  Fast Radio Bursts (FRBs) are bright, extragalactic radio pulses whose origins
are still unknown. Until recently, most FRBs have been detected at frequencies
greater than 1 GHz with a few exceptions at 800 MHz. The recent discoveries of
FRBs at 400 MHz from the Canadian Hydrogen Intensity Mapping Experiment (CHIME)
telescope has opened up possibilities for new insights about the progenitors
while many other low frequency surveys in the past have failed to find any
FRBs. Here, we present results from a FRB survey recently conducted at the
Jodrell Bank Observatory at 332 MHz with the 76-m Lovell telescope for a total
of 58 days. We did not detect any FRBs in the survey and report a 90$\%$ upper
limit of 5500 FRBs per day per sky for a Euclidean Universe above a fluence
threshold of 46 Jy ms. We discuss the possibility of absorption as the main
cause of non-detections in low frequency (< 800 MHz) searches and invoke
different absorption models to explain the same. We find that Induced Compton
Scattering alone cannot account for absorption of radio emission and that our
simulations favour a combination of Induced Compton Scattering and Free-Free
Absorption to explain the non-detections. For a free-free absorption scenario,
our constraints on the electron density are consistent with those expected in
the post-shock region of the ionized ejecta in Super-Luminous SuperNovae
(SLSNe).

High Energy Astrophysical Phenomena