  SALT spectra of the helium-rich hot subdwarf EC22536-5304 show strong
absorption lines of triply-ionized lead. Analysis of the HRS spectrum and a
follow-up SALT/RSS spectrum show EC22536-5304 to have surface properties
(temperature, gravity, helium/hydrogen ratio) similar to other heavy-metal
subdwarfs. With a lead overabundance of 4.8 dex relative to solar, EC22536-5304
is the most lead-rich intermediate helium subdwarf discovered so far.
