Limits to cosmic background radiation fluctuations at 8.44 GHz between angular scales 10″ and 200″

We have used the VLA at 8.44 GHz to measure fluctuations in the cosmic background radiation (CBR) from two deep images, each 7′ x 7′ in size. No fluctuations between the angular scales 10″ and 200″ were detected. The most accurate limit (95% confidence) is ΔT/T_CBR < 1.9 x 10^-5 for 80″ resolution. For random Gaussian fluctuations with coherence angle θ_c, the limits are ΔT/T_CBR < 30 x 10^-5 for 22″ < θ_c < 60″. Outside this range the limits increase to ΔT/T_CBR < 5 x 10^-5 at θ_c = 12″ or 100″ and ΔT/T_CBR < 10 x 10^-5 at θ_c = 5″ or 120″. Similar limits have been obtained for the circularly and linearly polarized components of the CBR fluctuations. These limits were derived from the residual fluctuations in the images after (1) removing brighter foreground sources (> 14.5 μJy) which covered about 10% of each image; (2) estimating fluctuations of weaker sources by extrapolating the count of dN/dS = 4.6S^-2.3 Jy^-1 sr^-1 to 4 μJy; and (3) determining fluctuations from receiver noise and instrumental errors by comparing the image variances from two independent halves of the data set. All analysis was made on dirty images, in which the statistical properties of instrumental and sky fluctuations are well-defined.