rev. Lett 133 (2024) 111802
- Development of a new CEDAR for kaon identification at the NA62 experiment at CERN, A. Bethani et al. , NA62 Collaboration, J. Instrum 19 (2024) P05005
- Astronomy potential of KM3NeT/ARCA, S. Aiello et al. , KM3NeT Collaboration, Eur. Phys. J. C 84 (2024) 885
- Differential Sensitivity of the KM3NeT/ARCA detector to a diffuse neutrino flux and to point-like source emission: exploring the case of the Starburst Galaxies, S. Aiello et al. , KM3NeT Collaboration, Astropart. Phys. 162 (2024) 102990
- Results of the follow-up of ANTARES neutrino alerts, Albert, A. et al. , ANTARES Collaboration, Master Collaboration, MWA Collaboration, Swift Collaboration, TAROT Collaboration, J. Cosmol. Astropart. P 09 (2024) 042
- Atmospheric muons measured with the KM3NeT detectors in comparison with updated numeric predictions, S. Aiello et al. , KM3NeT Collaboration, Eur. Phys. J. C 84 (2024) 696
- Search for Neutrino Emission from GRB 221009A using the KM3NeT ARCA and ORCA detectors, Aiello, S. et al. , KM3NeT Collaboration, J. Cosmol. Astropart. P 08 (2024) 006
- Constraints on the energy spectrum of the diffuse cosmic neutrino flux from the ANTARES neutrino telescope, A. Albert et al. , ANTARES Collaboration, J. Cosmol. Astropart. P 08 (2024) 038
- Measurement of neutrino oscillation parameters with the first six detection units of KM3NeT/ORCA, Aiello, S. et al. , KM3NeT Collaboration, J. High Energy Phys. 10 (2024) 206
- First search for decays, M. U. Ashraf et al. , NA62 Collaboration, Phys. Lett. B 859 (2024) 139122
- A simple model of dust extinction in gamma-ray burst host galaxies, N.A. Rakotondrainibe et al. , Astron. Astrophys. 690 (2024) A373
- The detectability of high-redshift gamma-ray bursts near-infrared afterglows with CAGIRE, F. Fortin et al. , Astron. Astrophys. 691 (2024) A324
2023: 23 articles
- Studying Bioluminescence Flashes with the ANTARES Deep Sea Neutrino Telescope, N. Reeb et al. , ANTARES Collaboration, Limnol. Oceanogr.: Methods 21 (2023) 734-760
- Measurement of double- decay of Nd to the 0 excited state of Sm in NEMO-3, X. Aguerre et al. , NEMO-3 Collaboration, Eur. Phys. J. C 83 (2023) 1117
- Performance of the NA62 trigger system, Cortina Gil, Eduardo et al. , J. High Energy Phys. 03 (2023) 122
- Limits on the nuclearite flux using the ANTARES neutrino telescope, A. Albert et al. , ANTARES Collaboration, J. Cosmol. Astropart. P 01 (2023) 012
- Search for Gamma-Ray and Neutrino Coincidences Using HAWC and ANTARES Data, Ayala Solares, H.A. et al. , ANTARES Collaboration, HAWC Collaboration, AMON Collaboration, Astrophys. J 944 (2023) 166
- KM3NeT broadcast optical data transport system, S. Aiello et al. , KM3NeT Collaboration, J. Instrum 18 (2023) T02001
- A search for the decay, Cortina Gil, Eduardo et al. , Phys. Lett. B 838 (2023) 137679
- Review of the online analyses of multi-messenger alerts and electromagnetic transient events with the ANTARES neutrino telescope, A. Albert et al. , J. Cosmol. Astropart. P 08 (2023) 072
- First observation of the cosmic ray shadow of the Moon and the Sun with KM3NeT/ORCA, S. Aiello et al. , KM3NeT Collaboration, Eur. Phys. J. C 83 (2023) 344
- JUNO Sensitivity on Proton Decay Searches, A. Abusleme et al. , JUNO Collaboration, Chin. Phys. C 47 (2023) 113002
- Hint for a TeV neutrino emission from the Galactic Ridge with ANTARES, A. Albert et al. , ANTARES Collaboration, Phys. Lett. B 841 (2023) 137951
- Probing invisible neutrino decay with KM3NeT/ORCA, S. Aiello et al. , KM3NeT Collaboration, J. High Energy Phys. 04 (2023) 090
- GRANDMA and HXMT Observations of GRB 221009A: The Standard Luminosity Afterglow of a Hyperluminous Gamma-Ray Burst—In Gedenken an David Alexander Kann, D. A. Kann et al. , GRANDMA Collaboration, Astrophys. J. Lett 948 (2023) L12
- Search for neutrino counterparts to the gravitational wave sources from LIGO/Virgo O3 run with the ANTARES detector, A. Albert et al. , ANTARES Collaboration, J. Cosmol. Astropart. P 04 (2023) 004
- JUNO sensitivity to Be, pep, and CNO solar neutrinos, A. Abusleme et al. , JUNO Collaboration, J. Cosmol. Astropart. P 10 (2023) 022
- The JUNO experiment Top Tracker, A. Abusleme et al. , JUNO Collaboration, Nucl. Instrum. Meth. A 1057 (2023) 168680
- Search for dark photon decays to μ μ at NA62, Cortina Gil, Eduardo et al. , J. High Energy Phys. 09 (2023) 035
- High resolution seafloor thermometry for wave and upwelling monitoring using Distributed Acoustic Sensing, J. D. Pelaez Quiñones et al. , Sci. Rep 13 (2023) 17459
- Improved calorimetric particle identification in NA62 using machine learning techniques, Cortina Gil, Eduardo et al. , J. High Energy Phys. 11 (2023) 138
- A study of the decay, Cortina Gil, Eduardo et al. , J. High Energy Phys. 09 (2023) 040
- CAGIRE: a wide-field NIR imager for the COLIBRI 1.3 meter robotic telescope, A. Nouvel de la Flèche et al. , Exper. Astron. 56 (2023) 645-685
- JUNO sensitivity to the annihilation of MeV dark matter in the galactic halo, Abusleme, Angel et al. , JUNO Collaboration, J. Cosmol. Astropart. P 09 (2023) 001
- Search for decays into the final state, Cortina Gil, Eduardo et al. , Phys. Lett. B 846 (2023) 138193
2022: 20 articles
- Collaborative Experience between Scientific Software Projects using Agile Scrum Development, A. L. Baxter et al. , Softw Pract Exper. (2022) 1-20
- Determining the Neutrino Mass Ordering and Oscillation Parameters with KM3NeT/ORCA, S. Aiello et al. , KM3NeT Collaboration, Eur. Phys. J. C 82 (2022) 26
- Microplastics in the abyss: a first investigation into sediments at 2443-m depth (Toulon, France), L. Cutroneo et al. , Environ. Sci. Pollut. Res. (2022)
- Combined sensitivity of JUNO and KM3NeT/ORCA to the neutrino mass ordering, S. Aiello et al. , KM3NeT Collaboration, members of JUNO Collaboration, J. High Energy Phys. 03 (2022) 055
- Implementation and first results of the KM3NeT real-time core-collapse supernova neutrino search, S. Aiello et al. , KM3NeT Collaboration, Eur. Phys. J. C 82 (2022) 317
- SNEWPY: A Data Pipeline from Supernova Simulations to Neutrino Signals, A. L. Baxter et al. , Astrophys. J 925 (2022) 107
- Nanobeacon: A time calibration device for the KM3NeT neutrino telescope, S. Aiello et al. , KM3NeT Collaboration, Nucl. Instrum. Meth. A 1040 (2022) 167132
- Neutrino tagging: a new tool for accelerator based neutrino experiments, M. Perrin-Terrin et al. , Eur. Phys. J. C 82 (2022) 465
- Search for non-standard neutrino interactions with 10 years of ANTARES data, Albert, A. et al. , ANTARES Collaboration, J. High Energy Phys. 07 (2022) 048
- Damping signatures at JUNO, a medium-baseline reactor neutrino oscillation experiment, J. Wang et al. , JUNO Collaboration, J. High Energy Phys. 06 (2022) 062
- Search for Spatial Correlations of Neutrinos with Ultra-High-Energy Cosmic Rays, Abu-Zayyad, T. et al. , ANTARES Collaboration, IceCube Collaboration, Pierre Auger Collaboration, Telescope Array Collaboration, Astrophys. J 934 (2022) 164
- Search for solar atmospheric neutrinos with the ANTARES neutrino telescope, A. Albert et al. , ANTARES Collaboration, J. Cosmol. Astropart. P 06 (2022) 018
- Search for magnetic monopoles with ten years of the ANTARES neutrino telescope, A. Albert et al. , ANTARES Collaboration, J. High Energy Astron. Phys 34 (2022) 1-8
- Search for secluded dark matter towards the Galactic Centre with the ANTARES neutrino telescope, A. Albert et al. , ANTARES Collaboration, J. Cosmol. Astropart. P 06 (2022) 028
- The KM3NeT multi-PMT optical module, Aiello, S. et al. , KM3NeT Collaboration, J. Instrum 17 (2022) P07038
- Sub-percent precision measurement of neutrino oscillation parameters with JUNO, A. Abusleme et al. , JUNO Collaboration, Chin. Phys. C 46 (2022) 123001
- Mass testing and characterization of 20-inch PMTs for JUNO, A. Abusleme et al. , Eur. Phys. J. C 82 (2022) 1168
- Prospects for detecting the diffuse supernova neutrino background with JUNO, A. Abusleme et al. , JUNO Collaboration, J. Cosmol. Astropart. P 10 (2022) 033
- COLIBRI, a wide-field 1.3 m robotic telescope dedicated to the transient sky, S. Basa et al. , Proc. SPIE Int. Soc. Opt. Eng. 12182 (2022) 121821S
- A measurement of the decay, Cortina Gil, Eduardo et al. , J. High Energy Phys. 11 (2022) 011
Conference proceedings
2025: 3 conference proceedings
- Latest multi-messenger results of the KM3NeT real-time analysis framework, J. Palacios Gonzalez, V. Cecchini, S. Celli, I. Del Rosso, I., D. Dornic , F. Filippini, E. Le Guirriec , J. De Favereau, G. Illuminati, M. Lamoureux, M. Mastrodicasa, F. Salesa Greus, A. Sánchez Losa, S. Le Stum , G. Vannoye , A. Veutro, A. Zegarelli, PoS, 2024, 42nd International Conference on High Energy Physics (2025) 667, Prague, indéfini, 17-24 Jul 2024
- The KM3NeT online processing for multi-messenger alerts, M. Mastrodicasa, V. Cecchini, S. Celli, J. De Favereau de Jeneret, D. Dornic , F. Filippini, E. Giorgio, G. Illuminati, M. Lamoureux, E. Le Guirriec, S. Le Stum , J. Palacios Gonzalez, G. Vannoye , A. Veutro, A. Zegarelli, EPJ Web Conf., 319, 9th Roma International Conference on AstroParticle Physics (2025) 12010, Rome, Italy, 23-27 Sep 2024
- KM3NeT Online Multi-Messenger Results, F. Carenini, V. Cecchini, S. Celli, D. Dornic , J. De Favereau, F. Filippini, L. Fusco, E. Giorgio, E. Le Guirriec , G. Illuminati, M. Lamoureux, F. Magnani , M. Marconi, M. Mastrodicasa, J. Palacios González, E. Pastor Gómez, I. Del Rosso, F. Salesa Greus, A. Sánchez Losa, S. Le Stum , G. Vannoye , A. Veutro, EPJ Web Conf., 319, 9th Roma International Conference on AstroParticle Physics (2025) 08004, Rome, Italy, 23-27 Sep 2024
2024: 5 conference proceedings
- High Energy Physics Opportunities Using Reactor Antineutrinos, C. Awe, P. S. Barbeau, A. Haghighat, S. C. Li, J. M. Link, V. Mascolino, T. Subedi, K. Walkup, A. Aguilar-Arevalo, X. Bertou, C. Bonifazi, G. Cancelo, B. A. Cervantes-Vergara, C. Chavez, J. C. D'Olivo, J. M. De Egea, J. C. dos Anjos, J. Estrada, A. R. F. Neto, A. Foguel, R. Ford, J. Gasanego, V. Gollo, F. Izraelevitch, B. Kilminster, J. H. P. Lima, M. Makler, L. H. Mendes, J. Molina, P. Mota, I. Nasteva, E. Paolini, C. Romero, Y. Sarkis, M. S. Haro, A. Soto, D. Stalder, J. Tiffenberg, C. Torres, M. Lindner, F. P. An, A. B. Balantekin, H. R. Band, M. Bishai, S. Blyth, G. F. Cao, J. Cao, J. F. Chang, Y. Chang, H. S. Chen, S. M. Chen, Y. Chen, Y. X. Chen, J. Cheng, Z. K. Cheng, J. J. Cherwinka, M. C. Chu, J. P. Cummings, O. Dalager, F. S. Deng, Y. Y. Ding, M. V. Diwan, T. Dohnal, J. Dove, M. Dvořák, D. A. Dwyer, J. P. Gallo, M. Gonchar, G. H. Gong, H. Gong, W. Q. Gu, J. Y. Guo, L. Guo, X. H. Guo, Y. H. Guo, Z. Guo, R. W. Hackenburg, S. Hans, M. He, K. M. Heeger, Y. K. Heng, A. Higuera, Y. K. Hor, Y. B. Hsiung, B. Z. Hu, J. R. Hu, T. Hu, Z. J. Hu, H. X. Huang, X. T. Huang, P. Huber, D. E. Jaffe, K. L. Jen, X. L. Ji, X. P. Ji, R. A. Johnson, D. Jones, L. Kang, S. H. Kettell, S. Kohn, M. Kramer, J. Lee, J. H. C. Lee, R. T. Lei, R. Leitner, J. K. C. Leung, F. Li, H. L. Li, J. J. Li, Q. J. Li, S. Li, W. D. Li, X. N. Li, X. Q. Li, Y. F. Li, Z. B. Li, H. Liang, C. J. Lin, G. L. Lin, S. Lin, J. J. Ling, L. Littenberg, J. C. Liu, J. L. Liu, C. Lu, H. Q. Lu, J. S. Lu, K. B. Luk, X. B. Ma, X. Y. Ma, Y. Q. Ma, R. C. Mandujano, C. Marshall, D. A. Martinez Caicedo, K. T. McDonald, R. D. McKeown, Y. Meng, J. Napolitano, D. Naumov, E. Naumova, A. Olshevskiy, H.-R. Pan, J. Park, S. Patton, J. C. Peng, C. S. J. Pun, F. Z. Qi, M. Qi, X. Qian, N. Raper, J. Ren, C. M. Reveco, R. Rosero, B. Roskovec, X. C. Ruan, H. Steiner, J. L. Sun, T. Tmej, K. Treskov, W.-H. Tse, C. E. Tull, B. Viren, V. Vorobel, C. H. Wang, J. Wang, M. Wang, N. Y. Wang, R. G. Wang, W. Wang, X. Wang, Y. Wang, Y. F. Wang, Z. Wang, Z. M. Wang, H. Y. Wei, L. H. Wei, L. J. Wen, K. Whisnant, C. G. White, H. L. H. Wong, E. Worcester, D. R. Wu, F. L. Wu, Q. Wu, W. J. Wu, D. M. Xia, Z. Q. Xie, Z. Z. Xing, J. L. Xu, T. Xu, T. Xue, C. G. Yang, L. Yang, Y. Z. Yang, H. F. Yao, M. Ye, M. Yeh, B. L. Young, H. Z. Yu, Z. Y. Yu, B. B. Yue, S. Zeng, Y. Zeng, L. Zhan, F. Y. Zhang, H. H. Zhang, J. W. Zhang, Q. M. Zhang, X. T. Zhang, Y. M. Zhang, Y. X. Zhang, Y. Y. Zhang, Z. J. Zhang, Z. P. Zhang, Z. Y. Zhang, J. Zhao, L. Zhou, H. L. Zhuang, J. H. Zou, A. Abusleme, T. Adam, S. Ahmad, R. Ahmed, S. Aiello, G. P. An, Q. An, G. Andronico, N. Anfimov, V. Antonelli, T. Antoshkina, B. Asavapibhop, J. P. A. M. de André, D. Auguste, A. Babic, W. Baldini, A. Barresi, E. Baussan, M. Bellato, A. Bergnoli, E. Bernieri, T. Birkenfeld, S. Blin, D. Blum, A. Bolshakova, M. Bongrand, C. Bordereau, D. Breton, A. Brigatti, R. Brugnera, R. Bruno, A. Budano, M. Buesken, M. Buscemi, J. Busto , I. Butorov, A. Cabrera, H. Cai, X. Cai, Y. K. Cai, Z. Y. Cai, A. Cammi, A. Campeny, C. Y. Cao, R. Caruso, C. Cerna, I. Chakaberia, P. P. Chen, P. A. Chen, S. Chen, X. Chen, Y. W. Chen, Z. Chen, Y. Cheng, D. Chiesa, P. Chimenti, A. Chukanov, A. Chuvashova, G. Claverie, C. Clementi, B. Clerbaux, S. Di Lorenzo, D. Corti, S. Costa, F. D. Corso, C. De La Taille, J. Deng, Z. Deng, Z. Y. Deng, W. Depnering, M. Diaz, X. F. Ding, B. Dirgantara, S. Dmitrievsky, G. Donchenko, J. M. Dong, D. Dornic , E. Doroshkevich, M. Dracos, F. Druillole, S. X. Du, S. Dusini, M. Dvorak, T. Enqvist, H. Enzmann, A. Fabbri, L. Fajt, D. H. Fan, L. Fan, C. Fang, J. Fang, W. X. Fang, M. Fargetta, A. Fatkina, D. Fedoseev, V. Fekete, L. C. Feng, Q. C. Feng, A. Formozov, A. Fournier, H. N. Gan, F. Gao, A. Garfagnini, A. Göttel, C. Genster, M. Giammarchi, A. Giaz, N. Giudice, G. Gong, O. Gorchakov, Y. Gornushkin, M. Grassi, C. Grewing, V. Gromov, M. Gu, X. Gu, Y. Gu, M. Y. Guan, N. Guardone, M. Gul, C. Guo, W. L. Guo, P. Hackspacher, C. Hagner, R. Han, Y. Han, M. Hassan, W. He, T. Heinz, P. Hellmuth, R. Herrera, D. J. Hong, S. J. Hou, Y. Hsiung, H. Hu, J. Hu, S. Y. Hu, C. H. Huang, G. H. Huang, Q. H. Huang, W. H. Huang, X. Huang, Y. B. Huang, J. Q. Hui, L. Huo, W. Huo, C. Huss, S. Hussain, A. Insolia, A. Ioannisian, R. Isocrate, X. Z. Ji, H. H. Jia, J. J. Jia, S. Y. Jian, D. Jiang, X. S. Jiang, R. Y. Jin, X. P. Jing, C. Jollet, J. Joutsenvaara, S. Jungthawan, L. Kalousis, P. Kampmann, M. Karagounis, N. Kazarian, A. Khan, W. Khan, K. Khosonthongkee, P. Kinz, D. Korablev, K. Kouzakov, A. Krasnoperov, Z. Krumshteyn, A. Kruth, N. Kutovskiy, P. Kuusiniemi, T. Lachenmaier, C. Landini, S. Leblanc, V. Lebrin, F. Lefevre, R. Lei, J. Leung, C. Li, D. Li, H. Li, J. Li, K. J. Li, M. Z. Li, M. Li, N. Li, R. H. Li, S. F. Li, S. J. Li, T. Li, W. G. Li, X. M. Li, X. L. Li, Y. Li, Z. Li, Z. Y. Li, J. J. Liang, D. Liebau, A. Limphirat, S. Limpijumnong, S. X. Lin, T. Lin, I. Lippi, F. Liu, H. D. Liu, H. B. Liu, H. J. Liu, H. T. Liu, H. Liu, M. Liu, Q. Liu, R. X. Liu, S. Y. Liu, S. B. Liu, S. L. Liu, X. W. Liu, X. Liu, Y. Liu, A. Lokhov, P. Lombardi, C. Lombardo, K. Loo, J. B. Lu, J. G. Lu, S. X. Lu, X. X. Lu, B. Lubsandorzhiev, S. Lubsandorzhiev, L. Ludhova, F. J. Luo, G. Luo, P. W. Luo, S. Luo, W. M. Luo, V. Lyashuk, Q. M. Ma, S. Ma, J. Maalmi, Y. Malyshkin, F. Mantovani, F. Manzali, X. Mao, Y. J. Mao, S. M. Mari, F. Marini, S. Marium, C. Martellini, G. Martin-Chassard, A. Martini, D. Mayilyan, A. Müller, I. Mednieks, A. Meregaglia, E. Meroni, D. Meyhöfer, M. Mezzetto, J. Miller, L. Miramonti, S. Monforte, P. Montini, M. Montuschi, N. Morozov, A. Muhammad, P. Muralidharan, M. Nastasi, D. V. Naumov, I. Nemchenok, F. P. Ning, Z. Ning, H. Nunokawa, L. Oberauer, J. P. Ochoa-Ricoux, D. Orestano, F. Ortica, H. R. Pan, A. Paoloni, N. Parkalian, S. Parmeggiano, T. Payupol, Y. Pei, N. Pelliccia, A. Peng, H. Peng, F. Perrot, P. A. Petitjean, F. Petrucci, L. F. P. Rico, O. Pilarczyk, A. Popov, P. Poussot, W. Pratumwan, E. Previtali, F. Qi, S. Qian, X. H. Qian, H. Qiao, Z. H. Qin, S. K. Qiu, M. Rajput, G. Ranucci, A. Re, H. Rebber, A. Rebii, B. Ren, T. Rezinko, B. Ricci, M. Robens, M. Roche, N. Rodphai, A. Romani, C. Roth, X. Ruan, S. Rujirawat, A. Rybnikov, A. Sadovsky, P. Saggese, G. Salamanna, S. Sanfilippo, A. Sangka, N. Sanguansak, U. Sawangwit, J. Sawatzki, F. Sawy, M. Schever, J. Schuler, C. Schwab, K. Schweizer, D. Selivanov, A. Selyunin, A. Serafini, G. Settanta, M. Settimo, Z. Shao, V. Sharov, J. Shi, V. Shutov, A. Sidorenkov, F. Simkovic, C. Sirignano, J. Siripak, M. Sisti, M. Slupecki, M. Smirnov, O. Smirnov, T. Sogo-Bezerra, J. Songwadhana, B. Soonthornthum, A. Sotnikov, O. Sramek, W. Sreethawong, A. Stahl, L. Stanco, K. Stankevich, D. Stefanik, H. Steiger, J. Steinmann, T. Sterr, M. R. Stock, V. Strati, A. Studenikin, G. X. Sun, S. F. Sun, X. L. Sun, Y. J. Sun, Y. Z. Sun, N. Suwonjandee, M. Szelezniak, J. Tang, Q. Tang, X. Tang, A. Tietzsch, I. Tkachev, A. Triossi, G. Troni, W. Trzaska, C. Tuve, N. Ushakov, S. van Waasen, J. V. Boom, G. Vanroyen, N. Vassilopoulos, V. Vedin, G. Verde, M. Vialkov, B. Viaud, C. Volpe, D. Voronin, L. Votano, P. Walker, C. Wang, E. Wang, G. Wang, K. Y. Wang, L. Wang, M. F. Wang, S. G. Wang, W. S. Wang, X. Y. Wang, Y. G. Wang, Y. Q. Wang, Z. Y. Wang, M. Waqas, A. Watcharangkool, W. Wei, Y. D. Wei, C. Wiebusch, S. C. F. Wong, B. Wonsak, D. Wu, Z. Wu, M. Wurm, J. Wurtz, C. Wysotzki, Y. F. Xi, Y. G. Xie, B. Xu, C. Xu, D. L. Xu, F. R. Xu, H. K. Xu, J. Xu, M. H. Xu, Y. Xu, B. J. Yan, T. Yan, W. Q. Yan, X. B. Yan, Y. P. Yan, A. B. Yang, H. Yang, J. Yang, X. Y. Yang, Y. Yang, Y. F. Yang, Z. Yasin, J. X. Ye, Z. P. Ye, U. Yegin, F. Yermia, P. H. Yi, X. W. Yin, Z. Y. You, B. X. Yu, C. Y. Yu, C. X. Yu, M. Yu, X. H. Yu, C. Z. Yuan, Y. Yuan, Z. X. Yuan, Z. Y. Yuan, N. Zafar, A. Zambanini, T. X. Zeng, Y. D. Zeng, G. Q. Zhang, H. Q. Zhang, J. Zhang, J. B. Zhang, P. Zhang, S. Zhang, T. Zhang, X. M. Zhang, Y. Zhang, Y. H. Zhang, Y. P. Zhang, F. Y. Zhao, R. Zhao, S. J. Zhao, T. C. Zhao, D. Q. Zheng, H. Zheng, M. S. Zheng, Y. H. Zheng, W. R. Zhong, J. Zhou, N. Zhou, S. Zhou, X. Zhou, J. Zhu, K. J. Zhu, B. Zhuang, L. Zong, B. C. Rasco, B. Y. Han, E. J. Jeon, Y. Jeong, H. S. Jo, D. K. Kim, J. Y. Kim, J. G. Kim, Y. D. Kim, Y. J. Ko, H. M. Lee, M. H. Lee, C. S. Moon, Y. M. Oh, H. K. Park, K. S. Park, S. H. Seo, K. Siyeon, G. M. Sun, Y. S. Yoon, I. Yu, M. J. Borusinski, R. Dorrill, A. Druetzler, J. Learned, V. Li, D. Markoff, J. Maricic, S. Matsuno, H. P. Mumm, K. Nishimura, A. Irani, M. Pitt, C. Rasco, B. Thibodeau, G. Varner, B. Vogelaar, T. Wright, M. Andriamirado, C. D. Bass, D. E. Bergeron, D. Berish, J. P. Brodsky, C. D. Bryan, T. Classen, G. Deichert, M. J. Dolinski, A. Erickson, B. T. Foust, J. K. Gaison, A. Galindo-Uribarri, C. E. Gilbert, C. Grant, B. T. Hackett, A. B. Hansell, X. Ji, D. C. Jones, O. Kyzylova, C. E. Lane, T. J. Langford, J. LaRosa, B. R. Littlejohn, X. Lu, M. P. Mendenhall, A. M. Meyer, R. Milincic, I. Mitchell, P. E. Mueller, C. Nave, R. Neilson, J. A. Nikkel, D. Norcini, S. Nour, J. L. Palomino, D. A. Pushin, E. Romero-Romero, P. T. Surukuchi, M. A. Tyra, R. L. Varner, D. Venegas-Vargas, P. B. Weatherly, C. White, J. Wilhelmi, A. Woolverton, A. Zhang, C. Zhang, J. H. Choi, H. I. Jang, J. S. Jang, S. H. Jeon, K. K. Joo, K. Ju, D. E. Jung, J. H. Kim, S. B. Kim, S. Y. Kim, W. Kim, E. Kwon, D. H. Lee, H. G. Lee, I. T. Lim, D. H. Moon, M. Y. Pac, H. Seo, J. W. Seo, C. D. Shin, B. S. Yang, J. Yoo, S. G. Yoon, I. S. Yeo, C. Chang, L. Bergé, A. Broniatowski, L. Dumoulin, A. Giuliani, M. Chapellier, P. De Marcillac, S. Marnieros, E. Olivieri, D. Poda, M. Calvo, J. Goupy, A. Monfardini, Q. Arnaud, C. Augier, J. Billard, A. Cazes, J. Colas, J. Filippini, J. Gascon, M. De Jesus, H. Lattaud, A. Juillard, T. Salagnac, T. Soldner, A. Lubashevskiy, E. Yakushev, S. Rozov, J. Lamblin, B. Mom, A. Stutz, J. A. Formaggio, D. W. Mayer, J. Johnston, P. Harrington, S. Heine, V. Sibille, R. Chen, E. Figueroa-Feliciano, H. Ziqing, S. Hertel, P. Patel, D. Pinckney, A. Serafin, A. Shilcusky, N. Decheine, K. Palladino, S. Weber, C. Hirjibehedin, N. S. Bowden, L. Carman, S. Dazeley, M. Ford, I. Jovanovic, F. Sutanto, N. Zaitseva, X. Zhang, W. Beaumont, S. Binet, I. Bolognino, J. Borg, V. Buridon, H. Chanal, B. Coupé, P. Crochet, D. Cussans, A. De Roeck, D. Durand, M. Fallot, D. Galbinski, S. Gallego, L. Giot, B. Guillon, D. Henaff, S. Hayashida, B. Hosseini, S. Kalcheva, G. Lehaut, I. Michiels, S. Monteil, D. Newbold, N. Roy, D. Ryckbosch, H. R. Sfar, L. Simard, A. Vacheret, G. Vandierendonck, S. Van Dyck, N. van Remortel, S. Vercaemer, M. Verstraeten, A. Weber, M. Yeresko, F. Yermia., A. Bonhomme, C. Buck, P. del Amo Sanchez, I. El Atmani, L. Labit, A. Letourneau, D. Lhuillier, M. Licciardi, T. Materna, H. Pessard, R. Rogly, V. Savu, M. Vialat, A. Algora, A. Beloeuvre, M. Estienne, R. Kean, A. Porta, J. L. Tain, I. Sidelnik, O. A. Akindele, T. Anderson, M. Askins, Z. Bagdasarian, A. Baldoni, A. Barna, T. Benson, M. Bergevin, A. Bernstein, B. Birrittella, S. Bogetic, J. Boissevain, J. Borusinki, S. Boyd, T. Brooks, M. Budsworth, J. Burns, M. Calle, C. Camilo, A. Carroll, J. Coleman, R. Collins, C. Connor, D. Cowen, B. Crow, J. Curry, F. Dalnoki-Veress, D. Danielson, M. Diwan, S. Dixon, L. Drakopoulou, J. Duron, S. Dye, S. Fargher, A. Fienberg, V. Fischer, R. Foster, K. Frankiewicz, T. Gamble, D. Gooding, S. Gokhale, R. Gregorio, J. Gribble, J. Griskevich, D. Hadley, J. He, K. Healey, J. Hecla, G. Holt, C. Jabbari, K. Jewkes, R. Kaiser, M. Keenan, P. Keener, L. Kneale, V. Kudryavtsev, P. Kunkle, P. Litchfield, X. R. Liu, G. Lynch, M. Malek, P. Marr-Laundrie, B. Masic, C. Mauger, N. McCauley, C. Metelko, R. Mills, A. Mitra, F. Muheim, A. Mullen, A. Murphy, M. Needham, E. Neights, K. Ogren, G. Orebi Gann, L. Oxborough, S. Paling, A. Papatyi, B. Paulos, T. Pershing, L. Pickard, S. Quillin, R. Resoro, B. Richards, L. Sabarots, A. Scarff, Y.-J. Schnellbach, P. Scovell, B. Seitz, O. Shea, V. Shebalin, G. Smith, M. Smy, H. Song, N. Spooner, C. Stanton, O. Stone, R. Svoboda, S. Szoldos, L. Thompson, F. Thomson, C. Toth, M. Vagins, R. Van Berg, S. Ventura, B. Walsh, J. Webster, M. Weiss, D. Westphal, M. Wetstein, T. Wilson, S. Wilson, S. Wolcott, M. Wright, J. I. Collar, A. Erlandson, S. Gariazzo, M. V. Garzelli, C. Giunti, B. L. Goldblum, A. Hayes, S. Hedges, C. Mariani, D. Minic, X. Mougeot, D. Naim, J. Newby, K. Ni, T. O'Donnell, S. Ozturk, L. Périssé, R. Pestes, A. A. Sonzogni, Z. Tabrizi, M. Vivier, J. Phys. G-Nucl. Partic, 51, Snowmass 2021 (2024) 080501, Seattle, United States, 17-26 Jul 2022
- White Paper on Light Sterile Neutrino Searches and Related Phenomenology, M. A. Acero, C. A. Argüelles, M. Hostert, D. Kalra, G. Karagiorgi, K. J. Kelly, B. R. Littlejohn, P. Machado, W. Pettus, M. Toups, M. Ross-Lonergan, A. Sousa, P. T. Surukuchi, Y. Y. Y. Wong, W. Abdallah, A. M. Abdullahi, R. Akutsu, L. Alvarez-Ruso, D. S. M. Alves, A. Aurisano, A. B. Balantekin, J. M. Berryman, T. Bertólez-Martínez, J. Brunner , M. Blennow, S. Bolognesi, M. Borusinski, T. Y. Chen, D. Cianci, G. Collin, J. M. Conrad, B. Crow, P. B. Denton, M. Duvall, E. Fernández-Martinez, C. S. Fong, N. Foppiani, D. V. Forero, M. Friend, A. García-Soto, C. Giganti, C. Giunti, R. Gandhi, M. Ghosh, J. Hardin, K. M. Heeger, M. Ishitsuka, A. Izmaylov, B. J. P. Jones, J. R. Jordan, N. W. Kamp, T. Katori, S. B. Kim, L. W. Koerner, M. Lamoureux, T. Lasserre, K. G. Leach, J. Learned, Y. F. Li, J. M. Link, W. C. Louis, K. Mahn, P. D. Meyers, J. Maricic, D. Marko, D. Markoff, T. Maruyama, S. Mertens, H. Minakata, I. Mocioiu, M. Mooney, M. H. Moulai, H. Nunokawa, J. P. Ochoa-Ricoux, Y. M. Oh, T. Ohlsson, H. Päs, D. Pershey, R. G. H. Robertson, S. Rosauro-Alcaraz, C. Rott, S. Roy, J. Salvado, M. Scott, S. H. Seo, M. H. Shaevitz, M. Smiley, J. Spitz, J. Stachurska, M. Tammaro, T. Thakore, C. A. Ternes, A. Thompson, S. Tseng, B. Vogelaar, T. Weiss, R. A. Wendell, R. J. Wilson, T. Wright, Z. Xin, B. S. Yang, J. Yoo, J. Zennamo, J. Zettlemoyer, J. D. Zornoza, J. Zupan, S. Ahmad, E. Arrieta-Diaz, V. S. Basto-Gonzalez, N. S. Bowden, B. C. Cañas, D. Caratelli, C. V. Chang, C. Chen, T. Classen, M. Convery, G. S. Davies, S. R. Dennis, Z. Djurcic, R. Dorrill, Y. Du, J. J. Evans, U. Fahrendholz, J. A. Formaggio, B. T. Foust, H. F. Gatti, D. Garcia-Gamez, S. Gariazzo, J. Gehrlein, C. Grant, R. A. Gomes, A. B. Hansell, F. Halzen, S. Ho, J. H. Zink, R. S. Jones, P. Kunkle, J.-Y. Li, S. C. Li, X. Luo, Y. Malyshkin, C. J. Martoff, D. Massaro, A. Mastbaum, R. Mohanta, H. P. Mumm, M. Nebot-Guinot, R. Neilson, K. Ni, J. Nieves, G. D. Orebi Gann, V. Pandey, S. Pascoli, G. Paz, A. A. Petrov, X. Qian, M. Rajaoalisoa, S. H. Razafinime, C. Roca, G. Ron, B. Roskovec, E. Saul-Sala, L. Saldaña, D. W. Schmitz, K. Scholberg, B. Shakya, P. L. Slocum, E. L. Snider, H. T. J. Steiger, A. F. Steklain, M. R. Stock, F. Sutanto, V. Takhistov, R. Tayloe, Y.-D. Tsai, Y.-T. Tsai, D. Venegas-Vargas, M. Wallbank, E. Wang, P. Weatherly, S. Westerdale, E. Worcester, W. Wu, G. Yang, B. Zamorano, J. Phys. G-Nucl. Partic, 51, Snowmass 2021 (2024) 120501, Seattle, United States, 17-26 Jul 2022
- Tau neutrino appearance measurement in KM3NeT/ORCA 6, C. Lastoria , PoS TAUP2023, 2023, 18th International Conference on Topics in Astroparticle and Underground Physics (2024) 192, Vienna, Austria, 28 Aug - 01 Sep 2023
- Art and Astrophysics in Conversation with KM3NeT Deep in the Mediterranean Sea, J. Mauro, D. Fortescue, G. de Wasseige, P. Coyle , A. Ilioni, PoS TAUP2023, 2023, 18th International Conference on Topics in Astroparticle and Underground Physics (2024) 332, Vienna, Austria, 28 Aug - 01 Sep 2023
- The DDRAGO wide-field imager for the COLIBRÍ telescope, R. Langarica, A. M. Watson, L. C. Álvarez Núñez, F. Ángeles, J.-L. Atteia, S. Basa, S. Cuevas, F. Dolon, A. Farah, D. Dornic , J. Floriot, J. Fuentes-Fernández, A. Langlois, W. H. Lee, S. Lombardo, M. Pereyra, J. Ruíz-Díaz-Soto, S. Ronayette, S. Tinoco, H. Valentín, Proc. SPIE, 13096, SPIE Astronomical Telescopes + Instrumentation 2024 (2024) 130963D, Yokohama, Japan, 16-21 Jun 2024
2023: 13 conference proceedings
- Oscillation physics with KM3NeT/ORCA, C. Lastoria , PoS NOW2022, 2022, Neutrino Oscillation Workshop 2022 (2023) 025, Ostuni, Brindisi, Italy, 4-11 Sep 2022
- Searching for neutrinos from Microquasar flares, S. Le Stum , PoS ICRC2023, IRN Neutrino meeting (2023), Nantes, France, 19-20 Jun 2023
- Particle identification in KM3NeT/ORCA, L. Cerisy , A. Lazo, C. Lastoria , M. Perrin-Terrin , J. Brunner , V. Dabhi , PoS ICRC2023, 2023, 38th International Cosmic Ray Conference (2023) 1191, Nagoya, Japan, 26 Jul - 03 Aug 2023
- Art and Astrophysics in Conversation with KM3NeT Deep in the Mediterranean Sea, D. Fortescue, G. de Wasseige, J. Mauro, P. Coyle , A. Ilioni, PoS ICRC2023, 2023, 38th International Cosmic Ray Conference (2023) 1621, Nagoya, Japan, 26 Jul - 03 Aug 2023
- Implementation of the KM3NeT Online Core-Collapse Supernova neutrino search, D. Dornic , C. Donzaud, S., El Hedri, V. Kulikovskiy, G. Vannoye, PoS ICRC2023, 2023, 38th International Cosmic Ray Conference (2023) 1223, Nagoya, Japan, 26 Jul - 03 Aug 2023
- Searching for Core-Collapse Supernova neutrinos at KM3NeT, I. Goos, S. El Hedri, C. Donzaud, M. Bendahman, V. Kulikovskiy, G. Vannoye , D. Dornic , PoS ICRC2023, 2023, 38th International Cosmic Ray Conference (2023) 1160, Nagoya, Japan, 26 Jul - 03 Aug 2023
- Follow-up of multi-messenger alerts with the KM3NeT ARCA and ORCA detectors, J. Palacios Gonzalez, S. Celli, D. Dornic , F. Filippini, E. Le Guirriec , J. de Favereau de Jeneret, G. Illuminati, M. Lamoureux, M. Mastrodicasa, R. Muller, F. Salesa Greus, A. Sánchez Losa, S. Le Stum , G. Vannoye , A. Veutro, A. Zegarelli, PoS ICRC2023, 2023, 38th International Cosmic Ray Conference (2023) 1521, Nagoya, Japan, 26 Jul - 03 Aug 2023
- Refined neutrino follow-up analysis of GRB 221009A with KM3NeT ARCA and ORCA detectors, J. Palacios Gonzalez, D. Dornic , F. Filippini, G. Illuminati, S. Le Stum , F. Salesa Greus, A. Sánchez Losa, G. Vannoye , A. Zegarelli, PoS ICRC2023, 2023, 38th International Cosmic Ray Conference (2023) 1503, Nagoya, Japan, 26 Jul - 03 Aug 2023
- The Real-time Analysis Platform of KM3NeT and its first results, S. Celli, P. Demin, D. Dornic , F. Filippini, E. Giorgio, E. Le Guirriec , J. de Favereau de Jeneret, M. Lamoureux, M. Mastrodicasa, J. Palacios Gonzalez, S. Le Stum , A.-J. Tanasijczuk, G. Vannoye , A. Veutro, A. Zegarelli, PoS ICRC2023, 2023, 38th International Cosmic Ray Conference (2023) 1125, Nagoya, Japan, 26 Jul - 03 Aug 2023
- Combined KM3NeT-ARCA and ANTARES searches for diffuse and point-like neutrino emission, D. Dornic , B. Caiffi, V. Kulikovskiy, V. Parisi, M. Sanguineti, S. Zavatarelli, S. Alves Garre, T. van Eeden", A. Heijboer, G. Illuminati, R. Muller, PoS ICRC2023, 2023, 38th International Cosmic Ray Conference (2023) 1147, Nagoya, Japan, 26 Jul - 03 Aug 2023
- Searching for neutrinos from microquasar flares with ANTARES and KM3NeT, S. Le Stum , D. Dornic , S. Alves Garre, PoS ICRC2023, 2023, 38th International Cosmic Ray Conference (2023) 1505, Nagoya, Japan, 26 Jul - 03 Aug 2023
- Combined KM3NeT-ARCA and ANTARES searches for diffuse and point-like neutrino emission, D. Dornic , B. Caiffi, V. Kulikovskiy, V. Parisi, M. Sanguineti, S. Zavatarelli, S. Alves Garre, T. van Eeden", A. Heijboer, G. Illuminati, R. Muller, PoS ICRC2023, 38th International Cosmic Ray Conference (2023), Nagoya, Japan, 26 Jul - 03 Aug 2023
- Follow-up of O3 gravitational wave events with neutrinos in ANTARES and KM3NeT telescopes, M. Lamoureux, D. Dornic , S. Le Stum , G. Vannoye , PoS ICRC2023, 2023, 38th International Cosmic Ray Conference (2023) 1506, Nagoya, Japan, 26 Jul - 03 Aug 2023
2022: 3 conference proceedings
- Status of the Real-time Multi-messenger Program of KM3NeT, Lincetto, M., Dornic, D., Huang, F., Schnabel, J., ASP Conf. Ser., 532, 30th Astronomical Data Analysis Software and Systems (2022) 147, Granada, Spain, 8-12 Nov 2020
- Future Neutrino Beam Studies Under the Framework of Physics Beyond Colliders, E.G. Parozzi, A. Baratto, J. Bernhard, M. Brugger, N. Charitonidis, A. Longhin, C. Mussolini, M. Pari, F. Pupilli, M. Perrin-Terrin , Y. Nagai, F. Terranovai, JACoW, IPAC2022, 13th International Particle Accelerator Conference (IPAC 2022) (2022) WEPOTK008, Bangkok, Thailand, 12-17 Jun 2022
- The GRANDMA network in preparation for the fourth gravitational-wave observing run, S. Agayeva, V. Aivazyan, S. Alishov, M. Almualla, C. Andrade, S. Antier, J.-M. Bai, A. Baransky, S. Basa, P. Bendjoya, Z. Benkhaldoun, S. Beradze, D. Berezin, U. Bhardwaj, M. Blazek, O. Burkhonov, E. Burns, S. Caudill, N. Christensen, F. Colas, A. Coleiro, W. Corradi, M. W. Coughlin, T. Culino, D. Darson, D. Datashvili, G. de Wasseige, T. Dietrich, F. Dolon, D. Dornic , J. Dubouil, J.-G. Ducoin, P.-A. Duverne, A. Esamdin, A. Fouad, F. Guo, V. Godunova, P. Gokuldass, N. Guessoum, E. Gurbanov, R. Hainich, E. Hasanov, P. Hello, T. Hussenot-Desenonges, R. Inasaridze, A. Iskandar, E. E. O. Ishida, N. Ismailov, T. Jegou du Laz, D. A. Kann, G. Kapanadze, S. Karpov, R. W. Kiendrebeogo, A. Klotz, N. Kochiashvili, A. Kaeouach, J.-P. Kneib, W. Kou, K. Kruiswijk, S. Lombardo, M. Lamoureux, N. Leroy, A. Le Van Su, J. Mao, M. Mašek, T. Midavaine, A. Möller, D. Morris, R. Natsvlishvili, F. Navarete, S. Nissanke, K. Noonan, K. Noysena, N. B. Orange, J. Peloton, M. Pilloix, T. Pradier, M. Prouza, G. Raaijmakers, Y. Rajabov, J.-P. Rivet, Y. Romanyuk, L. Rousselot, F. Rünger, V. Rupchandani, T. Sadibekova, N. Sasaki, A. Simon, K. Smith, O. Sokoliuk, X. Song, A. Takey, Y. Tillayev, I. T. e. Melo, D. Turpin, A. de Ugarte Postigo, M. Vardosanidze, X. F. Wang, D. Vernet, Z. Vidadi, J. Zhu, Y. Zhu, Proc. SPIE Int. Soc. Opt. Eng., 12186, SPIE Astronomical Telescopes + Instrumentation 2022 (2022) 121861H, Montréal, Canada, 17-22 Jul 2022
Talks
2024: 8 talks
- Galactic gamma-ray and neutrino emission from interacting cosmic-ray nuclei, M. Breuhaus , J. A. Hinton, V. Joshi, B. Reville, H. Schoorlemmer, Journées SF2A 2024, Marseille, France, 04-07 Jun 2024
- Astroparticle and oscillation research in the abyss with KM3NeT, P. Coyle , International Symposium on Neutrino Physics and Beyond (NPB 2024), Hong Kong, China, 19-21 Fev 2024
- Multi-messenger astronomy with KM3NeT, D. Dornic , IRN Neutrino Meeting, Palaiseau, France, 23-24 Mai 2024
- Multi-messenger astronomy with KM3NeT, D. Dornic , Journées SF2A 2024, Marseille, France, 04-07 Jun 2024
- Future atmospheric neutrino detectors, J. Brunner , XXXI International Conference on Neutrino Physics and Astrophysics (Neutrino 2024), Milan, Italy, 16-22 Jun 2024
- The status of the KM3NeT neutrino telescope, P. Coyle , 42nd International Conference on High Energy Physics (ICHEP 2024), Prague, Czech Republic, 18-24 Jul 2024
- Undersea measurements of neutrino oscillations (KM3NeT), L. Cerisy , Neutrino Oscillation Workshop (NOW 2024), Otranto, Italy, 02-08 Sep 2024
- KM3NeT alerts system, J.-G. Ducoin , 3rd Astro-COLIBRI multi-messenger astrophysics workshop, Paris, France, 16-20 Sep 2024
2023: 7 talks
- Status of KM3NeT, P. Coyle , Workshop Multi-Aspect Young ORiented Advanced Neutrino Academy (MAYORANA), Modica, Italy, 12-14 Jul 2023
- Experimental proof of principle of the Neutrino Tagging technique at NA62, B. De Martino , M. Perrin-Terrin , The 24th International Workshop on Neutrinos from Accelerators (NuFACT 2023), Seoul, South Korea, 20-26 Aug 2023
- Tau neutrino appearance measurement in KM3NeT/ORCA6, C. Lastoria , XVIIIth International Conference on Topics in Astroparticle and Underground Physics (TAUP 2023), Vienna, Austria, 28 Aug - 01 Sep 2023
- Results from Tau neutrino appearance from KM3NeT/ORCA, L. Cerisy , IRN Neutrino Meeting, Karlsruhe, Allemagne, 27-28 Nov 2023
- First evidence for neutrino tagging, B. De Martino , IRN Neutrino Meeting, Karlsruhe, Allemagne, 27-28 Nov 2023
- Astroparticle and oscillation results from KM3NeT, P. Coyle , NuPhys2023: Prospects in Neutrino Physics, London, United Kingdom, 18-20 Dec 2023
- Neutrino tagging, M. Perrin-Terrin , NuPhys2023: Prospects in Neutrino Physics, London, United Kingdom, 18-20 Dec 2023
2022: 12 talks
- Real-time multi-messenger analysis framework of KM3NeT, D. Dornic , Low-latency alerts & Data analysis for Mumti-messenger Astrophysics, Paris, France, 13-14 Jan 2022
- Multi-Messenger Observations with Neutrinos, D. Dornic , 12th CosPa meeting : Multi-Messenger Sources and Observations, Louvain-la-Neuve, Belgium, 21 Apr 2022
- Multi channel high energy neutrino observations, D. Dornic , Bursting Universe by Robots Eyes 2022, Online, indéfini, 15-20 Aug 2022
- Oscillation physics with KM3NeT/ORCA, C. Lastoria , Neutrino Oscillation Workshop 2022, Ostuni, Brindisi, Italy, 4-11 Sep 2022
- KM3NeT : Astroparticles and oscillations research with cosmics in the Abyss, P. Coyle , Town Hall KM3NeT Meeting, Catania, Italy, 20-22 Sep 2022
- Return of experience of the ANTARES online framework and description of the KM3NeT real-time architecture, D. Dornic , Town Hall KM3NeT Meeting, Catania, Italy, 20-22 Sep 2022
- Neutrino alert system of KM3NeT, G. Vannoye , Town Hall KM3NeT Meeting, Catania, Italy, 20-22 Sep 2022
- Real-time correlation analysis with KM3NeT, S. Le Stum , Town Hall KM3NeT Meeting, Catania, Italy, 20-22 Sep 2022
- High-energy neutrinos and multi-messenger astronomy, D. Dornic , International conference PUMA22 Probing the Universe with Multimessenger Astrophysics, Sestri Levante, Italy, 26-30 Sep 2022
- KM3NeT open science programs, D. Dornic , Astrophysique des Hautes Energies dans l'Observatoire Virtuel, Strasbourg, France, 11 Oct 2022
- Observation of the cosmic ray shadow of Moon and Sun with 6 lines of KM3Net/ORCA, L. Cerisy , IRN Neutrino Meeting, Orsay, France, 16-17 Nov 2022
- Neutrino alerts and follow-up challenges, D. Dornic , Neutrinos in the Multi-Messenger Era, Louvain-la-Neuve, Belgium, 29 Nov - 2 Dec 2022
Posters
2024: 3 posters
- Non unitary neutrino mixing with KM3NeT/ORCA, L. Cerisy , XXXI International Conference on Neutrino Physics and Astrophysics (Neutrino 2024), Milan, Italy, 16-22 Jun 2024
- KM3NeT’s sensitivity to the next core-collapse supernova, S. El Hedri, I. Goos, C. Donzaud, G. Vannoye , XXXI International Conference on Neutrino Physics and Astrophysics (Neutrino 2024), Milan, Italy, 16-22 Jun 2024
- Experimental proof of principle of the Neutrino Tagging technique at NA62, L. Petit , XXXI International Conference on Neutrino Physics and Astrophysics (Neutrino 2024), Milan, Italy, 16-22 Jun 2024
2023: 9 posters
- Searching for Core-Collapse Supernova neutrinos at KM3NeT, I. Goos, S. El Hedri, C. Donzaud, M. Bendahman, V. Kulikovskiy, G. Vannoye , D. Dornic , 38th International Cosmic Ray Conference, Nagoya, Japan, 26 Jul - 03 Aug 2023
- Implementation of the KM3NeT Online Core-Collapse Supernova neutrino search, D. Dornic , C. Donzaud, S., El Hedri, V. Kulikovskiy, G. Vannoye , 38th International Cosmic Ray Conference, Nagoya, Japan, 26 Jul - 03 Aug 2023
- Refined neutrino follow-up analysis of GRB 221009A with KM3NeT ARCA and ORCA detectors, J. Palacios Gonzalez, D. Dornic , F. Filippini, G. Illuminati, S. Le Stum , F. Salesa Greus, A. Sánchez Losa, G. Vannoye , A. Zegarelli, 38th International Cosmic Ray Conference, Nagoya, Japan, 26 Jul - 03 Aug 2023
- Searching for neutrinos from microquasar flares with ANTARES and KM3NeT, S. Le Stum , D. Dornic , S. Alves Garre, 38th International Cosmic Ray Conference, Nagoya, Japan, 26 Jul - 03 Aug 2023
- Follow-up of multi-messenger alerts with the KM3NeT ARCA and ORCA detectors, J. Palacios Gonzalez, S. Celli, D. Dornic , F. Filippini, E. Le Guirriec , J. de Favereau de Jeneret, G. Illuminati, M. Lamoureux, M. Mastrodicasa, R. Muller, F. Salesa Greus, A. Sánchez Losa, S. Le Stum , G. Vannoye , A. Veutro, A. Zegarelli, 38th International Cosmic Ray Conference, Nagoya, Japan, 26 Jul - 03 Aug 2023
- Particle identification in KM3NeT/ORCA, L. Cerisy , A. Lazo, C. Lastoria , M. Perrin-Terrin , J. Brunner , V. Dabhi , 38th International Cosmic Ray Conference, Nagoya, Japan, 26 Jul - 03 Aug 2023
- Art and Astrophysics in Conversation with KM3NeT Deep in the Mediterranean Sea, D. Fortescue, G. de Wasseige, J. Mauro, P. Coyle , A. Ilioni, 38th International Cosmic Ray Conference, Nagoya, Japan, 26 Jul - 03 Aug 2023
- Follow-up of O3 gravitational wave events with neutrinos in ANTARES and KM3NeT telescopes, M. Lamoureux, D. Dornic , S. Le Stum , G. Vannoye , 38th International Cosmic Ray Conference, Nagoya, Japan, 26 Jul - 03 Aug 2023
- The Real-time Analysis Platform of KM3NeT and its first results, S. Celli, P. Demin, D. Dornic , F. Filippini, E. Giorgio, E. Le Guirriec , J. de Favereau de Jeneret, M. Lamoureux, M. Mastrodicasa, J. Palacios Gonzalez, S. Le Stum , A.-J. Tanasijczuk, G. Vannoye , A. Veutro, A. Zegarelli, 38th International Cosmic Ray Conference, Nagoya, Japan, 26 Jul - 03 Aug 2023
2022: 8 posters
- Tagged neutrino beams, B. De Martino , M. Perrin-Terrin , XXX International Conference on Neutrino Physics and Astrophysics (Neutrino 2022), Seoul, Korea, 30 May - 04 Jun 2021
- Monitoring the neutrino sky for the next Galactic Core-Collapse Supernova with KM3NeT, D. Dornic , V. Kulikovskiy, G. Vannoye , XXX International Conference on Neutrino Physics and Astrophysics (Neutrino 2022), Seoul, Korea, 30 May - 04 Jun 2021
- First search for neutrino counterparts from gravitational wave sources with KM3NeT/ORCA, D. Dornic , F. Huang , M. Lamoureux, S. Le Stum , G. Vannoye , G. De Wasseige, XXX International Conference on Neutrino Physics and Astrophysics (Neutrino 2022), Seoul, Korea, 30 May - 04 Jun 2021
- Online Multi-Messenger Program of KM3NeT, W. Assal , S. Celli, J. De Favereau de Jeneret, P. Demin, D. Dornic , F. Huang , V. Kulikovskiy, E. Le Guirriec , S. Le Stum , A. J. Tanasijczuk, H. Tedjditi, G. Vannoye , A. Zegarelli, XXX International Conference on Neutrino Physics and Astrophysics (Neutrino 2022), Seoul, Korea, 30 May - 04 Jun 2021
- Measurement of neutrino oscillations with KM3NeT/ORCA, Z. Aly , XXX International Conference on Neutrino Physics and Astrophysics (Neutrino 2022), Seoul, Korea, 30 May - 04 Jun 2021
- The online multi-messenger program of KM3NeT, G. Vannoye , Neutrinos in the Multi-Messenger Era, Louvain-la-Neuve, Belgium, 29 Nov - 2 Dec 2022
- Monitoring the neutrino sky for the next galactic core-collapse supernova with KM3NeT, G. Vannoye , Neutrinos in the Multi-Messenger Era, Louvain-la-Neuve, Belgium, 29 Nov - 2 Dec 2022
- Subsea observatories: Improvement on the deployment, position accuracies and communication to the surface, N. Olivier, P.-F. Adam, L. Bazin, V. Bertin , M.-N. Fabre , AGU (American Geophysical Union) Fall Meeting 2022, Chicago, United States, 12-16 Dec 2022
Report
2022: 1 report
- Moon and Sun shadow with ORCA6, L. Cerisy et al. , KM3NeT Collaboration, KM3NeT_CALIB_2022_001
Mémoires
2024: 1 mémoire
-
First tau neutrino appearance, non-unitary mixing and absolute orientation measurements in KM3NeT, L. Cerisy, Aix-Marseille Université, 25 Nov 2024
2023: 3 mémoires
-
Mesure de la hiérarchie de masse des neutrinos avec le détecteur KM3NeT/ORCA, Z. Aly, Aix-Marseille Université, 06 Oct 2023
-
Experimental proof of principle of the Neutrino Tagging at NA62, B. De Martino, Aix-Marseille Université, 10 Nov 2023
-
Recherche d'émission gamma de très haute énergie et de neutrinos venant de microquasars avec HESS et ANTARES / KM3NeT, S. Le Stum, Aix-Marseille Université, 15 Dec 2023
2022: 1 mémoire
-
Acoustic positioning systems and passive acoustic monitoring of cetaceans with the KM3NeT underwater neutrino telescope, C. Guidi, Université de Genoa, Aix-Marseille Université, 25 Jan 2022
- February 2025: Publication in the Nature revue of the detection of a neutrino with an energy estimated to 220 PeV, observed with the KM3NeT-ARCA detector on 13/02/2023. This neutrino has an energy 30 times larger that the one of all neutrinos previously detected worldwide.
- February 2025: Damien Dornic, physicist at CPPM, is nominated Deputy-Spokesman of the KM3NeT Collaboration for 2 years.
- Octobre 2024: Publication of the first measurement of the oscillation neutrino parameters with the data of the 6 first lines of the KM3NeT/ORCA detector, with a major contribution of the CPPM team.
- Octobre 2024: Installation of a new detection line and calibration instruments on the KM3NeT/ORCA site, as well as new detection lines on the KM3NeT/ARCA site. These detectors are now composed of 24 lines for ORCA and 33 lines for ARCA in continuous data taking.
- June 2024: First images of the COLIBRI robotic telescope taken with its visible camera, following its final installation définitive at San Pedro Martir Observatory in Baja California (Mexico).
- 22 June 2024: Launching in orbit of the SVOM satellite, the French-Chinese mission specialized on the study of gamma ray bursts.
- June 2024: Installation of 4 new detection lines on the KM3NeT/ORCA site. This detector is now composed of 23 lines in continuous data taking.
- September-October 2023: Presentation of more than 20 years of submarine research of neutrinos with ANTARES and KM3NeT at the exhibition "Des abysses au Cosmos" at Fort Napoléon in La Seyne sur Mer
- September 2023: Installation of new detection lines on the KM3NeT/ARCA site. This detector is now composed of 28 lines in continuous data taking.
- June 2023: After a test campaign at the Observatoire de Haute-Provence, the COLIBRI telescope is sent to Mexico for its final installation at San Pedro Martir Observatory in Baja California (Mexico).
- April 2023: Installation of 3 new detection lines on the KM3NeT/ORCA site. This detector is now composed of 18 lines in continuous data taking.
- December 2022: The Prize for Research 2022 of the Bouches-du-Rhône Department was awarded to the astroparticle neutrino team.
- December 2022: Installation of 4 new detection lines on the KM3NeT/ORCA site. This detector now comprises 15 deployed lines with more than 7500 photomultipliers.
- September 2022: Installation of new detection lines on the KM3NeT/ARCA site. This detector is now composed of 21 lines in continuous data taking.
- June 2022: New major step of the detector dismantling operation by the recovery of all detection lines. Only the junction box and its main linking cable to shore stay on the submarine site.
- February 2022: Definitive stop of the ANTARES detector operation, after 16 years of continuous data taking. During a first step of the dismantling operations of the detector, all cables linking the lines to the principal Junction Box have been unplugged.
- November 2021: Installation of 4 new detection lines on the KM3NeT/ORCA site. This detector is now composed of 10 lines in continuous data taking.
- September 2021: Installation of 2 new detection lines on the KM3NeT/ARCA site. This detector is now composed of 8 lines in continuous data taking.
- April 2021: Installation of a new junction box and 5 new detection lines on the KM3NeT/ARCA site. With 6 ORCA lines and 6 ARCA lines in operation, KM3NeT has now a sensitivity comparable as the one of ANTARES for the detection of neutrinos.
- March 2021: Publication of the sensitivity on the determination of the neutrino mass ordering and measurements of oscillation parameters with KM3NeT/ORCA, which CPPM is main author.
- February 2021: Paschal Coyle, physicist at CPPM, is nominated Spokesman of the KM3NeT Collaboration for 2 years.
- February 2021: Publication of the sensitivity on the detection of core-collapse supernovae neutrinos with KM3NeT, which CPPM is main author.
- October 2020: Deployment and connection of the Node2 of the MEUST/NUMerEnv/LSPM submarine infrastructure.
- Summer 2020: The integration of the Germanium detector, aimed to study the radioactivity in the deep sea on the MEUST/NUMerEnv site, is completed and the detector is currently under tests and calibration in the Prisna plateforme in Bordeaux.
- Spring 2020: Despite the confinement imposed by the sanitary crisis, the permanent data taking of the ANTARES and KM3NeT/ORCA detectors is carried on.
- April 2020: Labellisation of the submarine infrastructure MEUST/NUMerEnv as a national scientific platform oriented towards research and scientific culture, the Laboratoire Sous-Marin de Provence Méditerranée.
- March 2020: KM3NeT is now contributing to the alert network SNEWS for the detection of supernovae.
- February 2020: The Node2 of the MEUST/NUMerEnv submarine infrastructure is ready and transferred to La Seyne-sur-Mer to prepare its deployment.
- January 2020: Installation of two new lines of the KM3NeT/ORCA detector which is now taking data continuously with 6 detection lines.
- November 2019: First real-time follow-up of a multi-messenger alert (gravitational wave S191110af) with KM3NeT and publication of its first circular (GCN #26249).
- July 2019: Installation of two new lines of the KM3NeT/ORCA detector which is now taking data continuously with 4 detection lines.
- June 2019: Delivery of the COLIBRI telescope structure at the Observatoire de Haute Provence.
- June 2019: Publication of the first KM3NeT analysis paper (Dependence of atmospheric muon flux on seawater depth measured with the first KM3NeT detection units) with a major contribution from CPPM.
- June 2019: Ceremony of the new CNRS Cristal Collectif award delivered to the CPPM technical team for the development and the construction of the MEUST/NUMerEnv submarine infrastructure.
- May 2019: Publication by the newspaper Le Monde of the video by CNRS Images Pêcheurs de neutrinos on the construction of KM3NeT/ORCA.
- May 2019: Installation of a new line of the KM3NeT/ORCA detector which is now taking data continuously with 2 detection lines, installation of the oceanographic module MII.
- February 2019: Installation and operation of the first line of the KM3NeT/ORCA detector.
- January 2019: Launch of the LIA ERIDANUS between France (CNRS, CNES and AMU) and Mexico (UNAM and CONACyT) to form a strong scientific community on the scientific cases of SVOM.
- January 2019: Publication of the Letter of Interest for the Protvino-to-ORCA project (P2O) with a neutrino beam to measure the CP violation phase in the neutrino sector.
- December 2018: Publication of the new analysis on the measurement of the neutrino oscillation parameters with ANTARES.
- October 2018: Repair of the main electro-optical cable linking the MEUST/NUMerEnv infrastructure to shore and reinstallation of the Node1 of the infrastructure.
- May 2018: First stone for the construction of the observatory at the National Astronomical Observatory in Mexico which will host the COLIBRI telescope.
- May 2018: 10th anniversary of the completion of the ANTARES detector.
- January 2018: Reconnection of the ANTARES line L6 thanks to an operation of the submarine Nautile of Ifremer.
- October 2017: Publication of the participation by ANTARES to the follow-up of the coalescence of two neutron stars GW170817 detected by LIGO/Virgo.
- September-December 2017: Operation of the 1st KM3NeT/ORCA detection line and observation of the first neutrino candidates.
- July 2017: Repair of the main cable of the MEUST/NUMerEnv infrastructure and redeployment of the Node1
- October 2016: publication of the SVOM white paper (The Deep and Transient Universe in the SVOM Era: New Challenges and Opportunities - Scientific prospects of the SVOM mission)
- 2016: Extension of the TAToO alert network to the gamma observatories HESS and HAWC and to the radio antenna network MWA Murchinson
- January 2016: Publication of the Letter of Intent for KM3NeT 2.0 detailing the sensitivities of the KM3NeT/ORCA detector for the determination of the neutrino mass hierarchy
- December 2015: Start of the participation to the SVOM project in order to increase the follow-up potential of KM3NeT neutrino alerts
- September 2015: Start of the robotic telescope COLIBRI project
- May 2015: Installation of the Node1 of the MEUST/NUMerEnv submarine infrastructure
- 2015: Beginning of the NUMerEnv project, phase 2 of the MEUST project, for the development of the submarine infrastructure, the KM3NeT/ORCA detector and the addition of various environmental sensors
- December 2014: Deployment of the main electro-optical cable of the MEUST submarine infrastructure
- 2014: Development of the online analysis of ANTARES data for the search of neutrinos coming from astrophysical transient sources
- 2013: Extension of the TAToO alert network to the X-Rays satellite Swift
- 2010: Beginning of the MEUST project for the development of a submarine infrastructure to host the KM3NeT-France detector and Earth and Sea Sciences sensors within the framework of the seabed observatories EMSO
- 2009: Development and operation of the TAToO alert network for the optical follow-up of high energy neutrinos detected by ANTARES
- May 2008: End of construction of the ANTARES detector equipped with 12 neutrino detection lines and an instrumentation line
- February 2006: Deployment of the first line of the ANTARES detector
The videos presented are dedicated to the study of neutrinos in the marine environment and were produced to coincide with the ‘From the Abyss to the Cosmos’ exhibition at fort Napoléon in La Seyne-sur-Mer, from 14 September to 8 October 2023. The videos are divided into four series: the ANTARES project, the KM3NeT project, neutrinos and marine technologies.
The ANTARES project:
The ANTARES detector was the largest neutrino telescope in the northern hemisphere and the first to be built in a marine environment. Operating between 2006 and 2022, it was installed at a depth of 2.500 m, 40 km off the coast of Toulon (France). The main aim of ANTARES was to search for cosmic neutrinos originating from violent phenomena in the Universe. The ANTARES underwater infrastructure also provided a multi-disciplinary platform for experimentation, enabling a wide range of studies to be carried out in the fields of marine, earth and environmental sciences.
Presentation of the ANTARES project, by Antoine Kouchner, Researcher at APC | Production CPPM 2023
The origins of the ANTARES project, by Patrick Lamare, Technical Manager of ANTARES at CEA | Production CPPM 2023
t Why an underwater detector offshore from La Seyne-sur-Mer? By Vincent Bertin, Researcher at CPPM | Production CPPM 2023
Detecting neutrinos with ANTARES, by José Busto, Researcher at CPPM | Production CPPM 2023
How is an ANTARES detection line built? By Jérôme Laurence, Assistant Engineer at CPPM | Production CPPM 2023
How can ANTARES sensors be synchronised? By Frédéric Rhétoré, Engineer at CPPM | Production CPPM 2023
How to position the detection lines of the ANTARES telescope? By an Engineer at CPPM | Production CPPM 2023
How do you interface a detector at the bottom of the sea? By Michel Ageron, Engineer at CPPM | Production CPPM 2023
Why was the Michel Pacha Institute the control room for ANTARES? By Paschal Coyle, Researcher at CPPM | Production CPPM 2023
The main results of the ANTARES experiment, by Antoine Kouchner, Researcher at APC | Production CPPM 2023
The KM3NeT project:
The KM3NeT detector is a second-generation neutrino telescope installed in the Mediterranean abyss, designed using feedback from the ANTARES detector. A first version of the detector, called ARCA, installed off the coast of Sicily, is dedicated to the search for high-energy neutrinos coming from cataclysms in the Universe such as supernovae or the formation and evolution of black holes. A second detector, called ORCA, is under construction off the coast of Toulon. It will be used to determine the mass hierarchy of neutrinos, by precisely studying the flux of atmospheric neutrinos passing through the Earth. The ORCA detector's MEUST-NUMerEnv underwater infrastructure will also serve as a multi-disciplinary experimental platform for a wide range of studies in the fields of marine, earth and environmental sciences, as part of the EMSO seabed observatory.
What is the KM3NeT project? By Paschal Coyle, Researcher at CPPM | Production CPPM 2023
How to finance an international collaboration? By Victoria Ciarlet, Project Manager at CPPM | Production CPPM 2023
How is the KM3NeT detector being built? By Nick Lumb, Engineer at CPPM | Production CPPM 2023
The construction of a KM3NeT detection line, by Aurélien Marini, Head of KM3NeT line integration at CPPM | Production CPPM 2023
Deployment of KM3NeT lines at sea, by Sylvain Henry, Engineer at CPPM | Production CPPM 2023
Data transmission from the KM3NeT detector, by Evelyne Garçon, Engineer at CPPM | Production CPPM 2023
The power supply system of the KM3NeT detector, by Stéphane Théraube, Engineer at CPPM | Production CPPM 2023| Production CPPM 2023
How can data be recovered from the seabed? By Thomas Auphan, Engineer at CPPM| Production CPPM 2023
How to analyse the data flow from the KM3NeT detector in real time? By Emmanuel Le Guirriec, Engineer at the CPPM | Production CPPM 2023
Neutrinos:
The CPPM has a scientific team specialising in cosmic neutrino research and the study of the fundamental properties of neutrinos. These particles are studied using underwater detectors, installed at a depth of 2.500 metres in the deep Mediterranean Sea, off the coast of Toulon: ANTARES and its successor KM3NeT.
What is a neutrino? By Luc Cerizy, PhD student at CPPM | Production CPPM 2023
** The history of neutrinos, by José Busto, Researcher at CPPM | Production CPPM 2023
Neutrino oscillation, by Chiara Lastoria, Researcher at CPPM | Production CPPM 2023
The properties of neutrinos, by Matthieu Perrin-Terrin, Researcher at CPPM | Production CPPM 2023
How can neutrinos be detected at the bottom of the sea? By Jürgen Brunner, Engineer at CPPM | Production CPPM 2023
What are the sources of neutrinos in the Universe? By Sébastien Le Stum, PhD student at CPPM | Production CPPM 2023
The search for Dark Matter with neutrinos, by Vincent Bertin, Researcher at the CPPM | Production CPPM 2023
Surpernova et neutrinos, par Godefroy Vannoye, Doctorant au CPPM| Production CPPM 2023
The astronomy of the 21st century, by Damien Dornic, Researcher at the CPPM | Production CPPM 2023
Underwater technologies:
As part of the ANTARES and KM3NeT projects, the CPPM has developed a wide range of technological skills for the installation of a neutrino detector in the Mediterranean abyss, at a depth of 2.500 metres. These skills range from the design and manufacture of a telescope capable of withstanding the environmental constraints of the deep marine environment, to carrying out operations at sea and underwater to deploy the scientific instruments.
The challenges involved in designing an underwater sensor, by a CPPM engineer | Production CPPM 2023
What materials should be chosen to operate a detector deep under the sea? By Alain Cosquer, Engineer at CPPM | Production CPPM 2023
Designing a pressure-resistant detector, by Michel Billault, Engineer at CPPM | Production CPPM 2023
The stages in the design of an underwater telescope, by Christophe Lerouvillois, Project Designer at CPPM | Production CPPM 2023
How do you ensure the reliability of an inaccessible detector? By Laurence Caillat, Engineer at CPPM | Production CPPM 2023
Installing a detector on the seabed, by Jean Roux, Head of Offshore Operations for CNRS | Production CPPM 2023
How do you carry out underwater operations? By Stéphane Roubaud, Head of subsea operations at SAAS/Comex | Production CPPM 2023
Deploying a sensor at sea, by Bernard Corbasson, Captain at FOSELEV Marine | Production CPPM 2023
How do you install a high-speed communications network on the seabed? By Cyril Defais, Head of Operations at Orange Marine | Production CPPM 2023
Why use underwater robots? By Jean-François Drogou, Engineer at Ifremer | Production CPPM 2023
How do you position objects in the abyss? By Marie-Noëlle Fabre, Engineer at Exail | Production CPPM 2023
How do you position objects in the abyss? By Marie-Noëlle Fabre, Engineer at Exail | Production CPPM 2023
Photons
CTAO (Cherenkov Telescope Array Observatory) is a global initiative to build the world’s largest and most sensitive high-energy gamma-ray observatory. It will be constituted by more than 100 Imaging Air Cherenkov Telescopes (IACTs) of three different types (Large, Medium and Small Sized Telescopes) located both in the northern and southern hemispheres. CTA will detect high-energy radiation with unprecedented accuracy and approximately 10 times better sensitivity than current IACT instruments such as HESS.
CTAO will transform our understanding of the high-energy Universe by addressing three major study themes: understanding the origin and role of relativistic cosmic particles, probing extreme environments such as black holes and exploring the frontiers of physics searching for dark matter and deviations from Einstein’s theory of special relativity.
The CPPM participates both to CTA and to H.E.S.S. and has responsabilities in the following domains:
- Acquisition system for the Large and Medium Sized Telescopes (NectarCAM and LSTCAM)
- Monte Carlo Simulation and verification
- Offline calibration of the large sized telescopes (LST)
- Evaluation of CTA potentiality in detecting galactic cosmic ray sources
- Galactic target of opportunity program in H.E.S.S.
Researchers and Research professors
- Heide Costantini (team responsible)
- Jean-Pierre Ernenwein
- Lorenzo Feligioni
Engineers and Technicians
- William Assal, Detectors and Data department
- Franca Cassol, Detectors and Data department
- Dirk Hoffmann, Detectors and Data department (technical responsible)
- Julien Houles, Detectors and Data department
Post-docs
PhD students
Apprentices
Publications Astronomie gamma
Articles
2025: 1 article
- Detection of very-high-energy gamma-ray emission from Eta Carinae during its 2020 periastron passage, F. Aharonian et al. , HESS Collaboration, Astron. Astrophys. 694 (2025) A328
2024: 19 articles
- Prospects for -ray observations of the Perseus galaxy cluster with the Cherenkov Telescope Array, K. Abe et al. , CTA Consortium Collaboration, J. Cosmol. Astropart. P 10 (2024) 004
- Prospects for -ray observations of the Perseus galaxy cluster with the Cherenkov Telescope Array, K. Abe et al. , CTA Consortium Collaboration, J. Cosmol. Astropart. P 10 (2024) 004
- Prospects for a survey of the Galactic plane with the Cherenkov Telescope Array, S. Abe et al. , CTA Consortium Collaboration, J. Cosmol. Astropart. P 10 (2024) 081
- TeV flaring activity of the AGN PKS 0625-354 in November 2018, F. Aharonian et al. , HESS Collaboration, Astron. Astrophys. 683 (2024) A70
- Acceleration and transport of relativistic electrons in the jets of the microquasar SS 433, F. Aharonian et al. , HESS Collaboration, Science 383 (2024) nan-nan
- Curvature in the very-high energy gamma-ray spectrum of M87, F. Aharonian et al. , HESS Collaboration, Astron. Astrophys. 685 (2024) A96
- Dark Matter Line Searches with the Cherenkov Telescope Array, S. Abe et al. , J. Cosmol. Astropart. P 07 (2024) 047
- Dark Matter Line Searches with the Cherenkov Telescope Array, S. Abe et al. , CTA Consortium Collaboration, J. Cosmol. Astropart. P 07 (2024) 047
- Dark Matter Line Searches with the Cherenkov Telescope Array, S. Abe et al. , J. Cosmol. Astropart. P 07 (2024) 047
- Spectrum and extension of the inverse-Compton emission of the Crab Nebula from a combined Fermi-LAT and H.E.S.S. analysis, F. Aharonian et al. , HESS Collaboration, Astron. Astrophys. 686 (2024) A308
- Unveiling extended gamma-ray emission around HESS J1813-178, F. Aharonian et al. , HESS Collaboration, Astron. Astrophys. 686 (2024) A149
- Broadband Multi-wavelength Properties of M87 during the 2018 EHT Campaign including a Very High Energy Flaring Episode, J. C. Algaba et al. , Astron. Astrophys. 692 (2024)
- Broadband Multi-wavelength Properties of M87 during the 2018 EHT Campaign including a Very High Energy Flaring Episode, J. C. Algaba et al. , Astron. Astrophys. 692 (2024) A140
- H.E.S.S. observations of the 2021 periastron passage of PSR B1259-63/LS 2883, F. Aharonian et al. , HESS Collaboration, Astron. Astrophys. 687 (2024) A219
- A detailed study of the very-high-energy Crab pulsar emission with the LST-1, K. Abe et al. , CTA Consortium Collaboration, Astron. Astrophys. 690 (2024) A167
- Very-high-energy -ray emission from young massive star clusters in the Large Magellanic Cloud, F. Aharonian et al. , HESS Collaboration, Astrophys. J 970 (2024) L21
- A new method of reconstructing images of gamma-ray telescopes applied to the LST-1 of CTAO, K. Abe et al. , CTA Consortium Collaboration, Astron. Astrophys. 691 (2024) A328
- Multi-wavelength study of OT 081: broadband modelling of a transitional blazar, H. Abe et al. , HESS Collaboration, Mon. Not. Roy. Astron. Soc (2024)
- High-Statistics Measurement of the Cosmic-Ray Electron Spectrum with H.E.S.S, F. Aharonian et al. , HESS Collaboration, Phys. Rev. Lett 133 (2024) 221001
2023: 11 articles
- Multi-wavelength study of the galactic PeVatron candidate LHAASO J2108+5157, S. Abe et al. , CTA Consortium Collaboration, Astron. Astrophys. 673 (2023) A75
- HESS J1809 193: a halo of escaped electrons around a pulsar wind nebula?, F. Aharonian et al. , HESS Collaboration, Astron. Astrophys. 672 (2023) A103
- Search for the evaporation of primordial black holes with H.E.S.S, F. Aharonian et al. , HESS Collaboration, J. Cosmol. Astropart. P 04 (2023) 040
- Sensitivity to point-like sources of the ALTO atmospheric particle detector array, designed for 200 GeV–50 TeV -ray astronomy, M. Punch et al. , J. High Energy Astron. Phys 39 (2023) 1-13
- Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants, F. Acero et al. , CTA Consortium Collaboration, Astropart. Phys. 150 (2023) 102850
- Detection of extended gamma-ray emission around the Geminga pulsar with H.E.S.S, F. Aharonian et al. , HESS Collaboration, Astron. Astrophys. 673 (2023) A148
- Constraining the cosmic-ray pressure in the inner Virgo Cluster using H.E.S.S. observations of M 87, F. Aharonian et al. , HESS Collaboration, Astron. Astrophys. 675 (2023) A138
- Sensitivity of the Cherenkov Telescope Array to TeV photon emission from the Large Magellanic Cloud, A. Acharyya et al. , CTA Consortium Collaboration, Mon. Not. Roy. Astron. Soc 523 (2023) 5353-5387
- Star tracking for pointing determination of Imaging Atmospheric Cherenkov Telescopes - Application to the Large-Sized Telescope of the Cherenkov Telescope Array, K. Abe et al. , CTA Consortium Collaboration, Astron. Astrophys. 679 (2023) A90
- Observations of the Crab Nebula and Pulsar with the Large-sized Telescope Prototype of the Cherenkov Telescope Array, H. Abe et al. , CTA Consortium Collaboration, Astrophys. J 956 (2023) 80
- Discovery of a Radiation Component from the Vela Pulsar Reaching 20 Teraelectronvolts, F. Aharonian et al. , HESS Collaboration, Nature Astron. 7 (2023) 1341-1350
2022: 3 articles
- Evidence for gamma-ray emission from the remnant of Kepler's supernova based on deep H.E.S.S. observations, F. Aharonian et al. , HESS Collaboration, Astron. Astrophys. 662 (2022) A65
- Time-resolved hadronic particle acceleration in the recurrent Nova RS Ophiuchi, S. De Wolf et al. , HESS Collaboration, Science 376 (2022) abn0567
- Search for dark matter annihilation signals in the H.E.S.S. Inner Galaxy Survey, H. Abdalla et al. , HESS Collaboration, Phys. Rev. Lett 129 (2022) 111101
Conference proceedings
2024: 2 conference proceedings
- The Cherenkov Telescope Array Observatory workflow management system, L. Arrabito, J. Bregeon, A. Faure, O. Gueta, N. Pigoux, A. Tsaregorodtsev , EPJ Web Conf., 295, 26th International Conference on Computing in High Energy & Nuclear Physics (2024) 04044, Norfolk, United States, 8-12 May 2023
- Study of the PeVatron candidate SNR G106.3+2.7 observed at Large Zenith Angle with LST-1 and MAGIC, M.-S. Carrasco , indéfini, JRJC 2023 - Journées de Rencontre Jeunes Chercheurs (2024), Saint-Jean-de-Monts, France, 22-28 Oct 2023
2023: 5 conference proceedings
- The next generation cameras for the Large-Sized Telescopes of the Cherenkov Telescope Array Observatory, M. Heller, J. Altet, X. Aragones, J. A. Barrio, M. Bellato, E. Bernasconi, A. Biland, O. Blanch, L. Burmistrov, E. Charbon, M. Dalchenko, F. Di Pierro, L. Giangrande, D. Gascon, S. Gòmez, D. Hoffmann , G. Martinez, M. Mariotti, D. Matteo, T. Montaruli, A. Okumura, A. P. Aguilera, R. Manera, R. Rando, T. Saito, A. Sanuy, L. A. Tejedor, Y. Uzun, PoS ICRC2023, 2023, 38th International Cosmic Ray Conference (2023) 740, Nagoya, Japan, 26 Jul - 03 Aug 2023
- Searching for gamma-ray counterparts of FRBs with H.E.S.S., F. Aharonian, F. A. Benkhali, A. Alkan, J. Aschersleben, H. Ashkar, M. Backes, A. Baktash, V. Barbosa Martins, A. Barnacka, J. Barnard, R. Batzofin, Y. Becherini, G. Beck, D. Berge, K. Bernlöhr, B. Bi, M. Böttcher, C. Boisson, J. Bolmont, M. de Bony de Lavergne, J. Borowska, M. Bouyahiaoui, F. Bradascio, M. Breuhaus, R. Brose, A. Brown, F. Brun, B. Bruno, T. Bulik, C. Burger-Scheidlin, T. Bylund, F. Cangemi, S. Caroff, S. Casanova, R. Cecil, J. Celic, M. Cerruti, P. Chambery, T. Chand, S. Chandra, A. Chen, J. Chibueze, O. Chibueze, T. Collins, G. Cotter, P. Cristofari, J. D. Mbarubucyeye, I. D. Davids, J. Davies, L. de Jonge, J. Devin, A. Djannati-Ataï, A. Dmytriiev, V. Doroshenko, L. Dreyer, L. Du Plessis, K. Egberts, S. Einecke, J.-P. Ernenwein , S. Fegan, K. Feijen, G. F. de Clairfontaine, G. Fontaine, F. Lott, M. Füßling, S. Funk, S. Gabici, Y. A. Gallant, S. Ghafourizadeh, G. Giavitto, L. Giunti, D. Glawion, J. F. Glicenstein, J. Glombitza, P. Goswami, G. Grolleron, M.-H. Grondin, L. Haerer, S. Hattingh, M. Haupt, G. Hermann, J. A. Hinton, W. Hofmann, T. L. Holch, M. Holler, D. Horns, Z. Huang, A. Jaitly, M. Jamrozy, F. Jankowsky, A. Jardin-Blicq, V. Joshi, I. Jung-Richardt, E. Kasai, K. Katarzyński, H. Katjaita, D. Khangulyan, R. Khatoon, B. Khélifi, S. Klepser, W. Kluźniak, N. Komin, R. Konno, K. Kosack, D. Kostunin, A. Kundu, G. Lamanna, R. G. Lang, S. Le Stum , V. Lefranc, F. Leitl, A. Lemière, M. Lemoine-Goumard, J.-P. Lenain, F. Leuschner, A. Luashvili, I. Lypova, J. Mackey, D. Malyshev, V. Marandon, A. Marcowith, P. Marinos, G. Martí-Devesa, R. Marx, G. Maurin, A. Mehta, P. J. Meintjes, M. Meyer, A. Mitchell, R. Moderski, L. Mohrmann, A. Montanari, C. Moore, E. Moulin, T. Murach, K. Nakashima, M. de Naurois, H. Ndiyavala, J. Niemiec, A. P. Noel, P. O'Brien, S. Ohm, L. Olivera-Nieto, E. de Ona Wilhelmi, M. Ostrowski, E. Oukacha, S. Panny, M. Panter, R. D. Parsons, U. Pensec, G. Peron, S. Pita, V. Poireau, D. A. Prokhorov, H. Prokoph, G. Pühlhofer, M. Punch, A. Quirrenbach, M. Regeard, P. Reichherzer, A. Reimer, O. Reimer, I. Reis, Q. Remy, H. Ren, M. Renaud, B. Reville, F. Rieger, G. Roellinghoff, E. Rol, G. Rowell, B. Rudak, H. R. Ricarte, E. Ruiz-Velasco, K. Sabri, V. Sahakian, S. Sailer, H. Salzmann, D. A. Sanchez, A. Santangelo, M. Sasaki, J. Schäfer, F. Schüssler, H. M. Schutte, M. Senniappan, J. N. S. Shapopi, S. Shilunga, K. Shiningayamwe, H. Sol, H. Spackman, A. Specovius, S. Spencer, Ł. Stawarz, R. Steenkamp, C. Stegmann, S. Steinmassl, C. Steppa, K. Streil, I. Sushch, H. Suzuki, T. Takahashi, T. Tanaka, T. Tavernier, A. M. Taylor, R. Terrier, A. Thakur, J. H. E. Thiersen, C. Thorpe-Morgan, M. Tluczykont, M. Tsirou, N. Tsuji, R. Tuffs, Y. Uchiyama, M. Ullmo, T. Unbehaun, P. van der Merwe, C. van Eldik, B. van Soelen, G. Vasileiadis, M. Vecchi, J. Veh, C. Venter, J. Vink, H. J. Völk, N. Vogel, T. Wach, S. J. Wagner, F. Werner, R. White, A. Wierzcholska, Y. W. Wong, H. Yassin, M. Zacharias, D. Zargaryan, A. A. Zdziarski, A. Zech, S. J. Zhu, A. Zmija, S. Zouari, N. Żywucka, PoS ICRC2023, 2023, 38th International Cosmic Ray Conference (2023) 776, Nagoya, Japan, 26 Jul - 03 Aug 2023
- LST-1 observations of an enormous flare of BL Lacertae in 2021, Nozaki, Seiya, Asano, Katsuaki, Escudero, Juan, Emery, Gabriel, Priyadarshi, Chaitanya, PoS ICRC2023, 2023, 38th International Cosmic Ray Conference (2023) 552, Nagoya, Japan, 26 Jul - 03 Aug 2023
- NectarChain, the scientific software for the CTA-NectarCAM, G. Grolleron, H. Ashkar, F. Brun, H. Costantini , D. Dumora, P. Jean, D. Kerszberg, J.-P. Lenain, V. Marandon, S. R. Patel, L. Tibaldo, PoS ICRC2023, 2023, 38th International Cosmic Ray Conference (2023) 862, Nagoya, Japan, 26 Jul - 03 Aug 2023
- Timing performances of NectarCAM, a Medium Sized Telescope Camera for the Cherenkov Telescope Array, H. Rueda, F. Bradascio, J. A. Barrio, J. Biteau, F. Brun, C. Champion, J.-F. Glicenstein, D. Hoffmann , P. Jean, J. P. Lenain, F. Louis, A. Pérez, M. Punch, P. Sizun, K.-H. Sulanke, L. A. Tejedor, B. Vallage, PoS ICRC2023, 2023, 38th International Cosmic Ray Conference (2023) 853, Nagoya, Japan, 26 Jul - 03 Aug 2023
Mémoire
2022: 1 mémoire
-
Etude du candidat PeVatron SNR G106.3+2.7 et optimisation de la sensibilité de CTA-North aux hautes énergies, G. Verna, Aix-Marseille Université, 09 Nov 2022
- Telescope construction: The CPPM Event Builder was successfully operated on the first complete NectarCAM (265 modules with a total of 1855 PMTs) and validated together with the internal two-level "deep buffer" network structure at IRFU, CEA Saclay. (June 2021)
- Telescope commissioning: The LST-1 telescope has detected very high energy emissions from the Crab Nebula. See CTA press release (June 2020)
- Telescope commissioning: The LST-1 telescope has detected its first gamma-ray signal in a campaign of several days, during which it was pointed to the Crab Nebula, which is considered the standard candle in very high-energy astronomy. See CTA press release (December 2019)
- Telescope construction: The NectarCAM camera, equipped with 61 production modules, has been temporarily mounted on the MST telescope prototype in Berlin-Adlershof to operate under real environment conditions. (May/June 2019)
- Telescope construction: The first LST telescope was inaugurated at the Observatory of the Roque de Los Muchachos on La Palma, Canary Islands, and operates on a daily basis during the Commissioning campaign since. (October 2018)
- DAQ activity: The CPPM Event Builder was successfully operated on the first LSTCAM (265 modules with a total of 1855 PMTs) at IFAE, Barcelona. (June 2018)
- DAQ activity: The CPPM Event Builder was successfully adapted and tested on the partial prototype (19 modules of 7 PMTs, at IAC, Tenerife)of the LSTCAM.
- Monte Carlo activity : Second campaign of observation for SST-GCT in Meudon in March 2017 (first Cherenkov data of a CTA prototype). DATA-MC comparison performed by CPPM
- DAQ activity: The CPPM acquisition was successfully exploited on the first partial prototype of the NectarCAM camera (14 modules of 7 PMTs at the IRFU, Saclay) since December 2016.