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19 results on '"Chiarusi T"'

1. ATHENA detector proposal — a totally hermetic electron nucleus apparatus proposed for IP6 at the Electron-Ion Collider

Author

Adam, J, Adamczyk, L, Agrawal, N, Aidala, C, Akers, W, Alekseev, M, Allen, MM, Ameli, F, Angerami, A, Antonioli, P, Apadula, NJ, Aprahamian, A, Armstrong, W, Arratia, M, Arrington, JR, Asaturyan, A, Aschenauer, EC, Augsten, K, Aune, S, Bailey, K, Baldanza, C, Bansal, M, Barbosa, F, Barion, L, Barish, K, Battaglieri, M, Bazilevsky, A, Behera, NK, Berdnikov, V, Bernauer, J, Berriaud, C, Bhasin, A, Bhattacharya, DS, Bielcik, J, Bielcikova, J, Bissolotti, C, Boeglin, W, Bondì, M, Borri, M, Bossù, F, Bouyjou, F, Brandenburg, JD, Bressan, A, Brooks, M, Bültmann, SL, Byer, D, Caines, H, de la Barca Sanchez, M Calderon, Calvelli, V, Camsonne, A, Cappelli, L, Capua, M, Castro, M, Cavazza, D, Cebra, D, Celentano, A, Chakaberia, I, Chan, B, Chang, W, Chartier, M, Chatterjee, C, Chen, D, Chen, J, Chen, K, Chen, Z, Chetri, H, Chiarusi, T, Chiosso, M, Chu, X, Chwastowski, JJ, Cicala, G, Cisbani, E, Cline, E, Cloët, I, Colella, D, Contalbrigo, M, Contin, G, Corliss, R, Corrales-Morales, Y, Crafts, J, Crawford, C, Cruz-Torres, R, D'Ago, D, D'Angelo, A, D'Hose, N, Dainton, J, Torre, S Dalla, Dasgupta, SS, Dash, S, Dashyan, N, Datta, J, Daugherity, M, De Vita, R, Deconinck, W, Defurne, M, Dehmelt, K, Del Dotto, A, Delcarro, F, Dellacasa, G, and Demiroglu, ZS

Subjects
Nuclear and Plasma Physics, Physical Sciences, Large detector systems for particle and astroparticle physics, Calorimeters, Cherenkov detectors, Particle tracking detectors, Engineering, Nuclear & Particles Physics, Physical sciences
Abstract

ATHENA has been designed as a general purpose detector capable of delivering the full scientific scope of the Electron-Ion Collider. Careful technology choices provide fine tracking and momentum resolution, high performance electromagnetic and hadronic calorimetry, hadron identification over a wide kinematic range, and near-complete hermeticity. This article describes the detector design and its expected performance in the most relevant physics channels. It includes an evaluation of detector technology choices, the technical challenges to realizing the detector and the R&D required to meet those challenges.

Published
2022

2. Science Requirements and Detector Concepts for the Electron-Ion Collider EIC Yellow Report

Author

Khalek, R Abdul, Accardi, A, Adam, J, Adamiak, D, Akers, W, Albaladejo, M, Al-bataineh, A, Alexeev, MG, Ameli, F, Antonioli, P, Armesto, N, Armstrong, WR, Arratia, M, Arrington, J, Asaturyan, A, Asai, M, Aschenauer, EC, Aune, S, Avagyan, H, Gayoso, C Ayerbe, Azmoun, B, Bacchetta, A, Baker, MD, Barbosa, F, Barion, L, Barish, KN, Barry, PC, Battaglieri, M, Bazilevsky, A, Behera, NK, Benmokhtar, F, Berdnikov, VV, Bernauer, JC, Bertone, V, Bhattacharya, S, Bissolotti, C, Boer, D, Boglione, M, Bondì, M, Boora, P, Borsa, I, Bossù, F, Bozzi, G, Brandenburg, JD, Brei, N, Bressan, A, Brooks, WK, Bufalino, S, Bukhari, MHS, Burkert, V, Buttimore, NH, Camsonne, A, Celentano, A, Celiberto, FG, Chang, W, Chatterjee, C, Chen, K, Chetry, T, Chiarusi, T, Chien, Y-T, Chiosso, M, Chu, X, Chudakov, E, Cicala, G, Cisbani, E, Cloet, IC, Cocuzza, C, Cole, PL, Colella, D, Collins, JL, Constantinou, M, Contalbrigo, M, Contin, G, Corliss, R, Cosyn, W, Courtoy, A, Crafts, J, Cruz-Torres, R, Cuevas, RC, D'Alesio, U, Torre, S Dalla, Das, D, Dasgupta, SS, Da Silva, C, Deconinck, W, Defurne, M, DeGraw, W, Dehmelt, K, Del Dotto, A, Delcarro, F, Deshpande, A, Detmold, W, De Vita, R, Diefenthaler, M, Dilks, C, Dixit, DU, Dulat, S, Dumitru, A, Dupré, R, and Durham, JM

Subjects
Nuclear and Plasma Physics, Synchrotrons and Accelerators, Physical Sciences, Affordable and Clean Energy, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics, Astronomical sciences, Nuclear and plasma physics, Particle and high energy physics
Abstract

This report describes the physics case, the resulting detector requirements, and the evolving detector concepts for the experimental program at the Electron-Ion Collider (EIC). The EIC will be a powerful new high-luminosity facility in the United States with the capability to collide high-energy electron beams with high-energy proton and ion beams, providing access to those regions in the nucleon and nuclei where their structure is dominated by gluons. Moreover, polarized beams in the EIC will give unprecedented access to the spatial and spin structure of the proton, neutron, and light ions. The studies leading to this document were commissioned and organized by the EIC User Group with the objective of advancing the state and detail of the physics program and developing detector concepts that meet the emerging requirements in preparation for the realization of the EIC. The effort aims to provide the basis for further development of concepts for experimental equipment best suited for the science needs, including the importance of two complementary detectors and interaction regions. This report consists of three volumes. Volume I is an executive summary of our findings and developed concepts. In Volume II we describe studies of a wide range of physics measurements and the emerging requirements on detector acceptance and performance. Volume III discusses general-purpose detector concepts and the underlying technologies to meet the physics requirements. These considerations will form the basis for a world-class experimental program that aims to increase our understanding of the fundamental structure of all visible matter.

Published
2022

3. Search for Spatial Correlations of Neutrinos with Ultra-high-energy Cosmic Rays

Author

collaboration, The ANTARES, Albert, A, Alves, S, André, M, Anghinolfi, M, A., M, Ardid, S, Aubert, J-J, Aublin, J, Baret, B, Basa, S, Belhorma, B, Bendahman, M, Bertin, V, Biagi, S, Bissinger, M, Boumaaza, J, Bouta, M, Bouwhuis, MC, Brânzaş, H, Bruijn, R, Brunner, J, Busto, J, Caiffi, B, Calvo, D, Capone, A, Caramete, L, Carr, J, Carretero, V, Celli, S, Chabab, M, Chau, TN, Moursli, R Cherkaoui El, Chiarusi, T, Circella, M, Coleiro, A, Coniglione, R, Coyle, P, Creusot, A, Díaz, AF, Distefano, C, Di Palma, I, Domi, A, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, van Eeden, T, van Eijk, D, Khayati, N El, Enzenhöfer, A, Fermani, P, Ferrara, G, Filippini, F, Fusco, L, Gatelet, Y, Gay, P, Glotin, H, Gozzini, R, Ruiz, R Gracia, Graf, K, Guidi, C, Hallmann, S, van Haren, H, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hössl, J, Hofestädt, J, Huang, F, Illuminati, G, James, CW, Jisse-Jung, B, De Jong, M, de Jong, P, Kadler, M, Kalekin, O, Katz, U, Khan-Chowdhury, NR, Kouchner, A, Kreykenbohm, I, Kulikovskiy, V, Lahmann, R, Le Breton, R, LeStum, S, Lefèvre, D, Leonora, E, Levi, G, Lopez-Coto, D, Loucatos, S, Maderer, L, Manczak, J, Marcelin, M, Margiotta, A, Marinelli, A, Martínez-Mora, JA, Martino, B, Melis, K, Migliozzi, P, and Moussa, A

Subjects
Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, Neutrino astronomy, High energy astrophysics, Ultra-high-energy cosmic radiation, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural), Astronomy & Astrophysics, Astronomical sciences, Particle and high energy physics, Space sciences
Abstract

For several decades, the origin of ultra-high-energy cosmic rays (UHECRs) has been an unsolved question of high-energy astrophysics. One approach for solving this puzzle is to correlate UHECRs with high-energy neutrinos, since neutrinos are a direct probe of hadronic interactions of cosmic rays and are not deflected by magnetic fields. In this paper, we present three different approaches for correlating the arrival directions of neutrinos with the arrival directions of UHECRs. The neutrino data are provided by the IceCube Neutrino Observatory and ANTARES, while the UHECR data with energies above ∼50 EeV are provided by the Pierre Auger Observatory and the Telescope Array. All experiments provide increased statistics and improved reconstructions with respect to our previous results reported in 2015. The first analysis uses a high-statistics neutrino sample optimized for point-source searches to search for excesses of neutrino clustering in the vicinity of UHECR directions. The second analysis searches for an excess of UHECRs in the direction of the highest-energy neutrinos. The third analysis searches for an excess of pairs of UHECRs and highest-energy neutrinos on different angular scales. None of the analyses have found a significant excess, and previously reported overfluctuations are reduced in significance. Based on these results, we further constrain the neutrino flux spatially correlated with UHECRs.

Published
2022

4. Combined search for neutrinos from dark matter self-annihilation in the Galactic Center with ANTARES and IceCube

Author

Albert, A, Andre, M, Anghinolfi, M, Ardid, M, Aubert, J-J, Aublin, J, Baret, B, Basa, S, Belhorma, B, Bertin, V, Biagi, S, Bissinger, M, Boumaaza, J, Bouta, M, Bouwhuis, MC, Branzas, H, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chabab, M, Chau, TN, El Moursli, R Cherkaoui, Chiarusi, T, Circella, M, Coleiro, A, Colomer, M, Coniglione, R, Coyle, P, Creusot, A, Diaz, AF, Deschamps, A, Distefano, C, Di Palma, I, Domi, A, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, El Khayati, N, Enzenhoefer, A, Ettahiri, A, Fermani, P, Ferrara, G, Filippini, F, Fusco, L, Gay, P, Glotin, H, Gozzini, R, Ruiz, R Gracia, Graf, K, Guidi, C, Hallmann, S, van Haren, H, Heijboer, AJ, Hello, Y, Hernandez-Rey, JJ, Hoessl, J, Hofestaedt, J, Huang, F, Illuminati, G, James, CW, de Jong, M, de Jong, P, Jongen, M, Kadler, M, Kalekin, O, Katz, U, Khan-Chowdhury, NR, Kouchner, A, Kreykenbohm, I, Kulikovskiy, V, Lahmann, R, Le Breton, R, Lefevre, D, Leonora, E, Levi, G, Lincetto, M, Lopez-Coto, D, Loucatos, S, Maggi, G, Manczak, J, Marcelin, M, Margiotta, A, Marinelli, A, Martinez-Mora, JA, Mele, R, Melis, K, Migliozzi, P, Moser, M, Moussa, A, Muller, R, Nauta, L, Navas, S, Nezri, E, Nielsen, C, and Nunez-Castineyra, A

Subjects
astro-ph.HE
Abstract

We present the results of the first combined dark matter search targeting theGalactic Centre using the ANTARES and IceCube neutrino telescopes. For darkmatter particles with masses from 50 to 1000 GeV, the sensitivities on theself-annihilation cross section set by ANTARES and IceCube are comparable,making this mass range particularly interesting for a joint analysis. Darkmatter self-annihilation through the $\tau^+\tau^-$, $\mu^+\mu^-$, $b\bar{b}$and $W^+W^-$ channels is considered for both the Navarro-Frenk-White andBurkert halo profiles. In the combination of 2,101.6 days of ANTARES data and1,007 days of IceCube data, no excess over the expected background is observed.Limits on the thermally-averaged dark matter annihilation cross section$\langle\sigma_A\upsilon\rangle$ are set. These limits present an improvementof up to a factor of two in the studied dark matter mass range with respect tothe individual limits published by both collaborations. When considering darkmatter particles with a mass of 200 GeV annihilating through the $\tau^+\tau^-$channel, the value obtained for the limit is $7.44 \times 10^{-24}\text{cm}^{3}\text{s}^{-1}$ for the Navarro-Frenk-White halo profile. For thepurpose of this joint analysis, the model parameters and the likelihood areunified, providing a benchmark for forthcoming dark matter searches performedby neutrino telescopes.

Published
2020

5. Combined search for neutrinos from dark matter self-annihilation in the Galactic Center with ANTARES and IceCube

Author

Albert, A, André, M, Anghinolfi, M, Ardid, M, Aubert, J-J, Aublin, J, Baret, B, Basa, S, Belhorma, B, Bertin, V, Biagi, S, Bissinger, M, Boumaaza, J, Bouta, M, Bouwhuis, MC, Brânzaş, H, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chabab, M, Chau, TN, Moursli, R Cherkaoui El, Chiarusi, T, Circella, M, Coleiro, A, Colomer, M, Coniglione, R, Coyle, P, Creusot, A, Díaz, AF, Deschamps, A, Distefano, C, Di Palma, I, Domi, A, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, Khayati, N El, Enzenhöfer, A, Ettahiri, A, Fermani, P, Ferrara, G, Filippini, F, Fusco, L, Gay, P, Glotin, H, Gozzini, R, Ruiz, R Gracia, Graf, K, Guidi, C, Hallmann, S, van Haren, H, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hößl, J, Hofestädt, J, Huang, F, Illuminati, G, James, CW, de Jong, M, de Jong, P, Jongen, M, Kadler, M, Kalekin, O, Katz, U, Khan-Chowdhury, NR, Kouchner, A, Kreykenbohm, I, Kulikovskiy, V, Lahmann, R, Le Breton, R, Lefèvre, D, Leonora, E, Levi, G, Lincetto, M, Lopez-Coto, D, Loucatos, S, Maggi, G, Manczak, J, Marcelin, M, Margiotta, A, Marinelli, A, Martínez-Mora, JA, Mele, R, Melis, K, Migliozzi, P, Moser, M, Moussa, A, Muller, R, Nauta, L, Navas, S, Nezri, E, Nielsen, C, and Nuñez-Castiñeyra, A

Subjects
Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, astro-ph.HE, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics, Mathematical physics, Astronomical sciences, Particle and high energy physics
Abstract

We present the results of the first combined dark matter search targeting the Galactic Center using the ANTARES and IceCube neutrino telescopes. For dark matter particles with masses from 50 to 1000 GeV, the sensitivities on the self-annihilation cross section set by ANTARES and IceCube are comparable, making this mass range particularly interesting for a joint analysis. Dark matter self-annihilation through the τþτ−, μþμ−, bb¯, and WþW− channels is considered for both the Navarro-Frenk-White and Burkert halo profiles. In the combination of 2101.6 days of ANTARES data and 1007 days of IceCube data, no excess over the expected background is observed. Limits on the thermally averaged dark matter annihilation cross section hσAυi are set. These limits present an improvement of up to a factor of 2 in the studied dark matter mass range with respect to the individual limits published by both collaborations. When considering dark matter particles with a mass of 200 GeV annihilating through the τþτ− channel, the value obtained for the limit is 7.44 × 10−24 cm3 s−1 for the Navarro-Frenk-White halo profile. For the purpose of this joint analysis, the model parameters and the likelihood are unified, providing a benchmark for forthcoming dark matter searches performed by neutrino telescopes.

Published
2020

6. ANTARES and IceCube Combined Search for Neutrino Point-like and Extended Sources in the Southern Sky

Author

Albert, A, André, M, Anghinolfi, M, Anton, G, Ardid, M, Aubert, JJ, Aublin, J, Baret, B, Basa, S, Belhorma, B, Bertin, V, Biagi, S, Bissinger, M, Boumaaza, J, Bourret, S, Bouta, M, Bouwhuis, MC, Brânzaş, H, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chabab, M, Chau, TN, El Moursli, RC, Chiarusi, T, Circella, M, Coleiro, A, Colomer, M, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Diáz, AF, Wasseige, GD, Deschamps, A, Distefano, C, Palma, ID, Domi, A, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, Bojaddaini, IE, Khayati, NE, Elsässer, D, Enzenhöfer, A, Ettahiri, A, Fassi, F, Fermani, P, Ferrara, G, Filippini, F, Fusco, L, Gay, P, Glotin, H, Gozzini, R, Ruiz, RG, Graf, K, Guidi, C, Hallmann, S, Van Haren, H, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hößl, J, Hofestädt, J, Illuminati, G, James, CW, Jong, MD, Jong, PD, Jongen, M, Kadler, M, Kalekin, O, Katz, U, Khan-Chowdhury, NR, Kouchner, A, Kreter, M, Kreykenbohm, I, Kulikovskiy, V, Lahmann, R, Breton, RL, Lefèvre, D, Leonora, E, Levi, G, Lincetto, M, Lopez-Coto, D, Loucatos, S, Maggi, G, Manczak, J, Marcelin, M, Margiotta, A, Marinelli, A, Martínez-Mora, JA, Mele, R, Melis, K, Migliozzi, P, and Moser, M

Subjects
astro-ph.HE, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry, Astronomy & Astrophysics, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural)
Abstract

A search for point-like and extended sources of cosmic neutrinos using data collected by the ANTARES and IceCube neutrino telescopes is presented. The data set consists of all the track-like and shower-like events pointing in the direction of the Southern Sky included in the nine-year ANTARES point-source analysis, combined with the throughgoing track-like events used in the seven-year IceCube point-source search. The advantageous field of view of ANTARES and the large size of IceCube are exploited to improve the sensitivity in the Southern Sky by a factor of ∼2 compared to both individual analyses. In this work, the Southern Sky is scanned for possible excesses of spatial clustering, and the positions of preselected candidate sources are investigated. In addition, special focus is given to the region around the Galactic Center, whereby a dedicated search at the location of SgrA∗ is performed, and to the location of the supernova remnant RXJ 1713.7-3946. No significant evidence for cosmic neutrino sources is found, and upper limits on the flux from the various searches are presented.

Published
2020

7. ANTARES and IceCube Combined Search for Neutrino Point-like and Extended Sources in the Southern Sky

Author

Albert, A, André, M, Anghinolfi, M, Anton, G, Ardid, M, Aubert, J-J, Aublin, J, Baret, B, Basa, S, Belhorma, B, Bertin, V, Biagi, S, Bissinger, M, Boumaaza, J, Bourret, S, Bouta, M, Bouwhuis, MC, Brânzaş, H, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chabab, M, Chau, TN, Moursli, R Cherkaoui El, Chiarusi, T, Circella, M, Coleiro, A, Colomer, M, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Díaz, AF, de Wasseige, G, Deschamps, A, Distefano, C, Di Palma, I, Domi, A, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, Bojaddaini, I El, Khayati, N El, Elsässer, D, Enzenhöfer, A, Ettahiri, A, Fassi, F, Fermani, P, Ferrara, G, Filippini, F, Fusco, L, Gay, P, Glotin, H, Gozzini, R, Ruiz, R Gracia, Graf, K, Guidi, C, Hallmann, S, van Haren, H, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hößl, J, Hofestädt, J, Illuminati, G, James, CW, de Jong, M, de Jong, P, Jongen, M, Kadler, M, Kalekin, O, Katz, U, Khan-Chowdhury, NR, Kouchner, A, Kreter, M, Kreykenbohm, I, Kulikovskiy, V, Lahmann, R, Le Breton, R, Lefèvre, D, Leonora, E, Levi, G, Lincetto, M, Lopez-Coto, D, Loucatos, S, Maggi, G, Manczak, J, Marcelin, M, Margiotta, A, Marinelli, A, Martínez-Mora, JA, Mele, R, Melis, K, Migliozzi, P, and Moser, M

Subjects
Particle and High Energy Physics, Physical Sciences, astro-ph.HE, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural), Astronomy & Astrophysics, Astronomical sciences, Particle and high energy physics, Space sciences
Abstract

A search for point-like and extended sources of cosmic neutrinos using data collected by the ANTARES and IceCube neutrino telescopes is presented. The data set consists of all the track-like and shower-like events pointing in the direction of the Southern Sky included in the nine-year ANTARES point-source analysis, combined with the throughgoing track-like events used in the seven-year IceCube point-source search. The advantageous field of view of ANTARES and the large size of IceCube are exploited to improve the sensitivity in the Southern Sky by a factor of ∼2 compared to both individual analyses. In this work, the Southern Sky is scanned for possible excesses of spatial clustering, and the positions of preselected candidate sources are investigated. In addition, special focus is given to the region around the Galactic Center, whereby a dedicated search at the location of SgrA∗ is performed, and to the location of the supernova remnant RXJ 1713.7-3946. No significant evidence for cosmic neutrino sources is found, and upper limits on the flux from the various searches are presented.

Published
2020

8. Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube

Author

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, Boumaaza, J, Bourret, S, Bouwhuis, MC, Brânzaş, H, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chabab, M, Moursli, R Cherkaoui El, Chiarusi, T, Circella, M, Coelho, JAB, Coleiro, A, Colomer, M, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Díaz, AF, Deschamps, A, Distefano, C, Di Palma, I, Domi, A, Donà, R, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, Bojaddaini, I El, Khayati, N El, Elsässer, D, Enzenhöfer, A, Ettahiri, A, Fassi, F, Felis, I, Fermani, P, Ferrara, G, Fusco, L, Gay, P, Glotin, H, Grégoire, T, Ruiz, R Gracia, Graf, K, Hallmann, S, van Haren, H, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hößl, J, Hofestädt, J, Illuminati, G, de Jong, M, Jongen, M, Kadler, M, Kalekin, O, Katz, U, Khan-Chowdhury, NR, Kouchner, A, Kreter, M, Kreykenbohm, I, Kulikovskiy, V, Lachaud, C, Lahmann, R, Lefèvre, D, Leonora, E, Levi, G, Lotze, M, Loucatos, S, Maggi, G, Marcelin, M, Margiotta, A, Marinelli, A, Martínez-Mora, JA, Mele, R, Melis, K, Migliozzi, P, Moussa, A, Navas, S, Nezri, E, Nuñez, A, Organokov, M, and Păvălaş, GE

Subjects
Nuclear and Plasma Physics, Particle and High Energy Physics, Astronomical Sciences, Physical Sciences, gravitational waves, neutrinos, astro-ph.HE, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural), Astronomy & Astrophysics, Astronomical sciences, Particle and high energy physics, Space sciences
Abstract

Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. High-energy neutrinos are signatures of such outflows. The detection of gravitational waves and high-energy neutrinos from common sources could help establish the connection between the dynamics of the progenitor and the properties of the outflow. We searched for associated emission of gravitational waves and high-energy neutrinos from astrophysical transients with minimal assumptions using data from Advanced LIGO from its first observing run O1, and data from the Antares and IceCube neutrino observatories from the same time period. We focused on candidate events whose astrophysical origins could not be determined from a single messenger. We found no significant coincident candidate, which we used to constrain the rate density of astrophysical sources dependent on their gravitational-wave and neutrino emission processes.

Published
2019

9. Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube

Author

Albert, A, André, M, Anghinolfi, M, Ardid, M, Aubert, JJ, Aublin, J, Avgitas, T, Baret, B, Barrios-Martí, J, Basa, S, Belhorma, B, Bertin, V, Biagi, S, Bormuth, R, Boumaaza, J, Bourret, S, Bouwhuis, MC, Brânzaş, H, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chabab, M, El Moursli, RC, Chiarusi, T, Circella, M, Coelho, JAB, Coleiro, A, Colomer, M, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Díaz, AF, Deschamps, A, Distefano, C, Di Palma, I, Domi, A, Donà, R, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, El Bojaddaini, I, El Khayati, N, Elsässer, D, Enzenhöfer, A, Ettahiri, A, Fassi, F, Felis, I, Fermani, P, Ferrara, G, Fusco, L, Gay, P, Glotin, H, Grégoire, T, Ruiz, RG, Graf, K, Hallmann, S, Van Haren, H, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hößl, J, Hofestädt, J, Illuminati, G, De Jong, M, Jongen, M, Kadler, M, Kalekin, O, Katz, U, Khan-Chowdhury, NR, Kouchner, A, Kreter, M, Kreykenbohm, I, Kulikovskiy, V, Lachaud, C, Lahmann, R, Lefèvre, D, Leonora, E, Levi, G, Lotze, M, Loucatos, S, Maggi, G, Marcelin, M, Margiotta, A, Marinelli, A, Martínez-Mora, JA, Mele, R, Melis, K, Migliozzi, P, Moussa, A, Navas, S, Nezri, E, Nuñez, A, Organokov, M, and Pǎvǎlaş, GE

Subjects
gravitational waves, neutrinos, astro-ph.HE, Astronomy & Astrophysics, Astronomical and Space Sciences, Organic Chemistry, Physical Chemistry, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural)
Abstract

Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. High-energy neutrinos are signatures of such outflows. The detection of gravitational waves and high-energy neutrinos from common sources could help establish the connection between the dynamics of the progenitor and the properties of the outflow. We searched for associated emission of gravitational waves and high-energy neutrinos from astrophysical transients with minimal assumptions using data from Advanced LIGO from its first observing run O1, and data from the Antares and IceCube neutrino observatories from the same time period. We focused on candidate events whose astrophysical origins could not be determined from a single messenger. We found no significant coincident candidate, which we used to constrain the rate density of astrophysical sources dependent on their gravitational-wave and neutrino emission processes.

Published
2019

10. Joint Constraints on Galactic Diffuse Neutrino Emission from the ANTARES and IceCube Neutrino Telescopes

Author

Albert, A, André, M, Anghinolfi, M, Ardid, M, Aubert, JJ, Aublin, J, Avgitas, T, Baret, B, Barrios-Martí, J, Basa, S, Belhorma, B, Bertin, V, Biagi, S, Bormuth, R, Boumaaza, J, Bourret, S, Bouwhuis, MC, Brânzaş, H, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chabab, M, El Moursli, RC, Chiarusi, T, Circella, M, Coelho, JAB, Coleiro, A, Colomer, M, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Díaz, AF, Deschamps, A, Distefano, C, Palma, ID, Domi, A, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, Bojaddaini, IE, Khayati, NE, Elsässer, D, Enzenhöfer, A, Ettahiri, A, Fassi, F, Felis, I, Fermani, P, Ferrara, G, Fusco, L, Gay, P, Glotin, H, Grégoire, T, Ruiz, RG, Graf, K, Hallmann, S, Haren, HV, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hößl, J, Hofestädt, J, Illuminati, G, James, CW, Jong, MD, Jongen, M, Kadler, M, Kalekin, O, Katz, U, Khan-Chowdhury, NR, Kouchner, A, Kreter, M, Kreykenbohm, I, Kulikovskiy, V, Lachaud, C, Lahmann, R, Lefèvre, D, Leonora, E, Levi, G, Lotze, M, Loucatos, S, Marcelin, M, Margiotta, A, Marinelli, A, Martínez-Mora, JA, Mele, R, Melis, K, Migliozzi, P, Moussa, A, Navas, S, Nezri, E, Nuñez, A, Organokov, M, Pǎvǎlaş, GE, and Pellegrino, C

Subjects
astro-ph.HE, Astronomy & Astrophysics, Astronomical and Space Sciences
Abstract

The existence of diffuse Galactic neutrino production is expected from cosmic-ray interactions with Galactic gas and radiation fields. Thus, neutrinos are a unique messenger offering the opportunity to test the products of Galactic cosmic-ray interactions up to energies of hundreds of TeV. Here we present a search for this production using ten years of Astronomy with a Neutrino Telescope and Abyss environmental RESearch (ANTARES) track and shower data, as well as seven years of IceCube track data. The data are combined into a joint likelihood test for neutrino emission according to the KRAg model assuming a 5 PeV per nucleon Galactic cosmic-ray cutoff. No significant excess is found. As a consequence, the limits presented in this Letter start constraining the model parameter space for Galactic cosmic-ray production and transport.

Published
2018

11. Joint Constraints on Galactic Diffuse Neutrino Emission from the ANTARES and IceCube Neutrino Telescopes

Author

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, Boumaaza, J, Bourret, S, Bouwhuis, MC, Brânzaş, H, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chabab, M, Moursli, R Cherkaoui El, Chiarusi, T, Circella, M, Coelho, JAB, Coleiro, A, Colomer, M, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Díaz, AF, Deschamps, A, Distefano, C, Di Palma, I, Domi, A, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, Bojaddaini, I El, Khayati, N El, Elsässer, D, Enzenhöfer, A, Ettahiri, A, Fassi, F, Felis, I, Fermani, P, Ferrara, G, Fusco, L, Gay, P, Glotin, H, Grégoire, T, Ruiz, R Gracia, Graf, K, Hallmann, S, van Haren, H, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hößl, J, Hofestädt, J, Illuminati, G, James, CW, de Jong, M, Jongen, M, Kadler, M, Kalekin, O, Katz, U, Khan-Chowdhury, NR, Kouchner, A, Kreter, M, Kreykenbohm, I, Kulikovskiy, V, Lachaud, C, Lahmann, R, Lefèvre, D, Leonora, E, Levi, G, Lotze, M, Loucatos, S, Marcelin, M, Margiotta, A, Marinelli, A, Martínez-Mora, JA, Mele, R, Melis, K, Migliozzi, P, Moussa, A, Navas, S, Nezri, E, Nuñez, A, Organokov, M, Păvălaş, GE, and Pellegrino, C

Subjects
Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, astro-ph.HE, Astronomical and Space Sciences, Astronomy & Astrophysics, Astronomical sciences, Space sciences
Abstract

The existence of diffuse Galactic neutrino production is expected from cosmic-ray interactions with Galactic gas and radiation fields. Thus, neutrinos are a unique messenger offering the opportunity to test the products of Galactic cosmic-ray interactions up to energies of hundreds of TeV. Here we present a search for this production using ten years of Astronomy with a Neutrino Telescope and Abyss environmental RESearch (ANTARES) track and shower data, as well as seven years of IceCube track data. The data are combined into a joint likelihood test for neutrino emission according to the KRAg model assuming a 5 PeV per nucleon Galactic cosmic-ray cutoff. No significant excess is found. As a consequence, the limits presented in this Letter start constraining the model parameter space for Galactic cosmic-ray production and transport.

Published
2018

12. Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory

Author

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, MC, Brânzaş, H, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Moursli, R Cherkaoui El, Chiarusi, T, Circella, M, Coelho, JAB, Coleiro, A, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Díaz, AF, Deschamps, A, De Bonis, G, Distefano, C, Di Palma, I, Domi, A, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, Bojaddaini, I El, Khayati, N El, Elsässer, D, Enzenhöfer, A, Ettahiri, A, Fassi, F, Felis, I, Fusco, LA, Gay, P, Giordano, V, Glotin, H, Grégoire, T, Ruiz, R Gracia, Graf, K, Hallmann, S, van Haren, H, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hößl, J, Hofestädt, J, Illuminati, G, James, CW, 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, JA, Mele, R, Melis, K, Michael, T, Migliozzi, P, Moussa, A, Navas, S, Nezri, E, Organokov, M, Păvălaş, GE, Pellegrino, C, Perrina, C, Piattelli, P, Popa, V, and Pradier, T

Subjects
Nuclear and Plasma Physics, Astronomical Sciences, Physical Sciences, gamma-ray burst: general, gravitational waves, neutrinos, astro-ph.HE, Astronomical and Space Sciences, Astronomy & Astrophysics, Astronomical sciences, Space sciences
Abstract

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.

Published
2017

13. Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory

Author

Albert, A, André, M, Anghinolfi, M, Ardid, M, Aubert, JJ, Aublin, J, Avgitas, T, Baret, B, Barrios-Martí, J, Basa, S, Belhorma, B, Bertin, V, Biagi, S, Bormuth, R, Bourret, S, Bouwhuis, MC, Brânzaş, H, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, El Moursli, RC, Chiarusi, T, Circella, M, Coelho, JAB, Coleiro, A, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Díaz, AF, Deschamps, A, De Bonis, G, Distefano, C, Di Palma, I, Domi, A, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, Bojaddaini, IE, Khayati, NE, Elsässer, D, Enzenhöfer, A, Ettahiri, A, Fassi, F, Felis, I, Fusco, LA, Gay, P, Giordano, V, Glotin, H, Grégoire, T, Ruiz, RG, Graf, K, Hallmann, S, Van Haren, H, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hößl, J, Hofestädt, J, Illuminati, G, James, CW, De Jong, MD, 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, JA, Mele, R, Melis, K, Michael, T, Migliozzi, P, Moussa, A, Navas, S, Nezri, E, Organokov, M, Pǎvǎlaş, GE, Pellegrino, C, Perrina, C, Piattelli, P, Popa, V, and Pradier, T

Subjects
gamma-ray burst: general, gravitational waves, neutrinos, astro-ph.HE, Astronomy & Astrophysics, Astronomical and Space Sciences
Abstract

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.

Published
2017

14. Search for high-energy neutrinos from gravitational wave event GW151226 and candidate LVT151012 with ANTARES and IceCube

Author

Albert, A, André, M, Anghinolfi, M, Anton, G, Ardid, M, Aubert, J-J, Avgitas, T, Baret, B, Barrios-Martí, J, Basa, S, Bertin, V, Biagi, S, Bormuth, R, Bourret, S, Bouwhuis, MC, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chiarusi, T, Circella, M, Coelho, JAB, Coleiro, A, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Deschamps, A, De Bonis, G, Distefano, C, Di Palma, I, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, Bojaddaini, I El, Elsässer, D, Enzenhöfer, A, Felis, I, Fusco, LA, Galatà, S, Gay, P, Giordano, V, Glotin, H, Grégoire, T, Ruiz, R Gracia, Graf, K, Hallmann, S, van Haren, H, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hößl, J, Hofestädt, J, Hugon, C, Illuminati, G, James, CW, 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, JA, Mathieu, A, Mele, R, Melis, K, Michael, T, Migliozzi, P, Moussa, A, Nezri, E, Păvălaş, GE, Pellegrino, C, Perrina, C, Piattelli, P, Popa, V, Pradier, T, Quinn, L, Racca, C, Riccobene, G, Sánchez-Losa, A, Saldaña, M, Salvadori, I, and Samtleben, DFE

Subjects
astro-ph.HE, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics
Abstract

The Advanced LIGO observatories detected gravitational waves from two binary black hole mergers during their first observation run (O1). We present a high-energy neutrino follow-up search for the second gravitational wave event, GW151226, as well as for gravitational wave candidate LVT151012. We find two and four neutrino candidates detected by IceCube, and one and zero detected by Antares, within ±500 s around the respective gravitational wave signals, consistent with the expected background rate. None of these neutrino candidates are found to be directionally coincident with GW151226 or LVT151012. We use nondetection to constrain isotropic-equivalent high-energy neutrino emission from GW151226, adopting the GW event's 3D localization, to less than 2×1051-2×1054 erg.

Published
2017

15. Search for high-energy neutrinos from gravitational wave event GW151226 and candidate LVT151012 with ANTARES and IceCube

Author

Albert, A, André, M, Anghinolfi, M, Anton, G, Ardid, M, Aubert, JJ, Avgitas, T, Baret, B, Barrios-Martí, J, Basa, S, Bertin, V, Biagi, S, Bormuth, R, Bourret, S, Bouwhuis, MC, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chiarusi, T, Circella, M, Coelho, JAB, Coleiro, A, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Deschamps, A, De Bonis, G, Distefano, C, Di Palma, I, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, El Bojaddaini, I, Elsässer, D, Enzenhöfer, A, Felis, I, Fusco, LA, Galatà, S, Gay, P, Giordano, V, Glotin, H, Grégoire, T, Gracia Ruiz, R, Graf, K, Hallmann, S, Van Haren, H, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hößl, J, Hofestädt, J, Hugon, C, Illuminati, G, James, CW, 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, JA, Mathieu, A, Mele, R, Melis, K, Michael, T, Migliozzi, P, Moussa, A, Nezri, E, Pavalaş, GE, Pellegrino, C, Perrina, C, Piattelli, P, Popa, V, Pradier, T, Quinn, L, Racca, C, Riccobene, G, Sánchez-Losa, A, Saldaña, M, Salvadori, I, and Samtleben, DFE

Subjects
astro-ph.HE
Abstract

The Advanced LIGO observatories detected gravitational waves from two binary black hole mergers during their first observation run (O1). We present a high-energy neutrino follow-up search for the second gravitational wave event, GW151226, as well as for gravitational wave candidate LVT151012. We find two and four neutrino candidates detected by IceCube, and one and zero detected by Antares, within ±500 s around the respective gravitational wave signals, consistent with the expected background rate. None of these neutrino candidates are found to be directionally coincident with GW151226 or LVT151012. We use nondetection to constrain isotropic-equivalent high-energy neutrino emission from GW151226, adopting the GW event's 3D localization, to less than 2×1051-2×1054 erg.

Published
2017

16. High-energy neutrino follow-up search of gravitational wave event GW150914 with ANTARES and IceCube

Author

Adrián-Martínez, S, Albert, A, André, M, Anghinolfi, M, Anton, G, Ardid, M, Aubert, JJ, Avgitas, T, Baret, B, Barrios-Martí, J, Basa, S, Bertin, V, Biagi, S, Bormuth, R, Bouwhuis, MC, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chiarusi, T, Circella, M, Coleiro, A, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Deschamps, A, De Bonis, G, Distefano, C, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, El Bojaddaini, I, Elsässer, D, Enzenhöfer, A, Fehn, K, Felis, I, Fusco, LA, Galatà, S, Gay, P, Geißelsöder, S, Geyer, K, Giordano, V, Gleixner, A, Glotin, H, Gracia-Ruiz, R, Graf, K, Hallmann, S, Van Haren, H, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hößl, J, Hofestädt, J, Hugon, C, Illuminati, G, James, CW, 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, JA, Mathieu, A, Melis, K, Michael, T, Migliozzi, P, Moussa, A, Mueller, C, Nezri, E, PǍvǍlaş, GE, Pellegrino, C, Perrina, C, Piattelli, P, Popa, V, Pradier, T, Racca, C, Riccobene, G, Roensch, K, Saldaña, M, Samtleben, DFE, Sánchez-Losa, A, and Sanguineti, M

Subjects
astro-ph.HE
Abstract

We present the high-energy-neutrino follow-up observations of the first gravitational wave transient GW150914 observed by the Advanced LIGO detectors on September 14, 2015. We search for coincident neutrino candidates within the data recorded by the IceCube and Antares neutrino detectors. A possible joint detection could be used in targeted electromagnetic follow-up observations, given the significantly better angular resolution of neutrino events compared to gravitational waves. We find no neutrino candidates in both temporal and spatial coincidence with the gravitational wave event. Within ±500 s of the gravitational wave event, the number of neutrino candidates detected by IceCube and Antares were three and zero, respectively. This is consistent with the expected atmospheric background, and none of the neutrino candidates were directionally coincident with GW150914. We use this nondetection to constrain neutrino emission from the gravitational-wave event.

Published
2016

17. High-energy neutrino follow-up search of gravitational wave event GW150914 with ANTARES and IceCube

Author

Adrián-Martínez, S, Albert, A, André, M, Anghinolfi, M, Anton, G, Ardid, M, Aubert, J-J, Avgitas, T, Baret, B, Barrios-Martí, J, Basa, S, Bertin, V, Biagi, S, Bormuth, R, Bouwhuis, MC, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chiarusi, T, Circella, M, Coleiro, A, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Deschamps, A, De Bonis, G, Distefano, C, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, Bojaddaini, I El, Elsässer, D, Enzenhöfer, A, Fehn, K, Felis, I, Fusco, LA, Galatà, S, Gay, P, Geißelsöder, S, Geyer, K, Giordano, V, Gleixner, A, Glotin, H, Gracia-Ruiz, R, Graf, K, Hallmann, S, van Haren, H, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hößl, J, Hofestädt, J, Hugon, C, Illuminati, G, James, CW, 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, JA, Mathieu, A, Melis, K, Michael, T, Migliozzi, P, Moussa, A, Mueller, C, Nezri, E, Păvălaş, GE, Pellegrino, C, Perrina, C, Piattelli, P, Popa, V, Pradier, T, Racca, C, Riccobene, G, Roensch, K, Saldaña, M, Samtleben, DFE, Sánchez-Losa, A, and Sanguineti, M

Subjects
Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, astro-ph.HE
Abstract

We present the high-energy-neutrino follow-up observations of the first gravitational wave transient GW150914 observed by the Advanced LIGO detectors on September 14, 2015. We search for coincident neutrino candidates within the data recorded by the IceCube and Antares neutrino detectors. A possible joint detection could be used in targeted electromagnetic follow-up observations, given the significantly better angular resolution of neutrino events compared to gravitational waves. We find no neutrino candidates in both temporal and spatial coincidence with the gravitational wave event. Within ±500 s of the gravitational wave event, the number of neutrino candidates detected by IceCube and Antares were three and zero, respectively. This is consistent with the expected atmospheric background, and none of the neutrino candidates were directionally coincident with GW150914. We use this nondetection to constrain neutrino emission from the gravitational-wave event.

Published
2016

18. THE FIRST COMBINED SEARCH FOR NEUTRINO POINT-SOURCES IN THE SOUTHERN HEMISPHERE WITH THE ANTARES AND ICECUBE NEUTRINO TELESCOPES

Author

Adrián-Martínez, S, Albert, A, André, M, Anton, G, Ardid, M, Aubert, J-J, Baret, B, Barrios-Martí, J, Basa, S, Bertin, V, Biagi, S, Bormuth, R, Bouwhuis, MC, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Chiarusi, T, Circella, M, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Dekeyser, I, Deschamps, A, De Bonis, G, Distefano, C, Donzaud, C, Dornic, D, Drouhin, D, Dumas, A, Eberl, T, Elsässer, D, Enzenhöfer, A, Fehn, K, Felis, I, Fermani, P, Folger, F, Fusco, LA, Galatà, S, Gay, P, Geißelsöder, S, Geyer, K, Giordano, V, Gleixner, A, Gracia-Ruiz, R, Graf, K, Hallmann, S, van Haren, H, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hößl, J, Hofestädt, J, Hugon, C, James, CW, de Jong, M, Kadler, M, Kalekin, O, Katz, U, Kießling, D, Kooijman, P, Kouchner, A, Kreter, M, Kreykenbohm, I, Kulikovskiy, V, Lahmann, R, Lefèvre, D, Leonora, E, Loucatos, S, Marcelin, M, Margiotta, A, Marinelli, A, Martínez-Mora, JA, Mathieu, A, Michael, T, Migliozzi, P, Moussa, A, Mueller, C, Nezri, E, Păvălaş, GE, Pellegrino, C, Perrina, C, Piattelli, P, Popa, V, Pradier, T, Racca, C, Riccobene, G, Richter, R, Roensch, K, Saldaña, M, Samtleben, DFE, Sánchez-Losa, A, Sanguineti, M, Sapienza, P, Schmid, J, Schnabel, J, and Schüssler, F

Subjects
astroparticle physics, neutrinos, hep-ex, astro-ph.HE, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural), Astronomy & Astrophysics
Abstract

We present the results of searches for point-like sources of neutrinos based on the first combined analysis of data from both the ANTARES and IceCube neutrino telescopes. The combination of both detectors, which differ in size and location, forms a window in the southern sky where the sensitivity to point sources improves by up to a factor of 2 compared with individual analyses. Using data recorded by ANTARES from 2007 to 2012, and by IceCube from 2008 to 2011, we search for sources of neutrino emission both across the southern sky and from a preselected list of candidate objects. No significant excess over background has been found in these searches, and flux upper limits for the candidate sources are presented for E -2.5 and E -2 power-law spectra with different energy cut-offs.

Published
2016

19. THE FIRST COMBINED SEARCH for NEUTRINO POINT-SOURCES in the SOUTHERN HEMISPHERE with the ANTARES and ICECUBE NEUTRINO TELESCOPES

Author

Adrián-Martínez, S, Albert, A, André, M, Anton, G, Ardid, M, Aubert, JJ, Baret, B, Barrios-Martí, J, Basa, S, Bertin, V, Biagi, S, Bormuth, R, Bouwhuis, MC, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Chiarusi, T, Circella, M, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Dekeyser, I, Deschamps, A, De Bonis, G, Distefano, C, Donzaud, C, Dornic, D, Drouhin, D, Dumas, A, Eberl, T, Elsässer, D, Enzenhöfer, A, Fehn, K, Felis, I, Fermani, P, Folger, F, Fusco, LA, Galatà, S, Gay, P, Geißelsöder, S, Geyer, K, Giordano, V, Gleixner, A, Gracia-Ruiz, R, Graf, K, Hallmann, S, Van Haren, H, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hößl, J, Hofestädt, J, Hugon, C, James, CW, Jong, MD, Kadler, M, Kalekin, O, Katz, U, Kießling, D, Kooijman, P, Kouchner, A, Kreter, M, Kreykenbohm, I, Kulikovskiy, V, Lahmann, R, Lefèvre, D, Leonora, E, Loucatos, S, Marcelin, M, Margiotta, A, Marinelli, A, Martínez-Mora, JA, Mathieu, A, Michael, T, Migliozzi, P, Moussa, A, Mueller, C, Nezri, E, PǍvǍlaş, GE, Pellegrino, C, Perrina, C, Piattelli, P, Popa, V, Pradier, T, Racca, C, Riccobene, G, Richter, R, Roensch, K, Saldaña, M, Samtleben, DFE, Sánchez-Losa, A, Sanguineti, M, Sapienza, P, Schmid, J, Schnabel, J, and Schüssler, F

Subjects
astroparticle physics, neutrinos, hep-ex, astro-ph.HE, Astronomy & Astrophysics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural)
Abstract

We present the results of searches for point-like sources of neutrinos based on the first combined analysis of data from both the ANTARES and IceCube neutrino telescopes. The combination of both detectors, which differ in size and location, forms a window in the southern sky where the sensitivity to point sources improves by up to a factor of 2 compared with individual analyses. Using data recorded by ANTARES from 2007 to 2012, and by IceCube from 2008 to 2011, we search for sources of neutrino emission both across the southern sky and from a preselected list of candidate objects. No significant excess over background has been found in these searches, and flux upper limits for the candidate sources are presented for E -2.5 and E -2 power-law spectra with different energy cut-offs.

Published
2016

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