========================================================================== J/MNRAS/341/1066 Very Small Array. II. CMB at 34GHz (Taylor+, 2003) The following files can be converted to FITS (extension .fit .fgz or .fiZ) table1.dat table3.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/MNRAS/341/1066 ==========================================================================
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Beginning of ReadMe : J/MNRAS/341/1066 Very Small Array. II. CMB at 34GHz (Taylor+, 2003) ================================================================================ First results from the Very Small Array - II. Observations of the cosmic microwave background. 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. <Mon. Not. R. Astron. Soc., 341, 1066-1075 (2003)> =2003MNRAS.341.1066T ================================================================================ ADC_Keywords: Radio sources Keywords: cosmic microwave background - cosmology: observations Abstract: 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 3.6deg-0.4deg (equivalent to angular multipoles l=150-900).
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