Please use this identifier to cite or link to this item:
https://hdl.handle.net/2440/101390
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dc.contributor.author | Aartsen, M. | - |
dc.contributor.author | Ackermann, M. | - |
dc.contributor.author | Adams, J. | - |
dc.contributor.author | Aguilar, J. | - |
dc.contributor.author | Ahlers, M. | - |
dc.contributor.author | Ahrens, M. | - |
dc.contributor.author | Altmann, D. | - |
dc.contributor.author | Anderson, T. | - |
dc.contributor.author | Archinger, M. | - |
dc.contributor.author | Arguelles, C. | - |
dc.contributor.author | Arlen, T. | - |
dc.contributor.author | Auffenberg, J. | - |
dc.contributor.author | Bai, X. | - |
dc.contributor.author | Barwick, S. | - |
dc.contributor.author | Baum, V. | - |
dc.contributor.author | Bay, R. | - |
dc.contributor.author | Baker, M. | - |
dc.contributor.author | Beatty, J. | - |
dc.contributor.author | Tjus, J. | - |
dc.contributor.author | Becker, K. | - |
dc.contributor.author | et al. | - |
dc.date.issued | 2015 | - |
dc.identifier.citation | The Astrophysical Journal: an international review of astronomy and astronomical physics, 2015; 807(1):46-1-46-17 | - |
dc.identifier.issn | 0004-637X | - |
dc.identifier.issn | 1538-4357 | - |
dc.identifier.uri | http://hdl.handle.net/2440/101390 | - |
dc.description.abstract | In this paper searches for flaring astrophysical neutrino sources and sources with periodic emission with the IceCube neutrino telescope are presented. In contrast to time-integrated searches, where steady emission is assumed, the analyses presented here look for a time-dependent signal of neutrinos using the information from the neutrino arrival times to enhance the discovery potential. A search was performed for correlations between neutrino arrival times and directions, as well as neutrino emission following time-dependent light curves, sporadic emission, or periodicities of candidate sources. These include active galactic nuclei, soft γ-ray repeaters, supernova remnants hosting pulsars, microquasars, and X-ray binaries. The work presented here updates and extends previously published results to a longer period that covers 4 years of data from 2008 April 5 to 2012 May 16, including the first year of operation of the completed 86 string detector. The analyses did not find any significant time-dependent point sources of neutrinos, and the results were used to set upper limits on the neutrino flux from source candidates. | - |
dc.description.statementofresponsibility | M. G. Aartsen ... G. C. Hill ... S. Robertson ... B. J. Whelan ... et al., IceCube Collaboration | - |
dc.language.iso | en | - |
dc.publisher | IOP Publishing | - |
dc.rights | © 2015. The American Astronomical Society. All rights reserved. | - |
dc.source.uri | http://dx.doi.org/10.1088/0004-637x/807/1/46 | - |
dc.subject | Astroparticle physics – binaries; general – BL Lacertae objects; general – galaxies; active – neutrinos – X-rays; binaries | - |
dc.title | Searches for time-dependent neutrino sources with IceCube data from 2008 to 2012 | - |
dc.type | Journal article | - |
dc.identifier.doi | 10.1088/0004-637X/807/1/46 | - |
dc.relation.grant | ARC | - |
pubs.publication-status | Published | - |
Appears in Collections: | Aurora harvest 3 Chemistry and Physics publications |
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