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  <name first="Geoffrey Norman" middle="" last="Taylor"></name>
  <organization>University of Melbourne (AU)</organization>
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<supportEmail caption="Support">javd@ph.unimelb.edu.au</supportEmail>
<title>ICHEP2012</title>
<description>36th International Conference on High Energy Physics.</description>
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<startDate>2012-07-04T14:00:00</startDate>
<endDate>2012-07-11T18:20:00</endDate>
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  <name first="Geoffrey" middle="" last="Taylor"></name>
  <organization>University of Melbourne (AU)</organization>
  <email>geoffrey.taylor@cern.ch</email>
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  <title>Prof.</title>
  <name first="Raymond" middle="" last="Volkas"></name>
  <organization>University of Melbourne</organization>
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 <track>Track 11. Particle Astrophysics and Cosmology</track>
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 <title>The status of the cosmic e+/e- anomaly</title>
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   <title>Prof.</title>
   <name first="Csaba" middle="" last="Balazs"></name>
   <organization>Monash University (AU)</organization>
   <email>csaba.balazs@monash.edu</email>
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   <title>Prof.</title>
   <name first="Csaba" middle="" last="Balazs"></name>
   <organization>Monash University (AU)</organization>
   <email>csaba.balazs@monash.edu</email>
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  <address>Melbourne
Australia</address>
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 <startDate>2012-07-07T12:30:00</startDate>
 <endDate>2012-07-07T12:45:00</endDate>
 <duration>00:15</duration>
 <abstract>The anomalous part of the cosmic electron-positron flux can be isolated within a Bayesian likelihood analysis.  From the cosmic ray data the values of relevant cosmic ray propagation parameters can be also be inferred.  I show how a tension arises between various cosmic ray datasets indicating an e+/e- anomaly.  Then I show how to calculate the anomalous part of the PAMELA and Fermi-LAT measurements.  I focus on the uncertainty of this 'signal'.  Finally, I briefly compare this signal to some theoretical results predicting such an anomaly.</abstract>
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