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  <organization>ICN-UNAM</organization>
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  <userid>3</userid>
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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>
<participants></participants>
<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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  <name first="José" middle="" last="Valdés"></name>
  <organization>IGeof-UNAM</organization>
  <emailHash>40af9343b8bb9d18708b4f0252d5f53c</emailHash>
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 <board>030 (2A)</board>
 <track>HE.1.4.A</track>
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  <name>Poster</name>
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 <title>New method for atmospheric calibration at the Pierre Auger Observatory using FRAM, a robotic astronomical telescope</title>
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   <title>Dr.</title>
   <name first="Petr" middle="" last="Travnicek,"></name>
   <organization>FZU, Academy of Sciences of the Czech Republic</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
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   <title></title>
   <name first="-" middle="" last="The Pierre Auger Collaboration"></name>
   <organization>The Pierre Auger Observatory</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
  </user>
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   <title>Dr.</title>
   <name first="Petr" middle="" last="Travnicek,"></name>
   <organization>FZU, Academy of Sciences of the Czech Republic</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
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  <name>Merida, Mexico</name>
  <address></address>
  <room>Regency (Hyatt)</room>
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 <startDate>2007-07-04T14:45:00</startDate>
 <endDate>2007-07-04T14:45:00</endDate>
 <abstract>FRAM - F/(Ph)otometric Robotic Atmospheric Monitor is the latest addition
to the atmospheric monitoring instruments of the Pierre Auger Observatory.
An optical telescope equipped with CCD camera and photometer, it
automatically observes a set of selected standard stars and a calibrated
terrestrial source. Primarily, the wavelength dependence of the
attenuation is derived and the comparison between its vertical values (for
stars) and horizontal values (for the terrestrial source) is made.
Further, the integral vertical aerosol optical depth can be obtained. A
secondary program of the instrument, the detection of optical counterparts
of gamma-ray bursts, has already proven successful. The hardware setup,
software system, data taking procedures, and first analysis results are
described in this paper.</abstract>
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