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Simple telescope used to view distant objects has eyepiece and objective lens of focal lengths \( \mathrm{f}_{\mathrm{e}} \) and \( \mathrm{f}_{0} \), respectively. Then
\begin{tabular}{|l|l|c|l|}
\hline & \multicolumn{1}{|c|}{ Column-I } & & \multicolumn{1}{|c|}{ Column-II } \\
\hline A. & \( \begin{array}{l}\text { Intensity of light } \\
\text { received by lens }\end{array} \) & p. & \( \begin{array}{l}\text { Radius of aperture } \\
\text { (R) }\end{array} \) \\
\hline B. & Angular magnification & q. & Dispersion of lens \\
\hline C. & Length of telescope & r. & Focal length \( \mathrm{f}_{0}, \mathrm{f}_{\mathrm{e}} \) \\
\hline D. & Sharpness of image & s. & Spherical aberration \\
\hline
\end{tabular}
(1) A-(r); B-(q); C-(p); D-(s)
(2) A-(p); B-(q); C-(r); D-(s)
(3) A-(p); B-(r); C-(r); D-(p,q,s)
(4) A-(q); B-(p); C-(s); D-(r)
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