Sources in VSA fields at 30GHz (Gawronski+, 2010)

Bibcode
2011yCat..74061853G
Gawronski, M. P.; Peel, M. W.; Lancaster, K.; Battye, R. A.; Birkinshaw, M.; Browne, I. W. A.; Davies, M. L.; Davis, R. J.; Feiler, R.; Franzen, T. M. O.; Genova-Santos, R.; Kus, A. J.; Lowe, S. R.; Pazderska, B. M.; Pazderski, E.; Pooley, G. G.; Roukema, B. F.; Waldram, E. M.; Wilkinson, P. N.
Referencia bibliográfica

VizieR On-line Data Catalog: J/MNRAS/406/1853. Originally published in: 2010MNRAS.406.1853G

Fecha de publicación:
2
2011
Número de autores
19
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
The VSA (Very Small Array) has made CMB observations in three different configurations, corresponding to different multipole order (l) ranges: compact for l=150-800 (Taylor et al. 2003, Cat. J/MNRAS/341/1066), extended for l=300-1500 (Dickinson et al. 2004MNRAS.353..732D) and super-extended for l=600-2500. The corresponding areas have been surveyed with the Ryle Telescope (RT) at 15GHz, to a greater depth the higher the l value, in order to identify the sources for subtraction at 33GHz. The five fields analyzed in this paper are those of the VSA super-extended observations. (2 data files).
Tipo
Sin árbitro
Fuentes de radio

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