We gratefully acknowledge financial support from the following agencies and organisations:
State Committee of Science of Armenia, Armenia; The Australian Research Council, Astronomy Australia Ltd, The University of Adelaide, Australian National University, Monash University, The University of New South Wales, The University of Sydney, Western Sydney University, Australia; Federal Ministry of Education, Science and Research, and Innsbruck University, Austria; Conselho Nacional de Desenvolvimento Cientı́fico e Tecnológico (CNPq), Fundação de Amparo à Pesquisa do Estado do Rio de Janeiro (FAPERJ), Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP), Fundação de Apoio à Ciência, Tecnologia e Inovação do Paraná – Fundação Araucária, Ministry of Science, Technology, Innovations and Communications (MCTIC), and Instituto Serrapilheira, Brasil; Ministry of Education and Science, National RI Roadmap Project DO1-153/28.08.2018, Bulgaria; The Natural Sciences and Engineering Research Council of Canada and the Canadian Space Agency, Canada; ANID PIA / APOYO AFB230003, ANID-Chile Basal grant FB 210003, Núcleo Milenio TITANs (NCN19-058), FONDECYT-Chile grants 1201582, 1210131, 1230345, and 1240904; Croatian Science Foundation, Rudjer Boskovic Institute, University of Osijek, University of Rijeka, University of Split, Faculty of Electrical Engineering, Mechanical Engineering and Naval Architecture, University of Zagreb, Faculty of Electrical Engineering and Computing, Croatia; Ministry of Education, Youth and Sports, MEYS LM2018105, LM2023047, EU/MEYS CZ.02.1.01/0.0/0.0/16 013/0001403, CZ.02.1.01/0.0/0.0/18 046/0016007, CZ.02.1.01/0.0/0.0/16 019/0000754 and CZ.02.01.01/00/22 008/0004632, Czech Republic; Academy of Finland (grant nr. 317636, 320045, 317383 and 320085), Finland; Ministry of Higher Education and Research, CNRS-INSU and CNRS-IN2P3, CEA-Irfu, ANR, Regional Council Ile de France, Labex ENIGMASS, OCEVU, OSUG2020 and P2IO, France; The German Bundesministerium für Forschung, Technologie und Raumfahrt (BMFTR), the Max Planck Society, the Deutsche Forschungsgemeinschaft (DFG, with Collaborative Research Centre 1491), and the Helmholtz Association, Germany; Department of Atomic Energy, Department of Science and Technology, India; Istituto Nazionale di Astrofisica (INAF), Istituto Nazionale di Fisica Nucleare (INFN), MIUR, Istituto Nazionale di Astrofisica (INAF-OABRERA) Grant Fondazione Cariplo/Regione Lombardia ID 2014-1980/RST ERC, Italy; ICRR, University of Tokyo, JSPS, MEXT, Japan; Netherlands Research School for Astronomy (NOVA), Netherlands Organization for Scientific Research (NWO), Netherlands; University of Oslo, Norway; Ministry of Science and Higher Education, DIR/WK/2017/12, the National Centre for Research and Development and the National Science Centre, UMO-2016/22/M/ST9/00583, Poland; Slovenian Research and Innovation Agency, grants P1-0031, I0-E018, J1-60014, Slovenia; South African Department of Science and Innovation and National Research Foundation through the South African Gamma-Ray Astronomy Programme, South Africa; The Spanish groups acknowledge funds from “ERDF A way of making Europe”, the Spanish Ministry of Science, Innovation and Universities, and the Spanish Research State Agency (AEI) via MCIN/AEI/10.13039/501100011033, grants CNS2023-144504, PID2024-155874NB-C21, PID2024-155316NB-I00, PDC2023-145839-I00, PID2022-137810NB-C22, PID2022-139117NB-C42/C43/C44, PID2022-136828NB-C41/C42, PID2022-138172NB-C41/C43, and budget lines 28.06.000X.411.01 and 28.06.000X.711.04 of PGE 2023, 2024 and 2025; the “Centro de Excelencia Severo Ochoa” program through grants no. CEX2020-001007-S, CEX2021-001131-S, CEX2024001442-S; the “Unidad de Excelencia María de Maeztu” program through grants no. CEX2019-000918-M and CEX2020-001058-M; the “Ramón y Cajal” program through grant RYC2024-048445-I and RYC2021-032991-I. They also acknowledge the support of the Spanish Research Council via the grant CSIC PIE 202350E189, as well as the projects funded by the Comunidad de Madrid regional government with refs. PR47/21 TAU and TEC-2024/TEC-182, the latter with the acronym “Mad4Space funded by Order 3177/2024 of Dirección General de Investigación e Innovación. Funds were also granted by the “Consejería de Universidad, Investigación e Innovación” of the regional government of Andalucía (Refs. AST22 00001 9 and AST22 0001 16) and “Plan Andaluz de Investigación, Desarrollo e Innovación” (Ref. FQM-322); and by the “Programa Operativo de Crecimiento Inteligente” FEDER 2014-2020 (Refs. ESFRI-2017-IAC-12 and ESFRI-2020-01-IAC-12) and Spanish Ministry of Science, Innovation and Universities, 15% co-financed by “Consejería de Economía, Industria, Comercio y Conocimiento” of the Gobierno de Canarias regional government. The Generalitat de Catalunya regional government is also gratefully acknowledged via its “CERCA” program, grant no. 2021SGR00679. Spanish groups were also kindly supported by European Union funds via NextGenerationEU, grants no. PRTR-C17.I1, CT19/23-INVM-109, the “MicroStars” ERC, ref. 101076533, and the INFRA/ACME, ref. 101131928. Views and opinions expressed are however those of the authors only and do not necessarily reflect those of the European Union or the European Research Council. Neither the European Union nor the granting authority can be held responsible for them. This research used computing and storage resources provided by the Port d’Informació Científica (PIC) data center; Swedish Research Council, Royal Physiographic Society of Lund, Royal Swedish Academy of Sciences, The Swedish National Infrastructure for Computing (SNIC) at Lunarc (Lund), Sweden; State Secretariat for Education, Research and Innovation (SERI) and Swiss National Science Foundation (SNSF), Switzerland; The National Research Foundation of Ukraine (project 2023.03/0149 and 2023.05/0024), Ukraine; Durham University, Leverhulme Trust, Liverpool University, University of Leicester, University of Oxford, Royal Society, Science and Technology Facilities Council, UK; U.S. National Science Foundation, U.S. Department of Energy, Argonne National Laboratory, Barnard College, University of California, University of Chicago, Columbia University, Georgia Institute of Technology, Institute for Nuclear and Particle Astrophysics (INPAC-MRPI program), Iowa State University, the Smithsonian Institution, V.V.D. is funded by NSF grant AST-1911061, Washington University McDonnell Center for the Space Sciences, The University of Wisconsin and the Wisconsin Alumni Research Foundation, USA.
The research leading to these results has received funding from the European Union’s Seventh Framework Programme (FP7/2007-2013) under grant agreements No 262053 and No 317446. This project is receiving funding from the European Union’s Horizon 2020 research and innovation programs under agreement No 676134.