We report here our observations at 35 MHz and 327 MHz made in the direction of the \gamma –Ray pulsar Geminga .
Based on the observed absence of any significant pulsed emission from this source above our detection thresholds at the two frequencies , we obtain useful upper-limits for the average flux to be 75–100 mJy at 35 MHz , and 0.2–0.3 mJy at 327 MHz .
We discuss a few possible reasons for the “ radio-quiet ” nature of this pulsar at frequencies other than around 100 MHz .