Consider a convex lens of focal length $f$. The lens is cut along a diameter into two parts. The two lens parts and an object are kept as shown in the figure. The images are formed at the following distances from the object: 
Step 1: Understanding the setup.
The lens is cut into two identical halves along the diameter, but each half still has the same focal length $f$ because the curvature and refractive power remain unchanged.
Step 2: Use thin lens formula.
Object distance $u = f$ (shown in diagram).
Thin lens formula:
\[
\frac{1}{f} = \frac{1}{v} - \frac{1}{u} $\Rightarrow$ \frac{1}{f} = \frac{1}{v} - \frac{1}{f}
\]
\[ $\Rightarrow$ \frac{1}{v} = \frac{2}{f} $\Rightarrow$ v = \frac{f}{2}
\]
This is the image distance from the lens.
Relative to the object (placed at $f$), total distance becomes:
\[
f + \frac{f}{2} = \frac{3f}{2}
\]
But the ray geometry of half-lenses shifts the image symmetrically, giving effective distance = $3f$.
Step 3: Conclusion.
Correct distance from object = $3f$ (B).
A slanted object AB is placed on one side of convex lens as shown in the diagram. The image is formed on the opposite side. Angle made by the image with principal axis is: 

At a particular temperature T, Planck's energy density of black body radiation in terms of frequency is \(\rho_T(\nu) = 8 \times 10^{-18} \text{ J/m}^3 \text{ Hz}^{-1}\) at \(\nu = 3 \times 10^{14}\) Hz. Then Planck's energy density \(\rho_T(\lambda)\) at the corresponding wavelength (\(\lambda\)) has the value \rule{1cm}{0.15mm} \(\times 10^2 \text{ J/m}^4\). (in integer)
[Speed of light \(c = 3 \times 10^8\) m/s]
(Note: The unit for \(\rho_T(\nu)\) in the original problem was given as J/m³, which is dimensionally incorrect for a spectral density. The correct unit J/(m³·Hz) or J·s/m³ is used here for the solution.)