Searches for Point-Like and Extended Neutrino Sources Close to the Galactic Center Using the Antares Neutrino Telescope

Adrián-Martínez, S.; Albert, A.; André, M.; Anghinolfi, M.; Anton, G.; Ardid, M.; Aubert, J.J.; Baret, B.; Barrios-Martí, J.; Basa, S.; Bertín, V.; Biagi, S.; Bogazzi, C.; Bormuth, R.; Bou-Cabo, M.; Bouwhuis, M. C.; Bruijn, R.; Brünner, J.; Busto, J.; Capone, A.; Caramete, L.; Cârloganu, C.; Carr, J.; Chiarusi, T.; Circella, M.; Core, L.; Costantini, H.; Coyle, P.; Creusot, A.; Curtil, C.; Rosa, G. De; Dekeyser, I.; Deschamps, A.; Bonis, G. De; Distefano, C.; Donzaud, C.; Dornic, D.; Dorosti, Q.; Drouhin, D.; Dumas, A.; Eberl, T.; Elsässer, Dominik; Enzenhöfer, A.; Escoffier, S.; Fehn, K.; Felis, I.; Fermani, P.; Folger, F.; Fusco, L.; Galatà, S.; Gay, P.; Geißelsöder, S.; Geyer, K.; Giordano, V.; Gleixner, A.; Gómez-González, J.; Graf, Κ.; Guillard, G.; Haren, Hans van; Heijboer, A.; Hello, Y.; Hernández-Rey, J. J.; Herold, B.; Herrero, Alicia; Hößl, J.; Hofestädt, J.; James, C. W.; Jong, M. de; Kadler, M.; Kalekin, O.; Katz, U.; Kießling, D.; Kooijman, P.; Kouchner, A.; Kreykenbohm, I.; Kulikovskiy, V.; Lahmann, R.; Lambard, E.; Lambard, G.; Lattuada, D.; Lefèvre, D.; Leonora, E.; Loehner, H.; Loucatos, S.; Mangano, S.; Marcelin, M.; Margiotta, A.; Martínez-Mora, J. A.; Martini, Séverine; Mathieu, A.; Michael, T.; Migliozzi, P.; Mueller, C. L.; Neff, M.; Nezri, E.; Palioselitis, D.; Păvălaş, G. E.; Perrina, C.; Piattelli, P.; Popa, V.; Pradier, T.; Racca, C.; Riccobene, G.; Richter, R.; Roensch, K.; Rostovtsev, A.; Saldaña, M.; Samtleben, D. F. E.; Sánchez-Losa, A.; Sanguineti, M.; Sapienza, P.; Schmid, Julia; Schnabel, J.; Schulte, S.; Schüßler, F.; Seitz, T.; Sieger, C.; Spies, A.; Spurio, M.; Steijger, J. J. M.; Stolarczyk, Th.; Taiuti, M.; Tamburini, Christian; Tayalati, Y.; Trovato, A.; Vallage, B.; Vallée, C.; Elewyck, V. Van; Visser, E.; Vivolo, D.; Wagner, S. J.; Wilms, J.; Wolf, E. de; Yatkin, K.; Yepes, H.; Zornoza, J.D.; Zúñiga, J.

doi:10.1088/2041-8205/786/1/l5

Cited by 115 publications

(100 citation statements)

References 16 publications

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“…These uncertainties are dominant over the uncertainties related to the detector response. The effects on the muon and neutrino rates due to the detector uncertainties are widely discussed elsewhere, particularly in [34,[37][38][39]. For the atmospheric neutrinos, the systematic uncertainties as a function of the energy are detailed in [38].…”

Section: Resultsmentioning

confidence: 99%

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Search for relativistic magnetic monopoles with five years of the ANTARES detector data

Albert

André

Anghinolfi

et al. 2017

J. High Energ. Phys.

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A search for magnetic monopoles using five years of data recorded with the ANTARES neutrino telescope from January 2008 to December 2012 with a total live time of 1121 days is presented. The analysis is carried out in the range β > 0.6 of magnetic monopole velocities using a strategy based on run-by-run Monte Carlo simulations. No signal above the background expectation from atmospheric muons and atmospheric neutrinos is observed, and upper limits are set on the magnetic monopole flux ranging from 5.7 × 10 −16 to 1.5 × 10 −18 cm −2 · s −1 · sr −1 .

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Section: Resultsmentioning

confidence: 99%

“…Some basic quality cuts have been applied to the data to ensure good data taking conditions [34]. To avoid any experimental bias, the search strategy is based on a blind analysis.…”

Section: Trigger and Reconstructionmentioning

confidence: 99%

Search for relativistic magnetic monopoles with five years of the ANTARES detector data

Albert

André

Anghinolfi

et al. 2017

J. High Energ. Phys.

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“…Therefore, the effective areas provided by ANTARES for a given decl. band are the day-averaged values (Adrian-Martinez et al 2014). A joint stacking analysis between IceCube and ANTARES (Adrian-Martinez et al 2016a, 2016b) could maximize the sensitivity of neutrino searches from FRBs across the full sky.…”

Section: Discussionmentioning

confidence: 99%

A Search for Neutrino Emission from Fast Radio Bursts with Six Years of IceCube Data

Aartsen

Ackermann²,

Adams

et al. 2018

ApJ

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We present a search for coincidence between IceCube TeV neutrinos and fast radio bursts (FRBs). During the search period from 2010 May 31 to 2016 May 12, a total of 29 FRBs with 13 unique locations have been detected in the whole sky. An unbinned maximum likelihood method was used to search for spatial and temporal coincidence between neutrinos and FRBs in expanding time windows, in both the northern and southern hemispheres. No significant correlation was found in six years of IceCube data. Therefore, we set upper limits on neutrino fluence emitted by FRBs as a function of time window duration. We set the most stringent limit obtained to date on neutrino fluence from FRBs with an E −2 energy spectrum assumed, which is 0.0021 GeV cm −2 per burst for emission timescales up to ∼10 2 s from the northern hemisphere stacking search.

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“…E rec μ is the reconstructed muon energy. σ rec μ is the (50% for IceCube, 1σ for ANTARES) angular uncertainty of the reconstructed track direction [37,38] (bottom), and the reconstructed directions for high-energy neutrino candidates detected by IceCube (green crosses) and ANTARES (blue cross) within AE500 s around the GW signals. The maps are in equatorial coordinates.…”

Section: Discussionmentioning

confidence: 99%

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

Albert¹,

André²,

Anghinolfi³

et al. 2017

Phys. Rev. D

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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 AE500 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 × 10 51 -2 × 10 54 erg.

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Searches for Point-Like and Extended Neutrino Sources Close to the Galactic Center Using the Antares Neutrino Telescope

Cited by 115 publications

References 16 publications

Search for relativistic magnetic monopoles with five years of the ANTARES detector data

Search for relativistic magnetic monopoles with five years of the ANTARES detector data

A Search for Neutrino Emission from Fast Radio Bursts with Six Years of IceCube Data

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

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