We report our search for and a possible detection of periodic radio pulses at 34.5 MHz from the Fermi-LAT pulsar J1732-3131 .
The candidate detection has been possible in only one of the many sessions of observations made with the low-frequency array at Gauribidanur , India , when the otherwise radio weak pulsar may have apparently brightened many folds .
The candidate dispersion measure along the sight-line , based on the broad periodic profiles from \sim 20 minutes of data , is estimated to be 15.44 \pm 0.32 pc/cc .
We present the details of our periodic & single-pulse search , and discuss the results and their implications relevant to both , the pulsar and the intervening medium .