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2022-02-11Zeitschriftenartikel DOI: 10.18452/26322
Search for High-energy Neutrinos from Ultraluminous Infrared Galaxies with IceCube
dc.contributor.authorAbbasi, R.
dc.contributor.authorAckermann, M.
dc.contributor.authorAdams, J.
dc.contributor.authorAguilar, J. A.
dc.contributor.authorAhlers, M.
dc.contributor.authorAhrens, M.
dc.contributor.authorAlispach, C.
dc.contributor.authorAlves, A. A.
dc.contributor.authorAmin, N. M.
dc.contributor.authorAn, R.
dc.contributor.authorAndeen, K.
dc.contributor.authorAnderson, T.
dc.contributor.authorAnton, G.
dc.contributor.authorArgüelles, C.
dc.contributor.authorAshida, Y.
dc.contributor.authorAxani, S.
dc.contributor.authorBai, X.
dc.contributor.authorV., A. Balagopal
dc.contributor.authorBarbano, A.
dc.contributor.authorBarwick, S. W.
dc.contributor.authorBastian, B.
dc.contributor.authorBasu, V.
dc.contributor.authorBaur, S.
dc.contributor.authorBay, R.
dc.contributor.authorBeatty, J. J.
dc.contributor.authorBecker, K.-H.
dc.contributor.authorTjus, J. Becker
dc.contributor.authorBellenghi, C.
dc.contributor.authorBenZvi, S.
dc.contributor.authorBerley, D.
dc.contributor.authorBernardini, E.
dc.contributor.authorBesson, D. Z.
dc.contributor.authorBinder, G.
dc.contributor.authorBindig, D.
dc.contributor.authorBlaufuss, E.
dc.contributor.authorBlot, S.
dc.contributor.authorBoddenberg, M.
dc.contributor.authorBontempo, F.
dc.contributor.authorBorowka, J.
dc.contributor.authorBöser, S.
dc.contributor.authorBotner, O.
dc.contributor.authorBöttcher, J.
dc.contributor.authorBourbeau, E.
dc.contributor.authorBradascio, F.
dc.contributor.authorBraun, J.
dc.contributor.authorBron, S.
dc.contributor.authorBrostean-Kaiser, J.
dc.contributor.authorBrowne, S.
dc.contributor.authorBurgman, A.
dc.contributor.authorBurley, R. T.
dc.contributor.authorBusse, R. S.
dc.contributor.authorCampana, M. A.
dc.contributor.authorCarnie-Bronca, E. G.
dc.contributor.authorChen, C.
dc.contributor.authorChirkin, D.
dc.contributor.authorChoi, K.
dc.contributor.authorClark, B. A.
dc.contributor.authorClark, K.
dc.contributor.authorClassen, L.
dc.contributor.authorColeman, A.
dc.contributor.authorCollin, G. H.
dc.contributor.authorConrad, J. M.
dc.contributor.authorCoppin, P.
dc.contributor.authorCorrea, P.
dc.contributor.authorCowen, D. F.
dc.contributor.authorCross, R.
dc.contributor.authorDappen, C.
dc.contributor.authorDave, P.
dc.contributor.authorDe Clercq, C.
dc.contributor.authorDeLaunay, J. J.
dc.contributor.authorDembinski, H.
dc.contributor.authorDeoskar, K.
dc.contributor.authorDe Ridder, S.
dc.contributor.authorDesai, A.
dc.contributor.authorDesiati, P.
dc.contributor.authorde Vries, K. D.
dc.contributor.authorde Wasseige, G.
dc.contributor.authorde With, M.
dc.contributor.authorDeYoung, T.
dc.contributor.authorDharani, S.
dc.contributor.authorDiaz, A.
dc.contributor.authorDíaz-Vélez, J. C.
dc.contributor.authorDittmer, M.
dc.contributor.authorDujmovic, H.
dc.contributor.authorDunkman, M.
dc.contributor.authorDuVernois, M. A.
dc.contributor.authorDvorak, E.
dc.contributor.authorEhrhardt, T.
dc.contributor.authorEller, P.
dc.contributor.authorEngel, R.
dc.contributor.authorErpenbeck, H.
dc.contributor.authorEvans, J.
dc.contributor.authorEvenson, P. A.
dc.contributor.authorFan, K. L.
dc.contributor.authorFazely, A. R.
dc.contributor.authorFiedlschuster, S.
dc.contributor.authorFienberg, A. T.
dc.contributor.authorFilimonov, K.
dc.contributor.authorFinley, C.
dc.contributor.authorFischer, L.
dc.date.accessioned2023-03-28T09:07:00Z
dc.date.available2023-03-28T09:07:00Z
dc.date.issued2022-02-11none
dc.date.updated2022-02-15T23:13:13Z
dc.identifier.issn0004-637X
dc.identifier.urihttp://edoc.hu-berlin.de/18452/27002
dc.description.abstractUltraluminous infrared galaxies (ULIRGs) have infrared luminosities LIR ≥ 1012L⊙, making them the most luminous objects in the infrared sky. These dusty objects are generally powered by starbursts with star formation rates that exceed 100 M⊙ yr−1, possibly combined with a contribution from an active galactic nucleus. Such environments make ULIRGs plausible sources of astrophysical high-energy neutrinos, which can be observed by the IceCube Neutrino Observatory at the South Pole. We present a stacking search for high-energy neutrinos from a representative sample of 75 ULIRGs with redshift z ≤ 0.13 using 7.5 yr of IceCube data. The results are consistent with a background-only observation, yielding upper limits on the neutrino flux from these 75 ULIRGs. For an unbroken E−2.5 power-law spectrum, we report an upper limit on the stacked flux ${{\rm{\Phi }}}_{{\nu }_{\mu }+{\bar{\nu }}_{\mu }}^{90 \% }=3.24\times {10}^{-14}\,{\mathrm{TeV}}^{-1}\,{\mathrm{cm}}^{-2}\,{{\rm{s}}}^{-1}\,{(E/10\,\mathrm{TeV})}^{-2.5}$ at 90% confidence level. In addition, we constrain the contribution of the ULIRG source population to the observed diffuse astrophysical neutrino flux as well as model predictions.eng
dc.language.isoengnone
dc.publisherHumboldt-Universität zu Berlin
dc.rights(CC BY 4.0) Attribution 4.0 Internationalger
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.subject.ddc520 Astronomie und zugeordnete Wissenschaftennone
dc.subject.ddc530 Physiknone
dc.titleSearch for High-energy Neutrinos from Ultraluminous Infrared Galaxies with IceCubenone
dc.typearticle
dc.identifier.urnurn:nbn:de:kobv:11-110-18452/27002-0
dc.identifier.doihttp://dx.doi.org/10.18452/26322
dc.type.versionpublishedVersionnone
local.edoc.pages15none
local.edoc.type-nameZeitschriftenartikel
local.edoc.container-typeperiodical
local.edoc.container-type-nameZeitschrift
dc.description.versionPeer Reviewednone
dc.identifier.eissn1538-4357
dcterms.bibliographicCitation.doi10.3847/1538-4357/ac3cb6none
dcterms.bibliographicCitation.journaltitleThe astrophysical journalnone
dcterms.bibliographicCitation.volume926none
dcterms.bibliographicCitation.issue1none
dcterms.bibliographicCitation.articlenumber59none
dcterms.bibliographicCitation.originalpublishernameInstitute of Physics Publ.none
dcterms.bibliographicCitation.originalpublisherplaceLondonnone
bua.departmentMathematisch-Naturwissenschaftliche Fakultätnone

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