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<supportEmail caption="Support">icrc2007@icrc2007.unam.mx</supportEmail>
<title>30th International Cosmic Ray Conference</title>
<description>The 30th International Cosmic Ray Conference will be held from July 3, 2007 to July 11, 2007 in Merida, Yucatan, Mexico.</description>
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<closed>True</closed>
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 <name>Merida, Mexico</name>
 <address></address>
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<startDate>2007-07-03T08:00:00</startDate>
<endDate>2007-07-11T19:00:00</endDate>
<creationDate>2005-09-26T05:04:53</creationDate>
<modificationDate>2024-04-12T17:46:55</modificationDate>
<timezone>Mexico/General</timezone>
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  <name first="José" middle="" last="Valdés"></name>
  <organization>IGeof-UNAM</organization>
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 <title>What is the effect of source parameters in the predictions of Small Scale Anisotropies for UHECR experiments?</title>
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   <name first="Daniel" middle="" last="De Marco"></name>
   <organization>Bartol Research Institute, University of Delaware</organization>
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   <title>Dr.</title>
   <name first="Daniel" middle="" last="De Marco"></name>
   <organization>Bartol Research Institute, University of Delaware</organization>
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   <name first="Paolo" middle="" last="Lipari"></name>
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   <name first="Angela" middle="" last="Olinto"></name>
   <organization>University of Chicago, Enrico Fermi Institute</organization>
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  <name>Merida, Mexico</name>
  <address></address>
  <room>Yucatan II+III+IV (Fiesta Americana)</room>
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 <startDate>2007-07-07T10:42:00</startDate>
 <endDate>2007-07-07T10:54:00</endDate>
 <duration>00:12</duration>
 <abstract>We discuss the small scale anisotropy signal predicted for present and future UHECR
experiments such as Auger, Telescope Array, Auger North and EUSO. We relax the
unrealistic, but commonly used assumption that the sources are all equal and we
concentrate our attention on how the expected signal depends on possible
distributions of the properties of the sources such as a luminosity function or a
varying maximum energy.</abstract>
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