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Consider the following diagram representing magnitude of magnification against image distance for a convex lens:
\begin{tabular}{|l|l|l|l|}
\hline \multicolumn{1}{|c|}{ Column-I } & & \multicolumn{1}{|c|}{ Column-II } \\
\hline A. & \( \begin{array}{l}\text { Focal length of the } \\
\text { lens }\end{array} \) & p. & Inverse of slope of line \\
\hline B. & Intercept on x-axis & q. & Unity \\
\hline C. & Intercept on y-axis & r. & Focal length \\
\hline D. & \( \begin{array}{l}\text { Magnitude of slope of } \\
\text { the line(s) }\end{array} \) & s. & \( \begin{array}{l}\text { Inverse of the focal } \\
\text { length }\end{array} \) \\
\hline
\end{tabular}
(1) A-(p); B-(q); C-(r); D-(s)
(2) A-(p); B-(r); C-(q); D-(s)
(3) A-(r); B-(q); C-(p); D-(s)
(4) A-(p); B-(r); C-(q); D-(s)
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