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dc.contributor.authorAdrian-Martinez, S.
dc.contributor.authorAlbert, A.
dc.contributor.authorAndre, M.
dc.contributor.authorAnton, G.
dc.contributor.authorArdid, M.
dc.contributor.authorAubert, J. J.
dc.contributor.authorBaret, B.
dc.contributor.authorBarrios-Marti, J.
dc.contributor.authorBasa, S.
dc.contributor.authorBertin, V.
dc.contributor.authorBesson, David Zeke
dc.date.accessioned2017-10-30T17:01:28Z
dc.date.available2017-10-30T17:01:28Z
dc.date.issued2016-05-23
dc.identifier.citationAdrián-Martínez, S., Albert, A., André, M., Anton, G., Ardid, M., Aubert, J., . . . Zoll, M. (2016). The First Combined Search For Neutrino Point-Sources In The Southern Hemisphere With The Antares And Icecube Neutrino Telescopes. The Astrophysical Journal, 823(1), 65. doi:10.3847/0004-637x/823/1/65en_US
dc.identifier.urihttp://hdl.handle.net/1808/25216
dc.description.abstractWe 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.en_US
dc.publisherAmerican Astronomical Societyen_US
dc.rights© 2016. The American Astronomical Society. All rights reserved.en_US
dc.subjectAstroparticle physicsen_US
dc.subjectNeutrinosen_US
dc.titleThe First Combined Search For Neutrino Point-Sources in The Southern Hemisphere With The Antares And Icecube Neutrino Telescopesen_US
dc.typeArticleen_US
kusw.kuauthorBesson, David Zeke
kusw.kudepartmentPhysics and Astronomyen_US
dc.identifier.doi10.3847/0004-637X/823/1/65en_US
kusw.oaversionScholarly/refereed, publisher versionen_US
kusw.oapolicyThis item meets KU Open Access policy criteria.en_US
dc.rights.accessrightsopenAccess


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