6533b832fe1ef96bd129a478
RESEARCH PRODUCT
Search for muon neutrinos from gamma-ray bursts with the ANTARES neutrino telescope using 2008 to 2011 data
Stephanie EscoffierJ-j. AubertGiorgio RiccobeneJ.d. ZornozaE. A. De WolfE. A. De WolfS. LoucatosB. VallageUli KatzB. HeroldT. PradierTommaso ChiarusiJutta SchnabelM. MorgantiS. BiagiM. CircellaA. GleixnerA. TrovatoCornelia MüllerCiro BigongiariJ. P. Gómez-gonzálezA. RobertA. RobertD. DornicJose BustoJ.-p. ErnenweinM. TaiutiA. CreusotP.m. KooijmanP.m. KooijmanP.m. KooijmanJ. SchmidM. AnghinolfiF. SimeoneL. CarameteC. CârloganuJ. ZúñigaG. De BonisGiuseppina LarosaS. GeißelsöderA. KouchnerOleg KalekinAnnarita MargiottaV. Van ElewyckQ. DorostiS. AnvarTri L. AstraatmadjaA. Sánchez-losaPaolo PiattelliP. BaerwaldT. SeitzRainer RichterDominique LefèvreDominique LefèvreTeresa MontaruliK. GeyerA. J. HeijboerL. CoreF. FolgerC. CurtilI. Al SamaraiA. EnzenhöferM. MarcelinV. KulikovskiyK. RoenschTh. StolarczykV. FlaminioS. ManganoRezo ShanidzeK. FehnH. LoehnerP. CoyleE. LambardAlexander KappesC. ValléeD. Lo PrestiZ. CharifGuillaume LambardV. GiordanoH. Van HarenMatthias KadlerH. YepesSéverine MartiniSéverine MartiniV. PopaG.e. PăvălaşB. BouhouS. SchulteIngo KreykenbohmU. EmanueleE. VisserS. GalatàGisela AntonChristian TamburiniChristian TamburiniT. MichaelPh. CharvisGiorgio GiacomelliStefan WagnerA. SpiesJörn WilmsM. NeffP. VerninH. CostantiniB. BaretJ. CarrS. CecchiniThomas EberlR. ConiglioneC. DistefanoD. F. E. SamtlebenD. F. E. SamtlebenJuan José Hernández-reyM. De JongC. RaccaF. ClassenMichel AndréJ. Barrios-martíL. A. FuscoJ. HößlS. BasaC. W. JamesYann HelloA. DumasG. GuillardAnne DeschampsA. RostovtsevArnauld AlbertF. SchüsslerMatteo SanguinetiS. Adrián-martínezC. SiegerP. FermaniMaurizio SpurioIvan DekeyserIvan DekeyserA. CaponeJ.a. Martínez-moraMiguel ArdidU. FritschE. LeonoraC. BogazziE. NezriK. GrafJos SteijgerF. LouisC. PerrinaYahya TayalatiC. DonzaudC. DonzaudR. LahmannC. RivièreD. DrouhinV. BertinD. PalioselitisJürgen BrunnerK. YatkinM.c. Bouwhuissubject
Astrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeMonte Carlo methodgamma-ray burst: generalFOS: Physical sciencesddc:500.201 natural sciencesCoincidenceSpectral lineGamma ray burstsmethods: numericalNuclear physicsneutrinoHigh Energy Physics - Phenomenology (hep-ph)Raigs gamma0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]NeutrinsNeutrinos010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics:Desenvolupament humà i sostenible [Àrees temàtiques de la UPC]Muonnumerical [Methods]010308 nuclear & particles physicsneutrinosAstronomy and Astrophysicsgeneral [Gamma-ray burst]neutrinos - gamma-ray burst: general - methods: numerical; methods: numerical; neutrinos; gamma-ray burst: generalHigh Energy Physics - PhenomenologyGamma-ray burst: general; Methods: numerical; NeutrinosNeutrino detectorSpace and Planetary ScienceFISICA APLICADAFísica nuclearHigh Energy Physics::ExperimentNeutrinoneutrinos - gamma-ray burst: general - methods: numericalGamma-ray burstAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]description
Aims. We search for muon neutrinos in coincidence with GRBs with the ANTARES neutrino detector using data from the end of 2007 to 2011. Methods. Expected neutrino fluxes were calculated for each burst individually. The most recent numerical calculations of the spectra using the NeuCosmA code were employed, which include Monte Carlo simulations of the full underlying photohadronic interaction processes. The discovery probability for a selection of 296 GRBs in the given period was optimised using an extended maximum-likelihood strategy. Results. No significant excess over background is found in the data, and 90% confidence level upper limits are placed on the total expected flux according to the model.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2013-11-01 |