GC4ICE3

Search for high energy neutrino emission from the galactic center

Coordinatore	RHEINISCH-WESTFAELISCHE TECHNISCHE HOCHSCHULE AACHEN    more  Organization address address: Templergraben 55 city: AACHEN postcode: 52062 contact info Titolo: Prof. Nome: Ernst Cognome: Schmachtenberg Email: send email Telefono: -8090682 Fax: -8092682
Nazionalità Coordinatore	Germany [DE]
Totale costo	75˙000 €
EC contributo	75˙000 €
Programma	FP7-PEOPLE Specific programme "People" implementing the Seventh Framework Programme of the European Community for research, technological development and demonstration activities (2007 to 2013)
Code Call	FP7-PEOPLE-2009-RG
Funding Scheme	MC-IRG
Anno di inizio	2009
Periodo (anno-mese-giorno)	2009-11-01   -   2012-10-31

 Partecipanti

#	participant	country	role	EC contrib. [€]
1	RHEINISCH-WESTFAELISCHE TECHNISCHE HOCHSCHULE AACHEN  Organization address address: Templergraben 55 city: AACHEN postcode: 52062 contact info Titolo: Prof. Nome: Ernst Cognome: Schmachtenberg Email: send email Telefono: -8090682 Fax: -8092682	DE (AACHEN)	coordinator	75˙000.00

Mappa

 Word cloud

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 Obiettivo del progetto (Objective)

'Main purpose of the IceCube neutrino telescope is to detect high energy neutrinos of astro- physical origin. Within this project we aim to extend the field of view of the instrument to observe the galactic center, which is not in the generic field of view of a neutrino telescope at the South Pole. This can be accomplished by a new data selection, which detects events of particularily high energy or events of low energy starting inside the detector and by the development of new, more sophisticated reconstruction methods. We propose to reintegrate Dr. David J. Boersma, who has previously been employed by the University of Wisconsin (Madison, USA),into the European astro-particle physics community. The IRG funds will be used for the foundation of a junior research group focused on this topic. Dr. Boersma is a key researcher of the IceCube neutrino telescope and expert on the reconstruction software. He has already succesfully conducted a similar analysis focused on the detection of the shadow of the Moon in underground cosmic rays muons.'