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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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<location>
 <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>
  <emailHash>40af9343b8bb9d18708b4f0252d5f53c</emailHash>
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 <track>OG.2.5</track>
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 <title>Neutrino Triggered Target of Opportunity (NToO) test run with AMANDA and MAGIC</title>
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   <name first="Elisa" middle="" last="Bernardini"></name>
   <organization>DESY, Zeuthen</organization>
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   <name first="Markus" middle="" last="Ackermann"></name>
   <organization>DESY, Zeuthen</organization>
   <emailHash>f32a1004fb275cfd11657a21dd17a21f</emailHash>
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   <title></title>
   <name first="Elisa" middle="" last="Bernardini"></name>
   <organization>DESY, Zeuthen</organization>
   <emailHash>09e6594f62189cebe3367513308ab9dd</emailHash>
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   <title></title>
   <name first="Nicola" middle="" last="Galante"></name>
   <organization>Max-Planck Institut für Physik, München</organization>
   <emailHash>d69dd94e1d34406cd503b5ca0bc141a1</emailHash>
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   <name first="Florian" middle="" last="Goebel"></name>
   <organization>Max-Planck Institut für Physik, München</organization>
   <emailHash>8056b736a38cf6672a00a646ea27eca1</emailHash>
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   <title></title>
   <name first="Masaaki" middle="" last="Hayashida"></name>
   <organization>Max-Planck Institut für Physik, München</organization>
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   <title></title>
   <name first="Konstancja" middle="" last="Satalecka"></name>
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   <name first="Martin" middle="" last="Tluczykont"></name>
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   <title></title>
   <name first="Robert" middle="" last="Wagner"></name>
   <organization>Max-Planck Institut für Physik, München</organization>
   <emailHash>a2c0a75b05cce2f034ff982635fe56fb</emailHash>
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  <name>Merida, Mexico</name>
  <address></address>
  <room>Uxmal + Tulum (Holiday Inn)</room>
 </location>
 <startDate>2007-07-10T12:53:00</startDate>
 <endDate>2007-07-10T13:05:00</endDate>
 <duration>00:12</duration>
 <abstract>Fourth generation neutrino telescopes are now being constructed (IceCube) and
designed (KM3NET). While no neutrino flux of cosmic origin has been discovered so
far, the first weak signals are expected to be discerned in the next few years.
Multi-messenger investigations aim at addressing the problem of extracting these
signals from irreducible backgrounds. One possible application is the search for time
correlations of high energy neutrinos and established signals. We show the first
adaptation of a Target of Opportunity strategy to collect simultaneous data of high
energy neutrinos and gamma-rays. A tentative neutrino signal is used to alert
gamma-ray observations. The detection of a positive coincidence can enhance the
neutrino discovery chance. More generally, this scheme of operation can increase the
availability of simultaneous observations. If cosmic neutrino signals can be
established, the combined observations will allow time correlation studies and
therefore constraints on the source modeling. A first technical implementation of
this scheme involving AMANDA and MAGIC has been realized for few pre-selected sources
in a short test run (Sept. to Dec. 2006), with the aim of a feasibility study. The
principles of the NToO test run and its first outcomes will be shown and the
potential for IceCube will be discussed.</abstract>
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