WIDEMAP

New directions in radio-interferometric wide-field mapping

 Coordinatore RHEINISCHE FRIEDRICH-WILHELMS-UNIVERSITAT BONN 

 Organization address address: REGINA PACIS WEG 3
city: BONN
postcode: 53113

contact info
Titolo: Prof.
Nome: Peter
Cognome: Schneider
Email: send email
Telefono: -3923
Fax: 49-228-73-4022

 Nazionalità Coordinatore Germany [DE]
 Totale costo 45˙000 €
 EC contributo 45˙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-2007-2-2-ERG
 Funding Scheme MC-ERG
 Anno di inizio 2008
 Periodo (anno-mese-giorno) 2008-04-01   -   2011-03-31

 Partecipanti

# participant  country  role  EC contrib. [€] 
1    RHEINISCHE FRIEDRICH-WILHELMS-UNIVERSITAT BONN

 Organization address address: REGINA PACIS WEG 3
city: BONN
postcode: 53113

contact info
Titolo: Prof.
Nome: Peter
Cognome: Schneider
Email: send email
Telefono: -3923
Fax: 49-228-73-4022

DE (BONN) coordinator 0.00

Mappa


 Word cloud

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radio    astronomical    observations    algorithms    hardware    vlbi    maps    graphics   

 Obiettivo del progetto (Objective)

'The main science driver for our proposal is to develop novel algorithms to produce wide-field maps from radio-interferometric astronomical observations. The technique of Very Long Baseline Interferometry (VLBI) achieves the highest resolution of astronomical observations at any wavelength. Until recently, the size of maps produced by VLBI was limited to tiny regions on the sky. Based on our previous experience in pushing VLBI to larger fields, we will develop methods that allow real wide-field VLBI using affordable computer hardware. In combination with the development of new algorithms, we will use special-purpose hardware that was originally developed for graphics processing. This hardware, available in the form of high-end graphics cards, provides high performance for a low price and is well-suited for our applications. Using this type of hardware is currently also explored in other areas, and we plan to combine the main goal with other fields of astrophysics. Closest to the wide-field mapping project are applications in modelling gravitational lenses and calibrating and imaging data from the new LOFAR radio telescope array. On the more distant side, we will explore the opportunities for numerical N-body simulations, one of the active research areas at the host institute.'

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