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arXiv 2017年

作者： Albert, A. André, M. Anghinolfi, M. Anton, G. Ardid, M. Aubert, J.-J. Avgitas, T. Baret, B. Barrios-Martí, J. Basa, S. Belhorma, B. Bertin, V. Biagi, S. Bormuth, R. Bourret, S. Bouwhuis, M.C. Brânzaş, H. Bruijn, R. Brunner, J. Busto, J. Capone, A. Caramete, L. Carr, J. Celli, S. Cherkaoui El Moursli, R. Chiarusi, T. Circella, M. Coelho, J.A.B. Coleiro, A. Coniglione, R. Costantini, H. Coyle, P. Creusot, A. Díaz, A.F. Deschamps, A. de Bonis, G. Distefano, C. Di Palma, I. Domi, A. Donzaud, C. Dornic, D. Drouhin, D. Eberl, T. El Bojaddaini, I. El Khayati, N. Elsässer, D. Enzenhöfer, A. Ettahiri, A. Fassi, F. Felis, I. Fusco, L.A. Gay, P. Giordano, V. Glotin, H. Grégoire, T. Gracia Ruiz, R. Graf, K. Hallmann, S. van Haren, H. Heijboer, A.J. Hello, Y. Hernández-Rey, J.J. Hößl, J. Hofestädt, J. Hugon, C. Illuminati, G. James, C.W. de Jong, M. Jongen, M. Kadler, M. Kalekin, O. Katz, U. Kießling, D. Kouchner, A. Kreter, M. Kreykenbohm, I. Kulikovskiy, V. Lachaud, C. Lahmann, R. Lefèvre, D. Leonora, E. Lotze, M. Loucatos, S. Marcelin, M. Margiotta, A. Marinelli, A. Martínez-Mora, J.A. Mele, R. Melis, K. Michael, T. Migliozzi, P. Moussa, A. Navas, S. Nezri, E. Organokov, M. Pav alaş, G.E. Pellegrino, C. Perrina, C. Piattelli, P. Popa, V. Pradier, T. Quinn, L. Racca, C. Riccobene, G. Sánchez-Losa, A. Saldaña, M. Salvadori, I. Samtleben, D.F.E. Sanguineti, M. Sapienza, P. Schüssler, F. Sieger, C. Spurio, M. Stolarczyk, Th. Taiuti, M. Tayalati, Y. Trovato, A. Turpin, D. Tönnis, C. Vallage, B. van Elewyck, V. Versari, F. Vivolo, D. Vizzoca, A. Wilms, J. Zornoza, J.D. Zúñiga, J. GRPHE Université de Haute Alsace Institut Universitaire de Technologie de Colmar 34 rue du Grillenbreit BP 50568 Colmar68008 France Technical University of Catalonia Laboratory of Applied Bioacoustics Rambla Exposició Vilanova i la Geltrú Barcelona08800 Spain INFN - Sezione di Genova Via Dodecaneso 33 Genova16146 Italy Friedrich-Alexander-Universität Erlangen-Nürnberg Erlangen Centre for Astroparticle Physics Erwin-Rommel-Str. 1 Erlangen91058 Germany Universitat Politècnica de València C/ Paranimf 1 Gandia46730 Spain Aix Marseille Univ CNRS IN2P3 CPPM Marseille France APC Univ Paris Diderot CNRS IN2P3 CEA Irfu Obs de Paris Sorbonne Paris Cité France IFIC - Instituto de Física Corpuscular CSIC Universitat de València c/ Catedrático José Beltrán 2 Paterna ValenciaE-46980 Spain LAM - Laboratoire d'Astrophysique de Marseille Pôle de l'Étoile Site de Château-Gombert rue Frédéric Joliot-Curie 38 Marseille Cedex 1313388 France National Center for Energy Sciences and Nuclear Techniques B.P.1382 R. P. Rabat10001 Morocco Via S. Sofia 62 Catania95123 Italy Nikhef Science Park Amsterdam Netherlands Huygens-Kamerlingh Onnes Laboratorium Universiteit Leiden Netherlands Institute for Space Science Bucharest MagureleRO-077125 Romania Universiteit van Amsterdam Instituut Voor Hoge-Energie Fysica Science Park 105 Amsterdam1098 XG Netherlands INFN - Sezione di Roma P.le Aldo Moro 2 Roma00185 Italy Dipartimento di Fisica dell'Università La Sapienza P.le Aldo Moro 2 Roma00185 Italy Gran Sasso Science Institute Viale Francesco Crispi 7 L'Aquila00167 Italy University Mohammed V in Rabat Faculty of Sciences 4 av. Ibn Battouta B.P. 1014 R.P Rabat10000 Morocco INFN - Sezione di Bologna Viale Berti-Pichat 6/2 Bologna40127 Italy INFN - Sezione di Bari Via E. Orabona 4 Bari70126 Italy Department of Computer Architecture and Technology CITIC University of Granada Granada18071 Spain Géoazur UCA CNRS IRD Observatoire de la Côte d'Azu

Advanced LIGO detected a significant gravitational wave signal (GW170104) originating from the coalescence of two black holes during the second observation run on January 4th, 2017. An all-sky high-energy neutrino follow-up search has been made using data from the Antares neutrino telescope, including both upgoing and downgoing events in two separate analyses. No neutrino candidates were found within ±500 s around the GW event time nor any time clustering of events over an extended time window of ±3 months. The non-detection is used to constrain isotropic-equivalent high-energy neutrino emission from GW170104 to less than ∼ 4 × 1054 erg for a E−2 spectrum. Copyright © 2017, The Authors. All rights reserved.

关键词： Gravity waves

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The ANTARES Collaboration: Contributions to ICRC 2017 Part I: Neutrino astronomy (diffuse fluxes and point sources)

arXiv

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arXiv 2017年

作者： Albert, A. André, M. Anghinolfi, M. Anton, G. Ardid, M. Aubert, J.-J. Avgitas, T. Baret, B. Barrios-Martí, J. Basa, S. Belhorma, B. Bertin, V. Biagi, S. Bormuth, R. Bourret, S. Bouwhuis, M.C. Brânzaş, H. Bruijn, R. Brunner, J. Busto, J. Capone, A. Caramete, L. Carr, J. Celli, S. Cherkaoui El Moursli, R. Chiarusi, T. Circella, M. Coelho, J.A.B. Coleiro, A. Coniglione, R. Costantini, H. Coyle, P. Creusot, A. Díaz, A.F. Deschamps, A. de Bonis, G. Distefano, C. Di Palma, I. Domi, A. Donzaud, C. Dornic, D. Drouhin, D. Eberl, T. El Bojaddaini, I. El Khayati, N. Elsässer, D. Enzenhöfer, A. Ettahiri, A. Fassi, F. Felis, I. Fusco, L.A. Gay, P. Giordano, V. Glotin, H. Grégoire, T. Gracia Ruiz, R. Graf, K. Hallmann, S. van Haren, H. Heijboer, A.J. Hello, Y. Hernández-Rey, J.J. Hößl, J. Hofestädt, J. Hugon, C. Illuminati, G. James, C.W. de Jong, M. Jongen, M. Kadler, M. Kalekin, O. Katz, U. Kießling, D. Kouchner, A. Kreter, M. Kreykenbohm, I. Kulikovskiy, V. Lachaud, C. Lahmann, R. Lefèvre, D. Leonora, E. Lotze, M. Loucatos, S. Marcelin, M. Margiotta, A. Marinelli, A. Martínez-Mora, J.A. Mele, R. Melis, K. Michael, T. Migliozzi, P. Moussa, A. Navas, S. Nezri, E. Organokov, M. Păvălaş, G.E. Pellegrino, C. Perrina, C. Piattelli, P. Popa, V. Pradier, T. Quinn, L. Racca, C. Riccobene, G. Sánchez-Losa, A. Saldaña, M. Salvadori, I. Samtleben, D.F.E. Sanguineti, M. Sapienza, P. Schüssler, F. Sieger, C. Spurio, M. Stolarczyk, Th. Taiuti, M. Tayalati, Y. Trovato, A. Turpin, D. Tönnis, C. Vallage, B. van Elewyck, Veronique Versari, F. Vivolo, D. Vizzoca, A. Wilms, J. Zornoza, J.D. Zúñiga, J. GRPHE Université de Haute Alsace Institut universitaire de technologie de Colmar 34 rue du Grillenbreit BP Colmar50568 - 68008 France Technical University of Catalonia Laboratory of Applied Bioacoustics Rambla Exposició Vilanova i la Geltrú Barcelona08800 Spain INFN - Sezione di Genova Via Dodecaneso 33 Genova16146 Italy Friedrich-Alexander-Universität Erlangen-Nürnberg Erlangen Centre for Astroparticle Physics Erwin-Rommel-Str. 1 Erlangen91058 Germany Universitat Politècnica de València C/ Paranimf 1 Gandia46730 Spain Aix Marseille Univ CNRS/IN2P3 CPPM Marseille France APC Univ Paris Diderot CNRS/IN2P3 CEA/Irfu Obs de Paris Sorbonne Paris Cité France c/ Catedrático José Beltrán 2 PaternaValenciaE-46980 Spain LAM - Laboratoire d’Astrophysique de Marseille Pôle de l’Étoile Site de Château-Gombert rue Frédéric Joliot-Curie 38 Marseille Cedex 1313388 France National Center for Energy Sciences and Nuclear Techniques B.P.1382 R. P. Rabat10001 Morocco Via S. Sofia 62 Catania95123 Italy Nikhef Science Park Amsterdam Netherlands Huygens-Kamerlingh Onnes Laboratorium Universiteit Leiden Netherlands Institute of Space Science Bucharest MagureleRO-077125 Romania Universiteit van Amsterdam Instituut voor Hoge-Energie Fysica Science Park 105 Amsterdam1098 XG Netherlands INFN - Sezione di Roma P.le Aldo Moro 2 Roma00185 Italy Dipartimento di Fisica dell’Università La Sapienza P.le Aldo Moro 2 Roma00185 Italy Gran Sasso Science Institute Viale Francesco Crispi 7 L’Aquila00167 Italy University Mohammed V in Rabat Faculty of Sciences 4 av. Ibn Battouta B.P. 1014 R.P Rabat10000 Morocco INFN - Sezione di Bologna Viale Berti-Pichat 6/2 Bologna40127 Italy INFN - Sezione di Bari Via E. Orabona 4 Bari70126 Italy Department of Computer Architecture and Technology CITIC University of Granada Granada18071 Spain Géoazur UCA CNRS IRD Observatoire de la Côte d’Azur Sophia Antipolis France Dipartimento di Fisica dell’Università Via

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26th Annual Computational Neuroscience Meeting (CNS*2017): Part 1

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BMC Neurosci 2017年第SUPPL 1期18卷 58-58页

作者： Sue Denham Panayiota Poirazi Erik De Schutter Karl Friston Ho Ka Chan Thomas Nowotny Dongqi Han Sungho Hong Sophie Rosay Tanja Wernle Alessandro Treves Sarah Goethals Romain Brette Tomas Van Pottelbergh Rodolphe Sepulchre Alex D. Bird Hermann Cuntz Pedro J. Gonçalves Jan-Matthis Lueckmann Giacomo Bassetto Marcel Nonnenmacher Jakob H. Macke Audrey J. Sederberg Jason N. MacLean Stephanie E. Palmer Ulisse Ferrari Christophe Gardella Olivier Marre Thierry Mora Emina Ibrahimovic Martin Müller Jean-Pascal Pfister Tushar Chauhan Timothée Masquelier Alexandre Montlibert Benoit R. Cottereau Moritz Helias Jannis Schuecker David Dahmen Sven Goedeke Alexandre Hyafil Ainhoa Hermoso-Mendizabal Pavel E. Rueda-Orozco Santiago Jaramillo David Robbe Jaime de la Rocha Marie Rooy Fani Koukouli David DiGregorio Uwe Maskos Boris Gutkin Andrey Yu Verisokin Darya V. Verveyko Dmitry E. Postnov Willy Wong Omid Talakoub Robert Chen Milos Popovic Dmitriy Lisitsyn Eric Drebitz Iris Grothe Sunita Mandon Andreas Kreiter Udo Ernst Peter A. Robinson Xuelong Zhao Kevin M. Aquino John D. Griffiths Grishma Mehta-Pandejee Natasha Gabay James MacLaurin Somwrita Sarkar Tim Kunze Jens Haueisen Thomas R. Knösche Subutai Ahmad Yuwei Cui Marcus Lewis Jeff Hawkins Simona Olmi Spase Petkoski Fabrice Bartolomei Maxime Guye Viktor Jirsa Hazem Toutounji Daniel Durstewitz Matteo Cantarelli Adrian Quintana Boris Marin Matt Earnshaw Padraig Gleeson Robert Court Robert McDougal R. Angus Silver Salvador Dura-Bernal Stephen Larson William W. Lytton Giovanni Idili Lorenzo Posani Simona Cocco Karel Ježek Rémi Monasson School of Psychology Faculty of Health & Human Sciences Plymouth University Plymouth Devon PL4 8AA UK Institute of Molecular Biology and Biotechnology (IMBB) Foundation for Research and Technology-Hellas (FORTH) Heraklion Crete Greece Okinawa Institute of Science and Technology Graduate University Okinawa Japan Wellcome Trust Centre for Neuroimaging Institute of Neurology UCL London WC1N 3BG UK School of Engineering and Informatics University of Sussex Brighton BN1 9QJ UK Graduate School Okinawa Institute of Science and Technology Okinawa 904-0495 Japan Computational Neuroscience Unit Okinawa Institute of Science and Technology Okinawa 904-0495 Japan Cognitive Neuroscience Area Scuola Internazionale Superiore di Studi Avanzati Trieste 34136 Italy Kavli Institute for Systems Neuroscience NTNU Trondheim 7030 Norway Institut de la Vision Sorbonne Universités UPMC Univ Paris 06 INSERM CNRS Paris 75012 France Department of Engineering University of Cambridge Cambridge Cambridgeshire CB2 1PZ UK Ernst Strüngmann Institute for Neuroscience Max Planck Society Frankfurt Germany Frankfurt Institute for Advanced Studies Frankfurt Germany Neural Systems Analysis Research Center Caesar An Associate of the Max Planck Society Bonn Germany Max Planck Institute for Biological Cybernetics Tübingen Germany Bernstein Center for Computational Neuroscience Tübingen Germany Present Address: Biomedical Engineering Department Georgia Institute of Technology Atlanta GA 30306 USA Department of Neurobiology University of Chicago Chicago IL 60637 USA Department of Organismal Biology and Anatomy University of Chicago Chicago IL 60637 USA Committee on Computational Neuroscience University of Chicago Chicago IL 60637 USA Institut de la Vision Sorbonne Universités INSERM Paris France Laboratoire de Physique Statistique Ecole Normale Supérieure Paris France Institute of Molecular Life Sciences University of Zürich 8057 Zürich Switzerland Institute of Neuroinformatics Univer

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The SUrvey for pulsars and extragalactic radio bursts II: New FRB discoveries and their follow-up

arXiv

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arXiv 2017年

作者： Bhandari, S. Keane, E.F. Barr, E.D. Jameson, A. Petroff, E. Johnston, S. Bailes, M. Bhat, N.D.R. Burgay, M. Burke-Spolaor, S. Caleb, M. Eatough, R.P. Flynn, C. Green, J.A. Jankowski, F. Kramer, M. Venkatraman Krishnan, V. Morello, V. Possenti, A. Stappers, B. Tiburzi, C. van Straten, W. Andreoni, I. Butterley, T. Chandra, P. Cooke, J. Corongiu, A. Coward, D.M. Dhillon, V.S. Dodson, R. Hardy, L.K. Howell, E.J. Jaroenjittichai, P. Klotz, A. Littlefair, S.P. Marsh, T.R. Mickaliger, M. Muxlow, T. Perrodin, D. Pritchard, T. Sawangwit, U. Terai, T. Tominaga, N. Torne, P. Totani, T. Trois, A. Turpin, D. Niino, Y. Wilson, R.W. Albert, A. André, M. Anghinolfi, M. Anton, G. Ardid, M. Aubert, J.-J. Avgitas, T. Baret, B. Barrios-Martí, J. Basa, S. Belhorma, B. Bertin, V. Biagi, S. Bormuth, R. Bourret, S. Bouwhuis, M.C. Brânzaş, H. Bruijn, R. Brunner, J. Busto, J. Capone, A. Caramete, L. Carr, J. Celli, S. Cherkaoui El Moursli, R. Chiarusi, T. Circella, M. Coelho, J.A.B. Coleiro, A. Coniglione, R. Costantini, H. Coyle, P. Creusot, A. Díaz, A.F. Deschamps, A. de Bonis, G. Distefano, C. Di Palma, I. Domi, A. Donzaud, C. Dornic, D. Drouhin, D. Eberl, T. El Bojaddaini, I. Elsässer, D. Enzenhöfer, A. Felis, I. Fusco, L.A. Gay, P. Giordano, V. Glotin, H. Gregoire, T. Gracia-Ruiz, R. Graf, K. Hallmann, S. van Haren, H. Heijboer, A.J. Hello, Y. Hernández-Rey, J.J. Hößl, J. Hofestädt, J. Hugon, C. Illuminati, G. James, C.W. de Jong, M. Jongen, M. Kadler, M. Kalekin, O. Katz, U. Kießling, D. Kouchner, A. Kreter, M. Kreykenbohm, I. Kulikovskiy, V. Lachaud, C. Lahmann, R. Lefèvre, D. Leonora, E. Loucatos, S. Marcelin, M. Margiotta, A. Marinelli, A. Martínez-Mora, J.A. Mele, R. Melis, K. Michael, T. Migliozzi, P. Moussa, A. Navas, S. Nezri, E. Organokov, M. Păvălaş, G.E. Pellegrino, C. Perrina, C. Piattelli, P. Popa, V. Pradier, T. Quinn, L. Racca, C. Riccobene, G. Sánchez-Losa, A. Centre for Astrophysics and Supercomputing Swinburne University of Technology Mail H30 PO Box 218 VIC3122 Australia CSIRO Astronomy & Space Science Australia Telescope National Facility P.O. Box 76 EppingNSW1710 Australia SKA Organisation Jodrell Bank Observatory CheshireSK11 9DL United Kingdom ASTRON Netherlands Institute for Radio Astronomy Postbus 2 AA Dwingeloo7990 Netherlands National Radio Astronomy Observatory 1003 Lopezville Rd. SocorroNM87801 United States Department of Physics and Astronomy West Virginia University P.O. Box 6315 MorgantownWV26506 United States Center for Gravitational Waves and Cosmology West Virginia University Chestnut RidgeResearch Building MorgantownWV26505 Australian Astronomical Observatory 105 Delhi Rd North RydeNSW2113 Australia Max Planck Institut für Radioastronomie Auf dem Hügel 69 BonnD-53121 Germany International Centre for Radio Astronomy Research Curtin University BentleyWA6102 Australia I-09047 Italy Research School of Astronomy and Astrophysics Australian National University ACT2611 Australia National Centre for Radio Astrophysics Tata Institute of Fundamental Research Pune University Campus Ganeshkhind Pune411 007 India Department of Physics and Astronomy University of Sheffield SheffieldS3 7RH United Kingdom Jodrell Bank Centre for Astrophysics University of Manchester Alan Turing Building Oxford Road ManchesterM13 9PL United Kingdom Fakultät fur Physik Universität Bielefeld Postfach 100131 BielefeldD-33501 Germany Institute for Radio Astronomy and Space Research Auckland University of Technology 120 Mayoral Drive Auckland1010 New Zealand University of British Columbia 2329 West Mall VancouverBCV6T 1Z4 Canada Konan University 8-9-1 Okamoto Higashinada Ward KobeHyogo Prefecture658-0072 Japan University of Tokyo 7 Chome-3-1 Hongo Bunkyo Tokyo113-8654 Japan School of Physics University of Western Australia M013 CrawleyWA6009 Australia Université de Toulouse UPS-OMP

We report the discovery of four Fast Radio Bursts (FRBs) in the ongoing SUrvey for Pulsars and Extragalactic Radio Bursts (SUPERB) at the Parkes Radio Telescope: FRBs 150610, 151206, 151230 and 160102. Our real-time discoveries have enabled us to conduct extensive, rapid multi-messenger 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 cutoff, 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+−01..62 and still consistent with a Euclidean distribution (α = −3/2). We also find that the all-sky rate is 1.7+−10..59 × 103FRBs/(4π sr)/day above ∼ 2 Jy ms and there is currently no strong evidence for a latitude-dependent FRB sky-rate. Copyright © 2017, The Authors. All rights reserved.

关键词： Surveys

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SEARCH for HIGH-ENERGY NEUTRINOS from BINARY NEUTRON STAR MERGER GW170817 with ANTARES, ICECUBE, and the PIERRE AUGER OBSERVATORY

arXiv

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arXiv 2017年

作者： Albert, A. André, M. Anghinolfi, M. Ardid, M. Aubert, J.-J. Aublin, J. Avgitas, T. Baret, B. Barrios-Martí, J. Basa, S. Belhorma, B. Bertin, V. Biagi, S. Bormuth, R. Bourret, S. Bouwhuis, M.C. Brânzaş, H. Bruijn, R. Brunner, J. Busto, J. Capone, A. Caramete, L. Carr, J. Celli, S. Cherkaoui El Moursli, R. Chiarusi, T. Circella, M. Coelho, J.A.B. Coleiro, A. Coniglione, R. Costantini, H. Coyle, P. Creusot, A. Díaz, A.F. Deschamps, A. de Bonis, G. Distefano, C. Di Palma, I. Domi, A. Donzaud, C. Dornic, D. Drouhin, D. Eberl, T. El Bojaddaini, I. El Khayati, N. Elsässer, D. Enzenhöfer, A. Ettahiri, A. Fassi, F. Felis, I. Fusco, L.A. Gay, P. Giordano, V. Glotin, H. Grégoire, T. Gracia Ruiz, R. Graf, K. Hallmann, S. van Haren, H. Heijboer, A.J. Hello, Y. Hernández-Rey, J.J. Hössl, J. Hofestädt, J. Illuminati, G. James, C.W. de Jong, M. Jongen, M. Kadler, M. Kalekin, O. Katz, U. Kiessling, D. Kouchner, A. Kreter, M. Kreykenbohm, I. Kulikovskiy, V. Lachaud, C. Lahmann, R. Lefèvre, D. Leonora, E. Lotze, M. Loucatos, S. Marcelin, M. Margiotta, A. Marinelli, A. Martínez-Mora, J.A. Mele, R. Melis, K. Michael, T. Migliozzi, P. Moussa, A. Navas, S. Nezri, E. Organokov, M. Pavălăş, G.E. Pellegrino, C. Perrina, C. Piattelli, P. Popa, V. Pradier, T. Quinn, L. Racca, C. Riccobene, G. Sánchez-Losa, A. Saldaña, M. Salvadori, I. Samtleben, D.F.E. Sanguineti, M. Sapienza, P. Schüssler, F. Sieger, C. Spurio, M. Stolarczyk, T.H. Taiuti, M. Tayalati, Y. Trovato, A. Turpin, D. Tönnis, C. Vallage, B. van Elewyck, V. Versari, F. Vivolo, D. Vizzoca, A. Wilms, J. Zornoza, J.D. Zúñiga, J. Aartsen, M.G. Ackermann, M. Adams, J. Aguilar, J.A. Ahlers, M. Ahrens, M. Al Samarai, I. Altmann, D. Andeen, K. Anderson, T. Ansseau, I. Anton, G. Argüelles, C. Auffenberg, J. Axani, S. Bagherpour, H. Bai, X. Barron, J.P. Barwick, S.W. Baum, V. Bay, R. Beatty, J.J. Becker Tjus, J. Becker, K.-H. Benzvi, S. Berley, D. GRPHE Université de Haute Alsace Institut Universitaire de Technologie de Colmar 34 rue du Grillenbreit BP 50568 Colmar68008 France Technical University of Catalonia Laboratory of Applied Bioacoustics Rambla Exposició Vilanova i la Geltrú Barcelona08800 Spain INFN Sezione di Genova Via Dodecaneso 33 Genova16146 Italy Universitat Politècnica de València C/ Paranimf 1 Gandia46730 Spain Aix Marseille Univ CNRS IN2P3 CPPM Marseille France APC Univ Paris Diderot CNRS IN2P3 CEA Irfu Obs de Paris Sorbonne Paris Cité France c/ Catedrático José Beltrán 2 Paterna ValenciaE-46980 Spain LAM - Laboratoire d’Astrophysique de Marseille Pôle de l’Étoile Site de Château-Gombert rue Frédéric Joliot-Curie 38 Marseille Cedex 1313388 France National Center for Energy Sciences and Nuclear Techniques B.P.1382 RabatR. P.10001 Morocco Via S. Sofia 62 Catania95123 Italy Nikhef Science Park Amsterdam Netherlands Huygens-Kamerlingh Onnes Laboratorium Universiteit Leiden Netherlands Institute of Space Science Mağurele BucharestRO-077125 Romania Universiteit van Amsterdam Instituut voor Hoge-Energie Fysica Science Park 105 Amsterdam1098 XG Netherlands INFN Sezione di Roma P.le Aldo Moro 2 Roma00185 Italy Dipartimento di Fisica Università La Sapienza P.le Aldo Moro 2 Roma00185 Italy Gran Sasso Science Institute Viale Francesco Crispi 7 L’Aquila00167 Italy University Mohammed V in Rabat Faculty of Sciences 4 av. Ibn Battouta B.P. 1014 RabatR.P. 10000 Morocco INFN Sezione di Bologna Viale Berti-Pichat 6/2 Bologna40127 Italy INFN Sezione di Bari Via E. Orabona 4 Bari70126 Italy Department of Computer Architecture and Technology CITIC University of Granada Granada18071 Spain Géoazur UCA CNRS IRD Observatoire de la Côte d’Azur Sophia Antipolis France Dipartimento di Fisica dell’Università Via Dodecaneso 33 Genova16146 Italy Université Paris-Sud Orsay Cedex91405 France Friedrich-Alexander-Universität Erlangen-Nürnberg Erlangen Cent

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 Anticoincidence 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. Copyright © 2017, The Authors. All rights reserved.

关键词： Gravity waves

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Smart sensor architectures for embedded biosignal analysis

Smart sensor architectures for embedded biosignal analysis

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Conference on Design and architectures for Signal and Image Processing

作者： Benjamin Pfundt Marc Reichenbach Björn Eskofier Dietmar Fey Department Computer Science Chair of Computer Architecture Department Computer Science Pattern Recognition Lab Friedrich-Alexander-University Erlangen-Nuremberg Germany

In many sports and medical applications small and wearable sensors are used that capture motion and physiological signals. Yet, commonly such sensor are only capable of acquiring raw data, which is afterwards transmitted to a smartphone or other mobile computing device where processing and classification is carried out. This results in limited usability because another device has to be worn. Moreover, high power consumption due to continuous transmission is a main disadvantage. Therefore, we propose a smart sensor approach that can alleviate these problems by carrying out the processing on the sensor itself. To house the processing schemes in the sensor node we developed a new computer architecture utilizing an FPGA and an ASIC. To show the benefits of the in-sensor processing, we chose two representative biosensor applications: a movement and fall detection system for the elderly and a swimming style recognition system for professional athletes. Compared to conventional approaches the same classification rate can be achieved while saving space, power, weight and setup costs.

关键词： computer architecture Accelerometers Feature extraction Intelligent sensors Monitoring Legged locomotion Pattern recognition

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Situation Recognition for Service Management Systems Using OWL 2 Reasoners

Situation Recognition for Service Management Systems Using O...

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IEEE Workshop on Context Modeling and Reasoning

作者： Waltenegus Dargie Eldora Julian Mendez Christoph Mobius Kateryna Rybina Veronika Thost Anni-Yasmin Turhan Chair of Computer Networks Institute of Systems Architecture Technische Universitat Dresden Chair for Automata Theory Institute for Theoretical Computer Science Technische Universitat Dresden

ISBN: (纸本)9781467350754

For service management systems the early recognition of situations that necessitate a rebinding or a migration of services is an important task. To describe these situations on differing levels of detail and to allow their recognition even if only incomplete information is available, we employ the ontology language OWL 2 and the reasoning services defined for it. In this paper we provide a case study on the performance of state of the art OWL 2 reasoning systems for answering class queries and conjunctive queries modeling the relevant situations for service rebinding or migration in the differing OWL 2 profiles.

关键词： OWL Servers Ontologies Cognition Runtime Hardware Power demand

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Object tracking as job-scheduling problem

Object tracking as job-scheduling problem

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ACM/IEEE International Conference on Distributed Smart Cameras, ICDSC

作者： Uwe Jaenen Henning Spiegelberg Lars Sommer Sebastian von Mammen Juergen Brehm Joerg Haehner Chair for Organic Computing Institute of Computer Science Universität Augsburg Augsburg Germany Department for System-and Computer-Architecture Leibniz Universität Hannover Hannover Germany

This paper establishes a connection between object tracking from a systems point of view and the job-scheduling or job-shop problem. Often, surveillance areas cannot be fully monitored by a set of smart cameras at any given point in time. Decisions have to be made, which objects are to be tracked. The computer vision aspects of object tracking have made substantial strides which permits for elaborately planning the monitoring jobs. In this paper, object tracking is handled as a job-scheduling problem. As a result, tracked objects are considered as scheduling jobs that rely on smart cameras as resources that follow according tracking policies. The presented job-scheduling approach is based on proactive quotations advertised by the jobs. The main advantages of this algorithm are the avoidance of negotiation chains and the acceptance of local non-optimal solutions to benefit the overall performance.

关键词： Cameras Trajectory Smart cameras Object tracking Surveillance Scheduling

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Connected media and presence

Connected media and presence

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2nd International Workshop on Socially-Aware Multimedia, SAM 2013 - Co-located with ACM Multimedia 2013

作者： Kort, Joke Nefs, Harold T. Gullström, Charlie De Greef, Tjerk Parnes, Peter TNO Eemsgolaan 3 9727 DW Groningen Netherlands Delft University of Technology Department of Electrical Engineering Mathematics and Computer Science Mekelweg 4 2628 CD Delft Netherlands KTH Royal Institute of Technology Dept. Architecture 100 44 Stockholm Sweden Lulea University of Technology Department of Computer Science Electrical and Space Engineering 971 87 Luleå Sweden

ISBN: (纸本)9781450323949

Effective design of shared mediated spaces, information and connectedness requires theory and practice from a range of disciplines such as found in European projects like Together Anywhere, Together Anytime (TA2) and the EIT ICT Labs Mediating Presence activity. Building on this work we continue to investigate the changes in the European digital media industry such as changed traditional distribution of media content and the progressive integration of (social) communication means in information distribution and shared mediated spaces. Our past research has given valuable insights in how to design and evaluate systems and services that provide a high quality of experience, in how trust is established in mediated environments, and how the formation of tacit communication between participants in new distributed and connected media is negotiated. In the new Seventh Framework Program project COnnected Media and Presence from European Institute of Technology (COMPEIT) we aim to enhance the quality of experience in face-to-face and broadcast communication further in three domains: 1) Spatial connectedness, 2) Social connectedness and 3) Information connectedness, by developing three key services: Shared Experience with Tangible Interaction (SETI);Broadcast Presence Studio (BPS) and Mixed-Reality Interaction (MRI). The quality of experience of these services will be enhanced in terms of for example: spatial connectedness, by providing shared spaces and supporting spatial features such as eye contact;social connectedness, by using natural means for interaction suiting different settings and activities;and information connectedness, by providing better means to share, manipulate and use information suiting different task or activities. In this paper we will discuss the background of this work and give an overview of our planned future work in COMPEIT. © 2013 ACM.

关键词： Mixed reality

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Multi-paradigm semantics for simulating SysML models using SystemC-AMS

Multi-paradigm semantics for simulating SysML models using S...

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Forum on Specification, Verification and Design Languages, FDL

作者： Daniel Chaves Café Filipe Vinci dos Santos Cécile Hardebolle Christophe Jacquet Frédéric Boulanger Supélec E3S-Computer Science Departement Thales Chair on Advanced Analog System Design Supélec Gif-sur-Yvette France Thales Chair on Advanced Analog System Design Supélec Gif-sur-Yvette France Supélec E3S-Computer Science Departement Supélec Gif-sur-Yvette France

SysML is an industrial standard for the modeling of systems, providing a graphical way to model structure and behavior. Despite its flexibility, SysML lacks semantics to give language elements a precise meaning. Current implementations of the standard allow multiple interpretations of syntactical elements and can cause misunderstandings when porting a model among tools. Our work focuses on the definition of concrete semantics for SysML to enable correct interpretation of heterogeneous models. We also add semantic adaptation elements to guarantee that interactions among different formalisms are unambiguous. We demonstrate our approach by generating SystemC-AMS code automatically from SysML diagrams for a case study with two distinct formalisms. This kind of translation allows the validation of system behavior through simulation.

关键词： Semantics Unified modeling language Adaptation models Computational modeling Standards Engines Mathematical model

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