  Rapid variability in the radio flux density of the BL Lac object PKSB1144-379
has been observed at four frequencies, ranging from 1.5 to 15 GHz, with the VLA
and the University of Tasmania's Ceduna antenna. Intrinsic and line of sight
effects were examined as possible causes of this variability, with interstellar
scintillation best explaining the frequency dependence of the variability
timescales and modulation indices. This scintillation is consistent with a
compact source 20-40 microarcseconds, or 0.15-0.3 pc in size. The inferred
brightness temperature for PKSB1144-379 (assuming that the observed variations
are due to scintillation) is 6.2e12 K at 4.9 GHz, with approximately 10 percent
of the total flux in the scintillating component. We show that scintillation
surveys aimed at identifying variability timescales of days to weeks are an
effective way to identify the AGN with the highest brightness temperatures.
