Very Small Array. II. CMB at 34GHz (Taylor+, 2003)

Bibcode
2005yCat..73411066T
Taylor, A. C.; Carreira, P.; Cleary, K.; Davies, R. D.; Davis, R. J.; Dickinson, C.; Grainge, K.; Gutierrez, C. M.; Hobson, M. P.; Jones, M. E.; Kneissl, R.; Lasenby, A.; Leahy, J. P.; Maisinger, K.; Pooley, G. G.; Rebolo, R.; Rubino-Martin, J. A.; Rusholme, B.; Saunders, R. D. E.; Savage, R.; Scott, P. F.; Slosar, A.; Sosa Molina, P. J.; Titterington, D.; Waldram, E.; Watson, R. A.; Wilkinson, A.
Bibliographical reference

VizieR On-line Data Catalog: J/MNRAS/341/1066. Originally published in: 2003MNRAS.341.1066T

Advertised on:
2
2005
Number of authors
27
IAC number of authors
0
Citations
0
Refereed citations
0
Description
We have observed the cosmic microwave background (CMB) temperature fluctuations in eight fields covering three separated areas of sky with the Very Small Array at 34GHz. A total area of 101 square degrees has been imaged, with sensitivity on angular scales of 3.6{deg}-0.4{deg} (equivalent to angular multipoles l=150-900). (2 data files).
Type
Non-refereed
Radio sources

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