  With its very wide energy band (0.1-100 keV), BeppoSAX has played a
fundamental role in the blazar field, allowing in particular a better study of
the highest synchrotron peaked objects. Here we summarize the results of an
observational program performed with the aim to find and study more extreme BL
Lac sources. We discuss the SEDs of the observed objects and their impact on
the "blazar sequence" scenario, and consider their relevance as possible TeV
emitting sources.
