Step 1: Write the radiation energy balance.
Every unit of incident energy on a surface must be reflected, absorbed, or transmitted, so:
\[
\alpha + \rho + \tau = 1
\]
Here we are given the reflected fraction \(\rho = 0.35\) and the transmitted fraction \(\tau = 0.3\).
Step 2: Solve for absorptivity and apply Kirchhoff's law.
\[
\alpha = 1 - \rho - \tau = 1 - 0.35 - 0.3 = 0.35
\]
For a surface in thermal equilibrium with its surroundings, Kirchhoff's law tells us emissivity equals absorptivity, \(\epsilon = \alpha\), so:
\[
\boxed{\epsilon = 0.35}
\]
This matches option 1.