The Review summarizes much of particle physics and cosmology. Using data from previous editions, plus 3,062 new measurements from 721 papers, we list, evaluate, and average measured properties of gauge bosons and the recently discovered Higgs boson, leptons, quarks, mesons, and baryons. We summarize searches for hypothetical particles such as supersymmetric particles, heavy bosons, axions, dark photons, etc. All the particle properties and search limits are listed in Summary Tables. We also give numerous tables, figures, formulae, and reviews of topics such as Higgs Boson Physics, Supersymmetry, Grand Unified Theories, Neutrino Mixing, Dark Energy, Dark Matter, Cosmology, Particle Detectors, Colliders, Probability and Statistics. Among the 117 reviews are many that are new or heavily revised, including new reviews on Pentaquarks and Inflation. The complete Review is published online in a journal and on the website of the Particle Data Group (http://pdg.lbl.gov). The printed PDG Book contains the Summary Tables and all review articles but no longer includes the detailed tables from the Particle Listings. A Booklet with the Summary Tables and abbreviated versions of some of the review articles is also available. ; The publication of the Review of Particle Physics is supported by the Director, Office of Science, Office of High Energy Physics of the U.S. Department of Energy under Contract No. DE–AC02–05CH11231; by the European Laboratory for Particle Physics (CERN); by an implementing arrangement between the governments of Japan (MEXT: Ministry of Education, Culture, Sports, Science and Technology) and the United States (DOE) on cooperative research and development; by the Institute of High Energy Physics, Chinese Academy of Sciences; and by the Italian National Institute of Nuclear Physics (INFN). ; The authors are grateful to Vincent Vennin for his careful reading of this manuscript and preparing Fig. 23.3 for this review. The work of J.E. was supported in part by the London Centre for Terauniverse Studies (LCTS), using funding from the European Research Council via the Advanced Investigator Grant 267352 and from the UK STFC via the research grant ST/L000326/1. The work of D.W. was supported in part by the UK STFC research grant ST/K00090X/1.
The Review summarizes much of particle physics and cosmology. Using data from previous editions, plus 3,283 new measurements from 899 papers, we list, evaluate, and average measured properties of gauge bosons and the recently discovered Higgs boson, leptons, quarks, mesons, and baryons. We summarize searches for hypothetical particles such as heavy neutrinos, supersymmetric and technicolor particles, axions, dark photons, etc. All the particle properties and search limits are listed in Summary Tables. We also give numerous tables, figures, formulae, and reviews of topics such as Supersymmetry, Extra Dimensions, Particle Detectors, Probability, and Statistics. Among the 112 reviews are many that are new or heavily revised including those on: Dark Energy, Higgs Boson Physics, Electroweak Model, Neutrino Cross Section Measurements, Monte Carlo Neutrino Generators, Top Quark, Dark Matter, Dynamical Electroweak Symmetry Breaking, Accelerator Physics of Colliders, High-Energy Collider Parameters, Big Bang Nucleosynthesis, Astrophysical Constants and Cosmological Parameters. All tables, listings, and reviews (and errata) are also available on the Particle Data Group website: http://pdg.lbl.gov. ; Grupo de Investigación FQM330. ; The publication of the Review of Particle Physics is supported by the Director, Office of Science, Office of High Energy Physics of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231; by the U.S. National Science Foundation under Agreement No. PHY-0652989; by the European Laboratory for Particle Physics (CERN); by an implementing arrangement between the governments of Japan (MEXT: Ministry of Education, Culture, Sports, Science and Technology) and the United States (DOE) on cooperative research and development; and by the Italian National Institute of Nuclear Physics (INFN).
This biennial Review summarizes much of particle physics. Using data from previous editions, plus 2658 new measurements from 644 papers, we list, evaluate, and average measured properties of gauge bosons, leptons, quarks, mesons, and baryons. We summarize searches for hypothetical particles such as Higgs bosons, heavy neutrinos, and supersymmetric particles. All the particle properties and search limits are listed in Summary Tables. We also give numerous tables, figures, formulae, and reviews of topics such as the Standard Model, particle detectors, probability, and statistics. Among the 112 reviews are many that are new or heavily revised including those on Heavy-Quark and Soft-Collinear Effective Theory, Neutrino Cross Section Measurements, Monte Carlo Event Generators, Lattice QCD, Heavy Quarkonium Spectroscopy, Top Quark, Dark Matter, Vcb & Vub, Quantum Chromodynamics, High-Energy Collider Parameters, Astrophysical Constants, Cosmological Parameters, and Dark Matter. A booklet is available containing the Summary Tables and abbreviated versions of some of the other sections of this full Review. All tables, listings, and reviews (and errata) are also available on the Particle Data Group website: http://pdg.lbl.gov/. The 2012 edition of Review of Particle Physics is published for the Particle Data Group as article 010001 in volume 86 of Physical Review D. ; MICINN, Spain (FPA2009-07264-E) ; The publication of the Review of Particle Physics is supported by the Director, Office of Science, Office of High Energy and Nuclear Physics, the Division of High Energy Physics of the U.S. Department of Energy under Contract No. DE–AC02–05CH11231; by the U.S. National Science Foundation under Agreement No. PHY-0652989; by the European Laboratory for Particle Physics (CERN); by an implementing arrangement between the governments of Japan (MEXT: Ministry of Education, Culture, Sports, Science and Technology) and the United States (DOE) on cooperative research and development; and by the Italian National Institute of Nuclear Physics (INFN).
A booklet is available containing the Summary Tables and abbreviated versions of some of the other sections of this full Review. All tables, listings, and reviews (and errata) are also available on the Particle Data Group website: pdg.lbl.gov. ; This biennial Review summarizes much of particle physics. Using data from previous editions, plus 2158 new measurements from 551 papers, we list, evaluate, and average measured properties of gauge bosons, leptons, quarks, mesons, and baryons. We also summarize searches for hypothetical particles such as Higgs bosons, heavy neutrinos, and supersymmetric particles. All the particle properties and search limits are listed in Summary Tables. We also give numerous tables, figures, formulae, and reviews of topics such as the Standard Model, particle detectors, probability, and statistics. Among the 108 reviews are many that are new or heavily revised including those on neutrino mass, mixing, and oscillations, QCD, top quark, CKM quark-mixing matrix, Vud & Vus, Vcb & Vub, fragmentation functions, particle detectors for accelerator and non-accelerator physics, magnetic monopoles, cosmological parameters, and big bang cosmology. ; MICINN, Spain (FPA2009-07264-E). The publication of the Review of Particle Physics is supported by the Director, Office of Science, Office of High Energy and Nuclear Physics, the Division of High Energy Physics of the U.S. Department of Energy under Contract No. DE–AC02–05CH11231; by the U.S. National Science Foundation under Agreement No. PHY-0652989; by the European Laboratory for Particle Physics (CERN); by an implementing arrangement between the governments of Japan (MEXT: Ministry of Education, Culture, Sports, Science and Technology) and the United States (DOE) on cooperative research and development; and by the Italian National Institute of Nuclear Physics (INFN).
A booklet is available containing the Summary Tables and abbreviated versions of some of the other sections of this full Review. All tables, listings, and reviews (and errata) are also available on the Particle Data Group website: http://pdg.lbl.gov. ; This biennial Review summarizes much of particle physics. Using data from previous editions, plus 2778 new measurements from 645 papers, we list, evaluate, and average measured properties of gauge bosons, leptons, quarks, mesons, and baryons. We also summarize searches for hypothetical particles such as Higgs bosons, heavy neutrinos, and supersymmetric particles. All the particle properties and search limits are listed in Summary Tables. We also give numerous tables, figures, formulae, and reviews of topics such as the Standard Model, particle detectors, probability, and statistics. Among the 108 reviews are many that are new or heavily revised including those on CKM quark-mixing matrix, Vud & Vus, Vcb & Vub, top quark, muon anomalous magnetic moment, extra dimensions, particle detectors, cosmic background radiation, dark matter, cosmological parameters, and big bang cosmology. ; MICINN, Spain (FPA2005-25354-E and FPA2007-29104-E). The publication of the Review of Particle Physics is supported by the Director, Office of Science, Office of High Energy and Nuclear Physics, the Division of High Energy Physics of the U.S. Department of Energy under Contract No. DE–AC02–05CH11231; by the U.S. National Science Foundation under Agreement No. PHY-0652989; by the European Laboratory for Particle Physics (CERN); by an implementing arrangement between the governments of Japan (MEXT: Ministry of Education, Culture, Sports, Science and Technology) and the United States (DOE) on cooperative research and development; and by the Italian National Institute of Nuclear Physics (INFN).
Neutrino detectors participate in the indirect search for the fundamental constituents of dark matter (DM) in form of weakly interacting massive particles (WIMPs). In WIMP scenarios, candidate DM particles can pair-annihilate into Standard Model products, yielding considerable fluxes of high-energy neutrinos. A detector like ANTARES, located in the Northern Hemisphere, is able to perform a complementary search looking towards the Galactic Centre, where a high density of dark matter is thought to accumulate. Both this directional information and the spectral features of annihilating DM pairs are entered into an unbinned likelihood method to scan the data set in search for DM-like signals in ANTARES data. Results obtained upon unblinding 3170 days of data reconstructed with updated methods are presented, which provides a larger, and more accurate, data set than a previously published result using 2101 days. A non-observation of dark matter is converted into limits on the velocity-averaged cross section for WIMP pair annihilation. ; Centre National de la Recherche Scientifique (CNRS) ; French Atomic Energy Commission ; Commission Europeenne (FEDER fund) ; European Union (EU) ; Institut Universitaire de France (IUF) ; IdEx program at Sorbonne Paris Cite ANR-10-LABX-0023 ANR-11-IDEX-0005-02 ; UnivEarthS Labex program at Sorbonne Paris Cite ANR-10-LABX-0023 ANR-11-IDEX-0005-02 ; Labex OCEVU ANR-11-LABX-0060 ; French National Research Agency (ANR) ANR-11-IDEX-0001-02 ; Region Ile-de-France ; Region Grand-Est ; Region Provence-Alpes-Cote d'Azur ; Federal Ministry of Education & Research (BMBF) ; Instituto Nazionale di Fisica Nucleare(INFN), Italy ; Netherlands Organization for Scientific Research (NWO) Netherlands Government ; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia ; Executive Unit for Financing Higher Education, Research, Development and Innovation (UEFISCDI), Romania ; Ministerio de Ciencia, Innovacion y Universidades(MCIU): Programa Estatal de Generacion de Conocimiento PGC2018-096663-B-C41 PGC2018-096663-A-C42 PGC2018-096663-B-C43 PGC2018-096663-B-C44 ; Severo Ochoa Centre of Excellence and MultiDark Consolider (MCIU) ; Junta de Andalucia SOMM17/6104/UGR ; Generalitat Valenciana: Grisolia, Spain GRISOLIA/2018/119 ; Ministry of Higher Education, Scientific Research and Training, Morocco
A booklet is available containing the Summary Tables and abbreviated versions of some of the other sections of this full Review. All tables, listings, and reviews (and errata) are also available on the Particle Data Group website: http://pdg.lbl.gov. ; This biennial Review summarizes much of particle physics. Using data from previous editions, plus 2633 new measurements from 689 papers, we list, evaluate, and average measured properties of gauge bosons, leptons, quarks, mesons, and baryons. We also summarize searches for hypothetical particles such as Higgs bosons, heavy neutrinos, and supersymmetric particles. All the particle properties and search limits are listed in Summary Tables. We also give numerous tables, figures, formulae, and reviews of topics such as the Standard Model, particle detectors, probability, and statistics. Among the 110 reviews are many that are new or heavily revised including those on CKM quark-mixing matrix, Vud & Vus, Vcb & Vub, top quark, muon anomalous magnetic moment, extra dimensions, particle detectors, cosmic background radiation, dark matter, cosmological parameters, and big bang cosmology. ; MCYT Spain (FPA2002-12065-E). The publication of the Review of Particle Physics is supported by the Director, Office of Science, Office of High Energy and Nuclear Physics, the Division of High Energy Physics of the U.S. Department of Energy under Contract No. DE–AC02–05CH11231; by the U.S. National Science Foundation under Agreement No. PHY-0355084; by the European Laboratory for Particle Physics (CERN); by an implementing arrangement between the governments of Japan (MEXT: Ministry of Education, Culture, Sports, Science and Technology) and the United States (DOE) on cooperative research and development; and by the Italian National Institute of Nuclear Physics (INFN).
An offline search for a neutrino counterpart to gravitational-wave (GW) events detected during the second observation run (O2) of Advanced-LIGO and Advanced- Virgo performed with ANTARES data is presented. In addition to the search for long tracks induced by νμ (νμ) charged current interactions, a search for showering events induced by interactions of neutrinos of any flavour is conducted. The severe spatial and time coincidence provided by the gravitational-wave alert allows regions above the detector horizon to be probed, extending the ANTARES sensitivity over the entire sky. The results of this all-neutrino-flavour and all-sky time dependent analysis are presented. The search for prompt neutrino emission within ±500 s around the time of six GW events yields no neutrino counterparts. Upper limits on the neutrino spectral fluence and constraints on the isotropic energy radiated via high-energy neutrinos (from a few TeV to a few tens of PeV) are set for each GW event analysed. ; Centre National de la Recherche Scientifique (CNRS) ; French Atomic Energy Commission ; Commission Europeenne (FEDER fund), France ; European Union (EU) ; Institut Universitaire de France (IUF), France ; LabEx UnivEarthS, France ANR-10-LABX-0023 ANR-18-IDEX-0001 ; Region Ile-de-France ; Region Grand-Est ; Region Provence-Alpes-Cote d'Azur ; Ville de La Seyne-sur-Mer, France ; Federal Ministry of Education & Research (BMBF) ; Istituto Nazionale di Fisica Nucleare (INFN) ; Netherlands Organization for Scientific Research (NWO) Netherlands Government ; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia ; Executive Unit for Financing Higher Education, Research, Development and Innovation (UEFISCDI), Romania ; Ministerio de Ciencia, Innovación, Investigación y Universidades (MCIU): Programa Estatal de Generación de Conocimiento, Spain PGC2018-096663-B-C41 PGC2018-096663-A-C42 PGC2018-096663-B-C43 PGC2018-096663-B-C44 ; Severo Ochoa Centre of Excellence and MultiDark Consolider (MCIU), Junta de Andalucía, Spain SOMM17/6104/UGR ; Generalitat Valenciana: Grisolia, Spain GRISOLIA/2018/119 ; Ministry of Higher Education, Scientific Research and Professional Training, Morocco
The Advanced LIGO and Advanced Virgo observatories recently discovered gravitational waves from a binary neutron star inspiral. A short gamma-ray burst (GRB) that followed the merger of this binary was also recorded by the Fermi Gamma-ray Burst Monitor (Fermi-GBM), and the Anti-Coincidence Shield for the Spectrometer for the International Gamma-Ray Astrophysics Laboratory (INTEGRAL), indicating particle acceleration by the source. The precise location of the event was determined by optical detections of emission following the merger. We searched for high-energy neutrinos from the merger in the GeV–EeV energy range using the ANTARES, IceCube, and Pierre Auger Observatories. No neutrinos directionally coincident with the source were detected within ±500 s around the merger time. Additionally, no MeV neutrino burst signal was detected coincident with the merger. We further carried out an extended search in the direction of the source for high-energy neutrinos within the 14 day period following the merger, but found no evidence of emission. We used these results to probe dissipation mechanisms in relativistic outflows driven by the binary neutron star merger. The non-detection is consistent with model predictions of short GRBs observed at a large off-axis angle. ; Centre National de la Recherche Scientifique (CNRS) ; French Atomic Energy Commission ; Commission Europeenne (FEDER fund) ; European Union (EU) ; Institut Universitaire de France (IUF) ; IdEx program ; UnivEarthS Labex program at Sorbonne Paris Cite ANR-10-LABX-0023 ANR-11-IDEX-0005-02 ; Labex OCEVU ANR-11-LABX-0060 ; French National Research Agency (ANR) ANR-11-IDEX-0001-02 ; Region Ile-de-France ; Region Grand-Est ; Region Provence-Alpes-Cote d'Azur ; Region Provence-Alpes-Cote d'Azur ; Ville de La Seyne-sur-Mer, France ; Federal Ministry of Education & Research (BMBF) ; Istituto Nazionale di Fisica Nucleare (INFN) ; Netherlands Organization for Scientific Research (NWO) Netherlands Government ; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia ; National Authority for Scientific Research (ANCS), Romania ; Ministerio de Economia y Competitividad (MINECO): Plan Estatal de Investigacion FPA2015-65150-C3-1-P FPA2015-65150-C3-2-P FPA2015-65150-C3-3-P ; Severo Ochoa Centre of Excellence and MultiDark Consolider (MINECO), Spain ; Prometeo program (Generalitat Valenciana), Spain ; Grisolia program (Generalitat Valenciana), Spain ; Ministry of Higher Education, Scientific Research and Professional Training, Morocco ; National Science Foundation (NSF) ; National Science Foundation (NSF) ; University of Wisconsin Alumni Research Foundation ; Grid Laboratory Of Wisconsin (GLOW) grid infrastructure at the University of Wisconsin-Madison ; Open Science Grid (OSG) grid infrastructure ; United States Department of Energy (DOE) ; National Energy Research Scientific Computing Center ; Natural Sciences and Engineering Research Council of Canada CGIAR ; WestGrid and Compute/Calcul Canada ; Swedish Research Council ; Swedish Polar Research Secretariat, Sweden ; Swedish National Infrastructure for Computing (SNIC), Sweden ; Knut & Alice Wallenberg Foundation ; Federal Ministry of Education & Research (BMBF) ; German Research Foundation (DFG) ; Helmholtz Alliance for Astroparticle Physics (HAP), Germany ; Initiative and Networking Fund of the Helmholtz Association, Germany ; Fonds de la Recherche Scientifique - FNRS ; FWO Odysseus programme (Belspo) ; Flanders Institute to encourage scientific and technological research in industry (IWT) (Belspo) ; Belgian Federal Science Policy Office ; Royal Society of New Zealand Marsden Fund (NZ) ; Australian Research Council ; Ministry of Education, Culture, Sports, Science and Technology, Japan (MEXT) Japan Society for the Promotion of Science ; Swiss National Science Foundation (SNSF) ; National Research Foundation of Korea ; Villum Fonden, Denmark ; Danish National Research Foundation (DNRF), Denmark ; Argentina-Comision Nacional de Energia Atomica ; ANPCyT ; Argentina-Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) ; Argentina-Gobierno de la Provincia de Mendoza ; Argentina-Municipalidad de Malargue ; Argentina-NDM Holdings and Valle Las Lenas ; Australian Research Council ; National Council for Scientific and Technological Development (CNPq) ; Brazil-Financiadora de Estudos e Projetos (FINEP) ; Carlos Chagas Filho Foundation for Research Support of the State of Rio de Janeiro (FAPERJ) ; Brazil-Sao Paulo Research Foundation (FAPESP) 2010/07359-6 1999/05404-3 ; Brazil-Ministerio da Ciencia, Tecnologia, Inovacoes e Comunicacoes (MCTIC) ; Czech Republic Government MSMT CR LG15014 LO1305 LM2015038 CZ.02.1.01/0.0/0.0/16_013/0001402 ; France-Centre de Calcul IN2P3/CNRS ; Centre National de la Recherche Scientifique (CNRS) ; France-Conseil Regional Ile-de-France ; France-Departement Physique Nucleaire et Corpusculaire (PNC-IN2P3/CNRS) ; France-Departement Sciences de l'Univers (SDU-INSU/CNRS) ; French National Research Agency (ANR) LABEX ANR-10-LABX-63 ANR-11-IDEX-0004-02 ; Federal Ministry of Education & Research (BMBF) ; German Research Foundation (DFG) ; Germany-Finanzministerium Baden-Wurttemberg ; Germany-Helmholtz Alliance for Astroparticle Physics (HAP) ; Germany-Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF) ; Germany-Ministerium fur Innovation, Wissenschaft und Forschung des Landes Nordrhein-Westfalen ; Germany-Ministerium fur Wissenschaft, Forschung und Kunst des Landes Baden-Wurttemberg ; Italy-Istituto Nazionale di Fisica Nucleare (INFN) ; Italy-Istituto Nazionale di Astrofisica (INAF) ; Italy-Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR) ; Italy-CETEMPS Center of Excellence ; Italy-Ministero degli Affari Esteri (MAE) ; Consejo Nacional de Ciencia y Tecnologia (CONACyT) 167733 ; Mexico-Universidad Nacional Autonoma de Mexico (UNAM) ; Mexico-PAPIIT DGAPA-UNAM ; The Netherlands-Ministerie van Onderwijs, Cultuur en Wetenschap ; The Netherlands-Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO) ; The Netherlands-Stichting voor Fundamenteel Onderzoek der Materie (FOM) ; Poland-National Centre for Research and Development ERA-NET-ASPERA/01/11 ERA-NET-ASPERA/02/11 ; Poland-National Science Centre 2013/08/M/ST9/00322 2013/08/M/ST9/00728 HARMONIA 5-2013/10/M/ST9/00062 UMO-2016/22/M/ST9/00198 ; Portugal-Portuguese national funds within Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia (COMPETE) ; Portugal-FEDER funds within Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia (COMPETE) ; Romania-Romanian Authority for Scientific Research ANCS ; Romania-CNDI-UEFISCDI partnership projects 20/2012 194/2012 PN 16 42 01 02 ; Slovenian Research Agency - Slovenia ; Spain-Comunidad de Madrid ; Spain-Fondo Europeo de Desarrollo Regional (FEDER) funds ; Spain-Ministerio de Economía y Competitividad ; Spain-Xunta de Galicia ; European Union (EU) FP7-PEOPLE-2012-IEF-328826 ; Spain-USA-Department of Energy DE-AC02-07CH11359 DE-FR02-04ER41300 DE-FG02-99ER41107 DE-SC0011689 ; Spain-National Science Foundation 0450696 ; Spain-The Grainger Foundation ; Spain-Marie Curie-IRSES/EPLANET ; Spain-European Particle Physics Latin American Network ; Spain-European Union 7th Framework Program PIRSES-2009-GA-246806 ; Spain-European Union's Horizon research and innovation programme 646623 ; Spain-UNESCO ; EGO consortium ; Council of Scientific & Industrial Research (CSIR) - India ; Department of Science & Technology (India) ; Science AMP; Engineering Research Board (SERB), India ; Ministry of Higher Education & Scientific Research (MHESR) ; Spanish Agencia Estatal de Investigación ; Vicepresidencia i Conselleria d'Innovacio Recerca i Turisme ; Conselleria d'Educacio i Universitat del Govern de les Illes Balears ; Conselleria d'Educacio Investigacio Cultura i Esport de la Generalitat Valenciana ; National Science Centre, Poland ; Swiss National Science Foundation (SNSF) ; Russian Foundation for Basic Research (RFBR) ; Russian Science Foundation (RSF) ; European Commission European Commission Joint Research Centre ; European Union (EU) ; Royal Society of London ; Scottish Funding Council ; Scottish Universities Physics Alliance ; Scottish Universities Physics Alliance ; Lyon Institute of Origins (LIO) ; National Research, Development and Innovation Office Hungary (NKFI) ; National Research Foundation of Korea ; Industry Canada ; Province of Ontario through the Ministry of Economic Development and Innovation ; Natural Sciences and Engineering Research Council of Canada ; Canadian Institute for Advanced Research (CIFAR) ; Brazilian Ministry of Science, Technology, Innovations, and Communications ; International Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR) ; Hong Kong Research Grants Council ; National Natural Science Foundation of China (NSFC) ; Leverhulme Trust ; Ministry of Science and Technology, Taiwan ; Kavli Foundation ; National Science Foundation (NSF) NSF - Directorate for Computer & Information Science & Engineering (CISE) 1626251 ; National Science Foundation (NSF) NSF- Directorate for Education & Human Resources (EHR) 1242090 ; 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SB would like to thank Tara Murphy, Martin Bell, Paul Hancock, Keith Bannister, Chris Blake and Bing Zhang for useful discussions. ; We report the discovery of four Fast Radio Bursts (FRBs) in the ongoing SUrvey for Pulsars and Extragalactic Radio Bursts at the Parkes Radio Telescope: FRBs 150610, 151206, 151230 and 160102. Our real-time discoveries have enabled us to conduct extensive, rapid multimessenger follow-up at 12 major facilities sensitive to radio, optical, X-ray, gamma-ray photons and neutrinos on time-scales ranging from an hour to a few months post-burst. No counterparts to the FRBs were found and we provide upper limits on afterglow luminosities. None of the FRBs were seen to repeat. Formal fits to all FRBs show hints of scattering while their intrinsic widths are unresolved in time. FRB 151206 is at low Galactic latitude, FRB 151230 shows a sharp spectral cut-off, and FRB 160102 has the highest dispersion measure (DM = 2596.1 ± 0.3 pc cm−3) detected to date. Three of the FRBs have high dispersion measures (DM > 1500 pc cm−3), favouring a scenario where the DM is dominated by contributions from the intergalactic medium. The slope of the Parkes FRB source counts distribution with fluences >2 Jy ms is α=−2.2+0.6−1.2 and still consistent with a Euclidean distribution (α = −3/2). We also find that the all-sky rate is 1.7+1.5−0.9×103 FRBs/(4π sr)/day above ∼2Jyms and there is currently no strong evidence for a latitude-dependent FRB sky rate. ; The Parkes radio telescope and the Australia Telescope Compact Array are part of the Australia Telescope National Facility which is funded by the Commonwealth of Australia for operation as a National Facility managed by CSIRO. Parts of this research were conducted by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020. The GMRT is run by the National Centre for Radio Astrophysics of the Tata Institute of Fundamental Research. VLAis run by theNational Radio Astronomy Observatory (NRAO). NRAO is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. This work was performed on the gSTAR national facility at Swinburne University of Technology. gSTAR is funded by Swinburne and the Australian Government's Education Investment Fund. This work is also based on data collected at Subaru Telescope, which is operated by the National Astronomical Observatory of Japan. We thank the LSST Project for making their code available as free software at http://dm.lsstcorp.org. Funding from the European Research Council under the European Union's Seventh Framework Programme (FP/2007-2013) / ERC Grant Agreement n. 617199 (EP). Access to the Lovell Telescope is supported through an STFC consolidated grant. The 100-m telescope in Effelsberg is operation by the Max- Planck-Institut für Radioastronomie with funds of the Max-Planck Society. The Sardinia Radio Telescope (SRT) is funded by the Department of University and Research (MIUR), the Italian Space Agency (ASI), and the Autonomous Region of Sardinia (RAS) and is operated as National Facility by the National Institute for Astrophysics (INAF). TB and RWW are grateful to the STFC for financial support (grant reference ST/P000541/1). Research support to IA is provided by the Australian Astronomical Observatory. The ANTARES authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Commission Européenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), IdEx program and UnivEarthS Labex program at Sorbonne Paris Cité (ANR-10- LABX-0023 and ANR-11-IDEX-0005-02), Labex OCEVU (ANR- 11-LABX-0060) and the A*MIDEX project (ANR-11-IDEX-0001- 02), Région Île-de-France (DIM-ACAV), Région Alsace (contrat CPER), Région Provence-Alpes-Côte d'Azur, Département du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium für Bildung und Forschung (BMBF), Germany; IstitutoNazionale di Fisica Nucleare (INFN), Italy; Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS), Romania; Ministerio de Economía y Competitividad (MINECO): Plan Estatal de Investigación (refs. FPA2015- 65150-C3-1-P, -2-P and -3-P, (MINECO/FEDER)), Severo Ochoa Centre of Excellence and MultiDark Consolider (MINECO), and Prometeo and Grisolía programs (Generalitat Valenciana), Spain; Ministry of Higher Education, Scientific Research and Professional Training, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities. This work made use of data supplied by the UK Swift Science Data Centre at the University of Leicester. This research has made use of data, software and/or web tools obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), a service of the Astrophysics Science Division at NASA/GSFC and of the Smithsonian Astrophysical Observatory's High Energy Astrophysics Division. This work is based in part on data collected at Subaru Telescope, which is operated by the National Astronomical Observatory of Japan. This paper makes use of software developed for the Large Synoptic Survey Telescope. We thank the LSST Project for making their code available as free software at http://dm.lsstcorp.org. RPE/MK gratefully acknowledges support from ERC Synergy Grant "BlackHoleCam" Grant Agreement Number 610058
The KM3NeT Collaboration runs a multi-site neutrino observatory in the Mediterranean Sea. Water Cherenkov particle detectors, deep in the sea and far off the coasts of France and Italy, are already taking data while incremental construction progresses. Data Acquisition Control software is operating off-shore detectors as well as testing and qualification stations for their components. The software, named Control Unit, is highly modular. It can undergo upgrades and reconfiguration with the acquisition running. Interplay with the central database of the Collaboration is obtained in a way that allows for data taking even if Internet links fail. In order to simplify the management of computing resources in the long term, and to cope with possible hardware failures of one or more computers, the KM3NeT Control Unit software features a custom dynamic resource provisioning and failover technology, which is especially important for ensuring continuity in case of rare transient events in multi-messenger ; French National Research Agency (ANR) ANR-15-CE31-0020 ; Centre National de la Recherche Scientifique (CNRS) ; Commission Europeenne (FEDER fund) ; European Union (EU) ; Institut Universitaire de France (IUF), France ; IdEx program ; Univearths Labex program at Sorbonne Paris Cite, France ANR-10-LABX-0023 ANR-11-IDEX-000502 ; Paris Ile-de-France Region, France ; Shota Rustaveli National Science Foundation of Georgia (SRNSFG), Georgia FR-18-1268 ; German Research Foundation (DFG) ; Greek Ministry of Development-GSRT ; Istituto Nazionale di Fisica Nucleare (INFN), Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR), PRIN 2017 program Italy NAT-NET 2017W4HA7S ; Ministry of Higher Education, Scientific Research and Professional Training, Morocco ; Netherlands Organization for Scientific Research (NWO) Netherlands Government ; National Science Center, Poland National Science Centre, Poland 2015/18/E/ST2/00758 ; National Authority for Scientific Research (ANCS), Romania ; Ministerio de Ciencia, Innovacion, Investigacion y Universidades (MCIU), Spain ; Programa Estatal de Generacion de Conocimiento (MCIU/FEDER) PGC2018-096663-B-C41 PGC2018-096663-A-C42 PGC2018-096663-B-C43 PGC2018-096663-BC44 ; Severo Ochoa Centre of Excellence ; MultiDark Consolider (MCIU), Spain ; Junta de Andalucía ; Generalitat Valenciana, Spain: Grisolia GRISOLIA/2018/119 ; Generalitat Valenciana CIDEGENT/2018/034 ; La Caixa Foundation LCF/BQ/IN17/11620019 ; EU: MSC program, Spain 713673
The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l'Energie Atomique et aux Energies Alternatives(CEA), Commission Europeenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), Labex UnivEarthS(ANR-10-LABX-0023 and ANR-18-IDEX-0001), Region Ile-de-France (DIM-ACAV), Region Alsace (contrat CPER), Region Provence-AlpesCote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fur Bildung und Forschung (BMBF), Germany; Instituto Nazionale di Fisica Nucleare(INFN), Italy; Nederlandse Organisatie voor Wetenschappelijk Onderzoek(NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; Executive Unit for Financing Higher Education, Research, Development and Innovation (UEFISCDI), Romania; Ministerio de Ciencia e Innovacion (MCI) and Agencia Estatal de Investigacion: Programa Estatal de Generacion de Conocimiento (refs. PGC2018096663-B-C41, -A-C42, -B-C43, -B-C44) (MCI/FEDER), Severo Ochoa Centre of Excellence and MultiDark Consolider, Junta de Andalucia (ref. SOMM17/6104/UGR and A-FQM-053-UGR18), Generalitat Valenciana: Grisolia (ref. GRISOLIA/2018/119) and GenT (ref. CIDEGENT/2018/034) programs, Spain; Ministry of Higher Education, Scientific Research and Professional Training, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities. The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l'Energie Atomique et aux Energies Alternatives(CEA), Commission Europeenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), Labex UnivEarthS(ANR-10-LABX-0023 and ANR-18-IDEX-0001), Region Ile-de-France (DIM-ACAV), Region Alsace (contrat CPER), Region Provence-AlpesCote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fur Bildung und Forschung (BMBF), Germany; Instituto Nazionale di Fisica Nucleare(INFN), Italy; Nederlandse Organisatie voor Wetenschappelijk Onderzoek(NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; Executive Unit for Financing Higher Education, Research, Development and Innovation (UEFISCDI), Romania; Ministerio de Ciencia e Innovacion (MCI) and Agencia Estatal de Investigacion: Programa Estatal de Generacion de Conocimiento (refs. PGC2018096663-B-C41, -A-C42, -B-C43, -B-C44) (MCI/FEDER), Severo Ochoa Centre of Excellence and MultiDark Consolider, Junta de Andalucia (ref. SOMM17/6104/UGR and A-FQM-053-UGR18), Generalitat Valenciana: Grisolia (ref. GRISOLIA/2018/119) and GenT (ref. CIDEGENT/2018/034) programs, Spain; Ministry of Higher Education, Scientific Research and Professional Training, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities. ; This letter presents a combined measurement of the energy spectra of atmospheric nu(e) and nu(mu) in the energy range between similar to 100 GeV and similar to 50 TeV with the ANTARES neutrino telescope. The analysis uses 3012 days of detector livetime in the period 2007-2017, and selects 1016 neutrinos interacting in (or close to) the instrumented volume of the detector, yielding shower-like events (mainly from nu(e) + (nu) over bar (e) charged current plus all neutrino neutral current interactions) and starting track events (mainly from nu(mu) + (nu) over bar (mu) charged current interactions). The contamination by atmospheric muons in the final sample is suppressed at the level of a few per mill by different steps in the selection analysis, including a Boosted Decision Tree classifier. The distribution of reconstructed events is unfolded in terms of electron and muon neutrino fluxes. The derived energy spectra are compared with previous measurements that, above 100 GeV, are limited to experiments in polar ice and, for nu(mu), to Super-Kamiokande. ; Centre National de la Recherche Scientifique (CNRS) ; French Atomic Energy Commission ; Commission Europeenne (FEDER fund) ; Institut Universitaire de France (IUF) ; Labex UnivEarthS ANR-10-LABX-0023 ANR-18-IDEX-0001 ; Region Ile-de-France ; Region Grand-Est ; Region Provence-Alpes-Cote d'Azur ; Region Provence-Alpes-Cote d'Azur ; Federal Ministry of Education & Research (BMBF) ; Instituto Nazionale di Fisica Nucleare(INFN), Italy ; Netherlands Organization for Scientific Research (NWO) ; Netherlands Government ; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia ; Consiliul National al Cercetarii Stiintifice (CNCS) ; Unitatea Executiva pentru Finantarea Invatamantului Superior, a Cercetarii, Dezvoltarii si Inovarii (UEFISCDI) ; Spanish Government PGC2018096663-B-C41 PGC2018096663-A-C42 PGC2018096663-B-C43 PGC2018096663-B-C44 ; Severo Ochoa Centre of Excellence and MultiDark Consolider ; Junta de Andalucia SOMM17/6104/UGR A-FQM-053-UGR18 ; Generalitat Valenciana: Grisolia program, Spain GRISOLIA/2018/119 ; Generalitat Valenciana: GenT program, Spain CIDEGENT/2018/034 ; Ministry of Higher Education, Scientific Research and Professional Training, Morocco ; Agencia Estatal de Investigacion PGC2018096663-B-C41 PGC2018096663-A-C42 PGC2018096663-B-C43 PGC2018096663-B-C44 ; Commission Europeenne (Marie Curie Program)
LIGO Scientific Collaboration and Virgo Collaboration, Fermi GBM, INTEGRAL, IceCube Collaboration, AstroSat Cadmium Zinc Telluride Imager Team, IPN Collaboration, The Insight-HXMT Collaboration, ANTARES Collaboration, The Swift Collaboration, AGILE Team, The 1M2H Team, The Dark Energy Camera GW-EM Collaboration and the DES Collaboration, The DLT40 Collaboration, GRAWITA: GRAvitational Wave Inaf TeAm, The Fermi Large Area Telescope Collaboration, ATCA: Australia Telescope Compact Array, ASKAP: Australian SKA Pathfinder, Las Cumbres Observatory Group, OzGrav, DWF (Deeper, Wider, Faster Program), AST3, and CAASTRO Collaborations, The VINROUGE Collaboration, MASTER Collaboration, J-GEM, GROWTH, JAGWAR, CaltechNRAO, TTU-NRAO, and NuSTAR Collaborations, Pan-STARRS, The MAXI Team, TZAC Consortium, KU Collaboration, Nordic Optical Telescope, ePESSTO, GROND, Texas Tech University, SALT Group, TOROS: Transient Robotic Observatory of the South Collaboration, The BOOTES Collaboration, MWA: Murchison Widefield Array, The CALET Collaboration, IKI-GW Follow-up Collaboration, H.E.S.S. Collaboration, LOFAR Collaboration, LWA: Long Wavelength Array, HAWC Collaboration, The Pierre Auger Collaboration, ALMA Collaboration, Euro VLBI Team, Pi of the Sky Collaboration, The Chandra Team at McGill University, DFN: Desert Fireball Network, ATLAS, High Time Resolution Universe Survey, RIMAS and RATIR, and SKA South Africa/MeerKAT ; On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of $\sim 1.7\,{\rm{s}}$ with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of ${40}_{-8}^{+8}$ Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 $\,{M}_{\odot }$. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at $\sim 40\,{\rm{Mpc}}$) less than 11 hours after the merger by the One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ~10 days. Following early non-detections, X-ray and radio emission were discovered at the transient's position $\sim 9$ and $\sim 16$ days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC 4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta. ; Kavli Foundation ; Danmarks Grundforskningsfond ; Niels Bohr International Academy ; DARK Cosmology Centre ; National Science Foundation (NSF) AST-1518052 AST-141242 AST-1411763 AST-1714498 AST-1517649 PHY-1607291 AST-1412421 AST-1313484 ; Gordon AMP; Betty Moore Foundation ; Heising-Simons Foundation ; Alfred P. 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JAXA (Japan) ; Knut & Alice Wallenberg Foundation ; Swedish Research Council ; National Space Board (Sweden) ; Istituto Nazionale Astrofisica (INAF) ; Centre National D'etudes Spatiales ; United States Department of Energy (DOE) DE-AC02-76SF00515 ; Office of Naval Research N00014-07-C0147 ; National Science Foundation under University Radio Observatory AST-1139963 AST-1139974 ; ESO Telescopes at the Paranal Observatory 099.D-0382 099.D-0622 099.D-0191 099.D-0116 ; REM telescope at the ESO La Silla Observatory 35020 ; Department of University and Research (MIUR) ; Italian Space Agency (ASI) ; Russian Academy of Sciences ; Istituto Nazionale Astrofisica (INAF) ; BIC 114332KYSB20160007 ; Chinese Academy of Sciences KJZD-EW-M06 ; National Natural Science Foundation of China 11673062 ; Oversea Talent Program of Yunnan Province ; Science & Technology Facilities Council (STFC) ; Slovenian Research Agency - Slovenia P1-0188 ; Sorbonne Paris Cite ANR-10-LABX-0023 ANR-11-IDEX-0005-02 ; GROWTH (Global Relay of Observatories Watching Transients Happen) - National Science Foundation under PIRE 1545949 ; California Institute of Technology (USA) ; University of Maryland College Park (USA) ; Ministry of Education, Culture, Sports, Science and Technology, Japan (MEXT) Japan Society for the Promotion of Science 15H05437 ; JST Consortia ; University of Wisconsin-Milwaukee (USA) ; Texas Tech University (USA) ; San Diego State University (USA) ; United States Department of Energy (DOE) ; Los Alamos National Laboratory ; Tokyo Institute of Technology (Japan) ; National Central University (Taiwan) ; Indian Institute of Astrophysics (India) ; Inter-University Center for Astronomy and Astrophysics (India) ; Weizmann Institute of Science (Israel) ; Oskar Klein Centre at Stockholm University (Sweden) ; Humboldt University (Germany) ; Liverpool John Moores University (UK) ; Planning and Budgeting Committee ; Israel Science Foundation ; Large Synoptic Survey Telescope Corporation ; National Science Foundation (NSF) 1455090 ; ERC grant TReX ; Naval Research Laboratory (NRL) ; NRL ; Oxford Centre for Astrophysical Surveys ; 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European Research Council (ERC) 647208 ; Netherlands Organization for Scientific Research through NWO VIDI 639.042.612-Nissanke ; Netherlands Organization for Scientific Research (NWO) 62002444-Nissanke ; VISIR 60.A-9392 ; MOST104-2923-M-008-004-MY5 ; MOST106-2112-M-008-007
The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargüe. We are very grateful to the following agencies and organizations for financial support: Comisión Nacional de Energía Atómica, Fundación Antorchas, Gobierno De La Provincia de Mendoza, Municipalidad de Malargüe, NDM Holdings and Valle Las Leñas, in gratitude for their continuing cooperation over land access, Argentina; the Australian Research Council; Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundação de Amparo à Pesquisa do Estado de Rio de Janeiro (FAPERJ), São Paulo Research Foundation (FAPESP) Grants # 2010/07359-6 and # 1999/05404-3, Ministério de Ciência e Tecnologia (MCT), Brazil; MSMT-CR LG13007, 7AMB14AR005, CZ.1.05/2.1.00/03.0058 and the Czech Science Foundation Grant 14-17501S, Czech Republic; Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Conseil Régional Ile-de-France, Département Physique Nucléaire et Corpusculaire (PNC-IN2P3/CNRS), Département Sciences de l'Univers (SDU-INSU/CNRS), Institut Lagrange de Paris, ILP LABEX ANR-10-LABX-63, within the Investissements d'Avenir ProgrammeANR-11-IDEX-0004-02, France; Bundesministerium für Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Finanzministerium Baden-Württemberg, Helmholtz Alliance for Astroparticle Physics (HAP), Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Ministerium für Wissenschaft und Forschung, Nordrhein Westfalen, Ministerium für Wissenschaft, Forschung und Kunst, Baden-Württemberg, Germany; Istituto Nazionale di Astrofisica (INAF), Istituto Nazionale di Fisica Nucleare (INFN), Ministero dell'Istruzione, dell'Università e della Ricerca (MIUR), Gran Sasso Center for Astroparticle Physics (CFA), CETEMPS Center of Excellence, Italy; Consejo Nacional de Ciencia y Tecnología (CONACYT), Mexico; Ministerie van Onderwijs, Cultuur en Wetenschap, Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Stichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands; National Centre for Research and Development, Grant nos. ERA-NETASPERA/01/11 and ERA-NET-ASPERA/02/11, National Science Centre, Grant nos. 2013/08/M/ST9/00322, and 2013/08/M/ST9/00728 and HARMONIA 5 – 2013/10/M/ST9/00062, Poland; Portuguese national funds and FEDER funds within COMPETE – Programa Operacional Factores de Competitividade through Fundação para a Ciencia e a Tecnologia, Portugal; Romanian Authority for Scientific Research ANCS, CNDI-UEFISCDI partnership projects nos. 20/2012 and nr.194/2012, project nos. 1/ASPERA2/2012 ERA-NET, PN-II-RU-PD-2011-3-0145-17, and PN-II-RU-PD-2011- 3-0062, the Minister of National Education, Programme for research – Space Technology and Advanced Research – STAR, project number 83/2013, Romania; Slovenian Research Agency, Slovenia; Comunidad de Madrid, FEDER funds, Ministerio de Educación y Ciencia, Xunta de Galicia, European Community 7th Framework Program, Grant no. FP7-PEOPLE-2012-IEF-328826, Spain; Science and Technology Facilities Council, United Kingdom; Department of Energy, Contract no. DE-AC02-07CH11359, DE-FR02-04ER41300, DE-FG02-99ER41107 and DE-SC0011689, National Science Foundation, Grant no. 0450696, The Grainger Foundation, USA; NAFOSTED, Vietnam; Marie Curie-IRSES/EPLANET, European Particle Physics Latin American Network, European Union 7th Framework Program, Grant no. PIRSES-2009- GA-246806; and UNESCO. ; The Pierre Auger Observatory, located on a vast, high plain in western Argentina, is the world׳s largest cosmic ray observatory. The objectives of the Observatory are to probe the origin and characteristics of cosmic rays above 1017 eV and to study the interactions of these, the most energetic particles observed in nature. The Auger design features an array of 1660 water Cherenkov particle detector stations spread over 3000 km2 overlooked by 24 air fluorescence telescopes. In addition, three high elevation fluorescence telescopes overlook a 23.5 km2, 61-detector infilled array with 750 m spacing. The Observatory has been in successful operation since completion in 2008 and has recorded data from an exposure exceeding 40,000 km2 sr yr. This paper describes the design and performance of the detectors, related subsystems and infrastructure that make up the Observatory. ; Comision Nacional de Energia Atomica ; Fundacion Antorchas ; Gobierno De La Provincia de Mendoza ; Municipalidad de Malargue ; NDM Holdings and Valle Las Lenas ; Australian Research Council ; National Council for Scientific and Technological Development (CNPq) ; Ciencia Tecnologia e Inovacao (FINEP) ; Carlos Chagas Filho Foundation for Research Support of the State of Rio de Janeiro (FAPERJ) ; Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP) 2010/07359-6 1999/05404-3 ; Ministerio de Ciencia e Tecnologia (MCT), Brazil ; Ministry of Education, Youth & Sports - Czech Republic LG13007 7AMB14AR005 CZ.1.05/2.1.00/03.0058 ; Grant Agency of the Czech Republic Czech Republic Government 14-17501S ; Centre National de la Recherche Scientifique (CNRS) ; Region Ile-de-France ; Departement Physique Nucleaire et Corpusculaire PNC-IN2P3/CNRS ; Departement Sciences de l'Univers (SDU-INSU/CNRS) ; Institut Lagrange de Paris ; French National Research Agency (ANR) ANR-11-IDEX-0004-02 ANR-10-LABX-63 ; Federal Ministry of Education & Research (BMBF) ; German Research Foundation (DFG) ; Finanzministerium Baden-Wurttemberg ; Helmholtz Alliance for Astroparticle Physics (HAP) ; Helmholtz Association ; Ministerium fur Wissenschaft und Forschung ; Nordrhein Westfalen ; Ministerium fur Wissenschaft ; Forschung und Kunst ; Baden-Wurttemberg, Germany ; Istituto Nazionale Astrofisica (INAF) ; Istituto Nazionale di Fisica Nucleare (INFN) ; Ministry of Education, Universities and Research (MIUR) ; Gran Sasso Center for Astroparticle Physics (CFA) ; CETEMPS Center of Excellence, Italy ; Consejo Nacional de Ciencia y Tecnologia (CONACyT) ; Ministerie van Onderwijs ; Cultuur en Wetenschap ; Netherlands Organization for Scientific Research (NWO) ; FOM (The Netherlands) Netherlands Government ; National Centre for Research and Development ERA-NET-ASPERA/01/11 ERA-NET-ASPERA/02/11 ; National Science Centre, Poland 2013/08/M/ST9/00322 2013/08/M/ST9/00728 HARMONIA 5 - 2013/10/M/ST9/00062 ; Portuguese national funds ; FEDER funds within COMPETE - Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia, Portugal ; Romanian Authority for Scientific Research ANCS ; CNDI-UEFISCDI 20/2012 194/2012 1/ASPERA2/2012 ERA-NET PN-II-RU-PD-2011-3-0145-17 PN-II-RU-PD-2011-3-0062 ; Programme for research - Space Technology and Advanced Research - STAR, Romania 83/2013 ; Slovenian Research Agency - Slovenia ; Comunidad de Madrid Instituto de Salud Carlos III ; European Union (EU) ; Spanish Government ; Xunta de Galicia ; European Community, Spain FP7-PEOPLE-2012-IEF-328826 ; Science & Technology Facilities Council (STFC) ; United States Department of Energy (DOE) DE-AC02-07CH11359 DE-FR02-04ER41300 DE-FG02-99ER41107 DE-SC0011689 ; National Science Foundation (NSF) 0450696 ; Grainger Foundation, USA ; National Foundation for Science & Technology Development (NAFOSTED) ; Marie Curie-IRSES/EPLANET ; European Particle Physics Latin American Network ; European Union (EU) PIRSES-2009-GA-246806 ; UNESCO
The authors acknowledge the financial support of the funding agencies: Agence Nationale de la Recherche (contract ANR-15-CE31-0020), Centre National de la Recherche Scientifique (CNRS), Commission Europeenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), LabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX-0001), Paris Ile-de-France Region, France; Shota Rustaveli National Science Foundation of Georgia (SRNSFG, FR-18-1268), Georgia; Deutsche Forschungsgemeinschaft (DFG), Germany; The General Secretariat of Research and Technology (GSRT), Greece; Istituto Nazionale di Fisica Nucleare (INFN), Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR), PRIN 2017 program (Grant NAT-NET 2017W4HA7S) Italy; Ministry of Higher Education Scientific Research and Professional Training, ICTP through Grant AF-13, Morocco; Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; The National Science Centre, Poland (2015/18/E/ST2/00758); National Authority for Scientific Research (ANCS), Romania; Ministerio de Ciencia, Innovacion, Investigacion y Universidades (MCIU): Programa Estatal de Generacion de Conocimiento (refs. PGC2018-096663-B-C41, -A-C42, -B-C43, -B-C44) (MCIU/FEDER), Severo Ochoa Centre of Excellence and MultiDark Consolider (MCIU), Junta de Andalucia (ref. SOMM17/6104/UGR), Generalitat Valenciana: Grisolia (ref. GRISOLIA/2018/119) and GenT (ref. CIDEGENT/2018/034) programs, La Caixa Foundation (ref. LCF/BQ/IN17/11620019), EU: MSC program (ref. 713673), Spain. ; The KM3NeT infrastructure consists of two deep-sea neutrino telescopes being deployed in the Mediterranean Sea. The telescopes will detect extraterrestrial and atmospheric neutrinos by means of the incident photons induced by the passage of relativistic charged particles through the seawater as a consequence of a neutrino interaction. The telescopes are configured in a three-dimensional grid of digital optical modules, each hosting 31 photomultipliers. The photomultiplier signals produced by the incident Cherenkov photons are converted into digital information consisting of the integrated pulse duration and the time at which it surpasses a chosen threshold. The digitization is done by means of time to digital converters (TDCs) embedded in the field programmable gate array of the central logic board. Subsequently, a state machine formats the acquired data for its transmission to shore. We present the architecture and performance of the front-end firmware consisting of the TDCs and the state machine. ; French National Research Agency (ANR) ANR-15-CE31-0020 ; Centre National de la Recherche Scientifique (CNRS) ; Commission Europeenne (FEDER fund), France ; Commission Europeenne (Marie Curie Program), France ; Institut Universitaire de France (IUF), France ; LabEx UnivEarthS, France ANR-10-LABX-0023 ANR-18-IDEX-0001 ; Paris Ile-de-France Region, France ; Shota Rustaveli National Science Foundation of Georgia (SRNSFG), Georgia FR-18-1268 ; German Research Foundation (DFG) ; Greek Ministry of Development-GSRT ; Istituto Nazionale di Fisica Nucleare (INFN) NAT-NET 2017W4HA7S ; Ministry of Education, Universities and Research (MIUR) NAT-NET 2017W4HA7S ; PRIN 2017 program Italy NAT-NET 2017W4HA7S ; Ministry of Higher Education Scientific Research and Professional Training, ICTP, Morocco AF-13 ; Netherlands Organization for Scientific Research (NWO) Netherlands Government ; National Science Centre, Poland 2015/18/E/ST2/00758 ; National Authority for Scientific Research (ANCS), Romania ; Ministerio de Ciencia, Innovacion, Investigacion y Universidades (MCIU): Programa Estatal de Generacion de Conocimiento (MCIU/FEDER), Spain PGC2018-096663-B-C41 PGC2018-096663-A-C42 PGC2018-096663-B-C43 PGC2018-096663-B-C44 ; Severo Ochoa Centre of Excellence and MultiDark Consolider (MCIU), Spain ; Junta de Andalucia European Commission SOMM17/6104/UGR ; Generalitat Valenciana: Grisolia program, Spain GRISOLIA/2018/119 ; Generalitat Valenciana: GenT program, Spain CIDEGENT/2018/034 ; La Caixa Foundation LCF/BQ/IN17/11620019 ; EU: MSC program, Spain 713673
