Very Small Array. Flux density at 33GHz (Cleary+, 2005)
We describe the source subtraction strategy and observations for the extended Very Small Array (VSA), a cosmic microwave background interferometer operating at 33GHz. A total of 453 sources were monitored at 33GHz using a dedicated source subtraction baseline. 131 sources brighter than 20mJy were directly subtracted from the VSA visibility data
Cleary, K. A. et al.
Fecha de publicación:
11
2009