First results from the Very Small Array — I. Observational methods

The Very Small Array (VSA) is a synthesis telescope designed to image faint structures in the cosmic microwave background on degree and sub-degree angular scales. The VSA has key differences from other CMB interferometers with the result that different systematic errors are expected. We have tested...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2003-06, Vol.341 (4), p.1057-1165
Hauptverfasser:	Watson, Robert A., Carreira, Pedro, Cleary, Kieran, Davies, Rod D., Davis, Richard J., Dickinson, Clive, Grainge, Keith, Gutiérrez, Carlos M., Hobson, Michael P., Jones, Michael E., Kneissl, Rüdiger, Lasenby, Anthony, Maisinger, Klaus, Pooley, Guy G., Rebolo, Rafael, Rubiño-Martin, José Alberto, Rusholme, Ben, Saunders, Richard D. E., Savage, Richard, Scott, Paul F., Slosar, Anže, Sosa Molina, Pedro J., Taylor, Angela C., Titterington, David, Waldram, Elizabeth, Wilkinson, Althea
Format:	Artikel
Sprache:	eng
Schlagworte:	cosmic microwave background cosmology: observations instrumentation: interferometers
Online-Zugang:	Volltext
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