  The lack of detected intermediate mass black holes poses a gap in our
understanding of the growth and evolution of the most exotic of astrophysical
objects. Here we investigate the possibility of low-luminosity relativistic
jets launched by intermediate mass black holes in the centers of dwarf
galaxies. We built population models that allow us to make predictions for
their radio emission and quantify their detectability by current and future
surveys. We find that the upcoming instruments in optical and radio like the
SKA, ngVLA and the Vera C. Rubin Observatory will likely be able to detect a
significant fraction ($>38\%$) of such sources population if they exist. In
addition, our results suggest that it is not unlikely a small number of
midiquasars possibly masquerading as low-luminosity active galactic nuclei may
have already been detected by existing surveys.
