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000408363 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2013-04/gustafsson_michael
000408363 0247_ $$2ISSN$$a1435-8077
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000408363 1001_ $$0P:(DE-HGF)0$$aGustafsson, M.$$b0$$eCorresponding author
000408363 1112_ $$0C13-06-24.5$$2inspire$$a9th Patras Workshop on Axions, WIMPs and WISPs$$cMainz$$d2013-06-24 - 2013-06-28$$gAXION-WIMP 2013$$wGermany
000408363 245__ $$aFermi-LAT and the Gamma-Ray Line Search
000408363 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2013
000408363 29510 $$aGustafsson, M. "Fermi-LAT and the Gamma-Ray Line Search" in Proceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013) / Oberlack, Uwe, Sissol, Pierre (eds.), 2013 ; AXION-WIMP 2013 : 9th Patras Workshop on Axions, WIMPs and WISPs , 2013-06-23 - 2013-06-28, Mainz
000408363 300__ $$a215-222
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000408363 520__ $$aA distinct signature for dark matter in the form of weakly interacting massive particles (WIMPs) would be the detection of a monochromatic spectral line in the gamma-ray sky. The Fermi-LAT collaboration has searched for such a line in the energy range from 5 to 300 GeV in five sky regions around the Galactic centre. No globally significant line is detected, and 95% CL upper limits on monochromatic-line strengths are presented. The smallest search region reveals a line-like structure at 133 GeV with a local significance of 2.9 σ after 4.4 years of data, which translates to less than 1σ global significance from a trial factor of around 200.
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000408363 7001_ $$0P:(DE-HGF)0$$aFermi LAT Collaboration$$b1$$eCollaboration author
000408363 7870_ $$0PUBDB-2015-05816$$aOberlack, Uwe et. al.$$iisPartOf$$rDESY-PROC-2013-04$$tProceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013)
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