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  <organization>ICN-UNAM</organization>
  <emailHash>1482bc95ee34f0461176da21871284c8</emailHash>
  <userid>3</userid>
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</announcer>
<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>
<location>
 <name>Merida, Mexico</name>
 <address></address>
 <room></room>
</location>
<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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  <title>Dr.</title>
  <name first="José" middle="" last="Valdés"></name>
  <organization>IGeof-UNAM</organization>
  <emailHash>40af9343b8bb9d18708b4f0252d5f53c</emailHash>
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  <name>Oral</name>
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 <title>H.E.S.S. Galactic Plane Survey unveils a Milagro Hotspot</title>
 <speakers>
  <user>
   <title>Dr.</title>
   <name first="Arache" middle="" last="Djannati-Ataï"></name>
   <organization>APC- CNRS/University Paris VII</organization>
   <emailHash>ccb9d87034b0cdd4b4cedbc3828ba251</emailHash>
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   <title>Dr.</title>
   <name first="Arache" middle="" last="Djannati-Ataï"></name>
   <organization>APC- CNRS/University Paris VII</organization>
   <emailHash>ccb9d87034b0cdd4b4cedbc3828ba251</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="Emma" middle="" last="Oña-Wilhelmi"></name>
   <organization>APC CRNS</organization>
   <emailHash>aadf21cd1d052aa5fc1ae344ed84072a</emailHash>
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 <location>
  <name>Merida, Mexico</name>
  <address></address>
  <room>Uxmal + Tulum (Holiday Inn)</room>
 </location>
 <startDate>2007-07-07T11:18:00</startDate>
 <endDate>2007-07-07T11:30:00</endDate>
 <duration>00:12</duration>
 <abstract>The Galactic Plane is accessible to H.E.S.S. at longitudes up to 80
degrees through very low elevation observations.
The ability of H.E.S.S. to observe at elevations as low as 25 degrees
corresponding to an energy threshold of few TeV has been
already validated through observations of the blazar Mkn 421.

We report on H.E.S.S. data on the Galactic Plane up to the 80° longitude range 
and will discuss the possible nature of Milagro hotspots for the cases where 
overlapping data exists.</abstract>
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