{"refrec":{"BRefID":365771,"RR":"<b>Albert, A.; Alves, S.; André, M.; Ardid, M.; Ardid, S.; Aubert, J.-J.; Aublin, J.; Baret, B.; Basa, S.; Becherini, Y.; Belhorma, B.; Bendahman, M.; Benfenati, F.; Bertin, V.; Biagi, S.; Bissinger, M.; Boumaaza, J.; Bouta, M.; Bouwhuis, M.C.; Brânzaş, H.; Bruijn, R.; Brunner, J.; Busto, J.; Caiffi, B.; Calvo, D.; Campion, S.; Capone, A.; Caramete, L.; Carenini, F.; Carr, J.; Carretero, V.; Celli, S.; Cerisy, L.; Chabab, M.; Chau, T.N.; Cherkaoui El Moursli, R.; Chiarusi, T.; Circella, M.; Coelho, J.A.B.; Coleiro, A.; Coniglione, R.; Coyle, P.; Creusot, A.; Cruz, A.S.M.; Díaz, A.F.; De Martino, B.; Distefano, C.; Di Palma, I.; Domi, A.; Donzaud, C.; Dornic, D.; Drouhin, D.; Eberl, T.; van Eeden, T.; van Eijk, D.; El Hedri, S.; El Khayati, N.; Enzenhöfer, A.; Fermani, P.; Ferrara, G.; Filippini, F.; Fusco, L.; Gagliardini, S.; García, J.; Gatius Oliver, C.; Gay, P.; Geißelbrecht, N.; Glotin, H.; Gozzini, R.; Gracia Ruiz, R.; Graf, K.; Guidi, C.; Haegel, L.; Hallmann, S.; van Haren, H.; Heijboer, A.J.; Hello, Y.; Hernández-Rey, J.J.; Hößl, J.; Hofestädt, J.; Huang, F.; Illuminati, G.; James, C.W.; Jisse-Jung, B.; de Jong, M.; de Jong, P.; Kadler, M.; Kalekin, O.; Katz, U.; Kouchner, A.; Kreykenbohm, I.; Kulikovskiy, V.; Lahmann, R.; Lamoureux, M.; Lazo, A.; Lefèvre, D.; Leonora, E.; Levi, G.; Le Stum, S.; Lopez-Coto, D.; Loucatos, S.; Maderer, L.; Manczak, J.; Marcelin, M.; Margiotta, A.; Marinelli, A.; Martínez-Mora, J.A.; Migliozzi, P.; Moussa, A.; Muller, R.; Nauta, L.; Navas, S.; Nezri, E.; Ó Fearraigh, B.; Păun, A.; Păvălaş, G.E.; Perrin-Terrin, M.; Pestel, V.; Piattelli, P.; Poirè, C.; Popa, V.; Pradier, T.; Randazzo, N.; Real, D.; Reck, S.; Riccobene, G.; Romanov, A.; Sánchez-Losa, A.; Saina, A.; Salesa Greus, F.; Samtleben, D.F.E.; Sanguineti, M.; Sapienza, P.; Schnabel, J.; Schumann, J.; Schüssler, F.; Seneca, J.; Spurio, M.; Stolarczyk, Th.; Taiuti, M.; Tayalati, Y.; Tingay, S.J.; Vallage, B.; Vannoye, G.; Van Elewyck, V.; Viola, S.; Vivolo, D.; Wilms, J.; Zavatarelli, S.; Zegarelli, A.; Zornoza, J.D.; Zúñiga, J.</b> (2023). Search for neutrino counterparts to the gravitational wave sources from LIGO/Virgo O3 run with the ANTARES detector. <i>Journal of Cosmology and Astroparticle Physics 2023(04)</i>: 004. <a href=\"https://dx.doi.org/10.1088/1475-7516/2023/04/004\" target=\"_blank\">https://dx.doi.org/10.1088/1475-7516/2023/04/004</a>","BEntID":363493,"PublicFlag":1,"CheckedFlag":0,"wosflag":1,"vabbflag":0,"RefStringPartII":". <i>Journal of Cosmology and Astroparticle Physics 2023(04)</i>: 004. <a href=\"https://dx.doi.org/10.1088/1475-7516/2023/04/004\" target=\"_blank\">https://dx.doi.org/10.1088/1475-7516/2023/04/004</a>","DocTypID":8,"DocType":"Journal article","MarineFlag":0,"FreshFlag":0,"BrackishFlag":0,"TerrestrialFlag":0,"Authorstring":"Albert, A.; Alves, S.; André, M.; Ardid, M.; Ardid, S.; Aubert, J.-J.; Aublin, J.; Baret, B.; Basa, S.; Becherini, Y.; Belhorma, B.; Bendahman, M.; Benfenati, F.; Bertin, V.; Biagi, S.; Bissinger, M.; Boumaaza, J.; Bouta, M.; Bouwhuis, M.C.; Brânzaş, H.; Bruijn, R.; Brunner, J.; Busto, J.; Caiffi, B.; Calvo, D.; Campion, S.; Capone, A.; Caramete, L.; Carenini, F.; Carr, J.; Carretero, V.; Celli, S.; Cerisy, L.; Chabab, M.; Chau, T.N.; Cherkaoui El Moursli, R.; Chiarusi, T.; Circella, M.; Coelho, J.A.B.; Coleiro, A.; Coniglione, R.; Coyle, P.; Creusot, A.; Cruz, A.S.M.; Díaz, A.F.; De Martino, B.; Distefano, C.; Di Palma, I.; Domi, A.; Donzaud, C.; Dornic, D.; Drouhin, D.; Eberl, T.; van Eeden, T.; van Eijk, D.; El Hedri, S.; El Khayati, N.; Enzenhöfer, A.; Fermani, P.; Ferrara, G.; Filippini, F.; Fusco, L.; Gagliardini, S.; García, J.; Gatius Oliver, C.; Gay, P.; Geißelbrecht, N.; Glotin, H.; Gozzini, R.; Gracia Ruiz, R.; Graf, K.; Guidi, C.; Haegel, L.; Hallmann, S.; van Haren, H.; Heijboer, A.J.; Hello, Y.; Hernández-Rey, J.J.; Hößl, J.; Hofestädt, J.; Huang, F.; Illuminati, G.; James, C.W.; Jisse-Jung, B.; de Jong, M.; de Jong, P.; Kadler, M.; Kalekin, O.; Katz, U.; Kouchner, A.; Kreykenbohm, I.; Kulikovskiy, V.; Lahmann, R.; Lamoureux, M.; Lazo, A.; Lefèvre, D.; Leonora, E.; Levi, G.; Le Stum, S.; Lopez-Coto, D.; Loucatos, S.; Maderer, L.; Manczak, J.; Marcelin, M.; Margiotta, A.; Marinelli, A.; Martínez-Mora, J.A.; Migliozzi, P.; Moussa, A.; Muller, R.; Nauta, L.; Navas, S.; Nezri, E.; Ó Fearraigh, B.; Păun, A.; Păvălaş, G.E.; Perrin-Terrin, M.; Pestel, V.; Piattelli, P.; Poirè, C.; Popa, V.; Pradier, T.; Randazzo, N.; Real, D.; Reck, S.; Riccobene, G.; Romanov, A.; Sánchez-Losa, A.; Saina, A.; Salesa Greus, F.; Samtleben, D.F.E.; Sanguineti, M.; Sapienza, P.; Schnabel, J.; Schumann, J.; Schüssler, F.; Seneca, J.; Spurio, M.; Stolarczyk, Th.; Taiuti, M.; Tayalati, Y.; Tingay, S.J.; Vallage, B.; Vannoye, G.; Van Elewyck, V.; Viola, S.; Vivolo, D.; Wilms, J.; Zavatarelli, S.; Zegarelli, A.; Zornoza, J.D.; Zúñiga, J.","OrigTitleTranslFlag":0,"Authorstringtrunc":"Albert, A. <i>et al.</i>","Englishabstract":"Since 2015 the LIGO and Virgo interferometers have detected  gravitational    waves from almost one hundred coalescences of compact objects  (black holes    and neutron stars). This article presents the results of a search  performed    with data from the ANTARES telescope to identify neutrino  counterparts to    the gravitational wave sources detected during the third  LIGO/Virgo    observing run and reported in the catalogues GWTC-2, GWTC-2.1, and  GWTC-3.    This search is sensitive to all-sky neutrinos of all flavours and of    energies > 100 GeV, thanks to the inclusion of both track-like events    (mainly induced by <i>ν<sub>μ</sub></i> charged-current interactions)  and    shower-like events (induced by other interaction types). Neutrinos are    selected if they are detected within ± 500 s from the GW merger and with a    reconstructed direction compatible with its sky localisation. No significant    excess is found for any of the 80 analysed GW events, and upper limits on    the  neutrino emission are derived. Using the information from the GW    catalogues and  assuming isotropic emission, upper limits on the total    energy <i>E</i><sub>tot,</sub> <i>ν</i> emitted as neutrinos of all flavours    and on the ratio <i>f<sub>ν</sub></i> = <i>E</i><sub>tot,</sub><i>ν</i>/<i>E</i>    <sub>GW</sub> between  neutrino and GW emissions are also computed. Finally,    a stacked analysis of all  the 72 binary black hole mergers (respectively    the 7 neutron star-black hole  merger candidates) has been performed to    constrain the typical neutrino  emission within this population, leading to    the limits: <i>E</i><sub>tot,</sub> <i>ν</i> <  4.0 <b>×</b> 10    <sup>        53    </sup>    erg and <i>f<sub>ν</sub></i> <  0.15 (respectively, <i>E</i><sub>tot,</sub><i>ν</i> <     3.2 <b>×</b> 10^53  erg and <i>f<sub>ν</sub></i> < 0.88) for <i>E</i>    <sup>-2</sup> spectrum  and isotropic emission. Other assumptions including    softer spectra and  non-isotropic scenarios have also been tested.","AbstractOtherLang":null,"BibLvlCode":"AS","StandardTitle":"Search for neutrino counterparts to the gravitational wave sources from LIGO/Virgo O3 run with the ANTARES detector","OrigTitleLangCode":"en","OrigTitleLangCodeExtended":"eng","OrigTitleLangID":15,"DateLastModified":{"date":"2024-12-10 01:33:17.368041","timezone_type":1,"timezone":"+01:00"},"UserAccessRight":null,"UserAccID":null,"AuthorKeywords":"gravitational waves / sources; neutrino astronomy; neutron stars","OtherDescriptors":null,"Notes":null,"AnaPub":2023,"MonPub":null,"DateUpdate":"2023-07-20","DateCreate":"2023-07-20","SecASFANote":null,"ConfID":null,"PeerRev":1,"VlizCoreFlag":0,"WoScode":"WOS:000989593000009","VABBcode":null,"OpenAcc":1,"DOI":"10.1088/1475-7516/2023/04/004"},"refs":null,"anarec":{"AnaID":365771,"PubliDate":2023,"Pagination":"004","XtraPublOfAnaID":null,"ISBN":null,"Volume":"2023","Issue":"04","BRefMon":null,"BRefMonRR":null,"BRefXtra":null,"BRefXtraRR":null,"SerBRefID":240564,"SerRR":"Journal of Cosmology and Astroparticle Physics. 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