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Fig. 3.5. The count N of radio sources brighter than S (marked I in this figure) in 1955. The dashed line is the relation in equation (3.18) (Ryle 1955). The excess counts between log I = 0.2 and 0.8 were the subject of considerable debate.

Fig. 3.5. The count N of radio sources brighter than S (marked I in this figure) in 1955. The dashed line is the relation in equation (3.18) (Ryle 1955). The excess counts between log I = 0.2 and 0.8 were the subject of considerable debate.

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