  A small fraction of subluminous B stars show short-period, multiperiodic
light variations and form the new class of pulsating star known as EC 14026
variables, after the prototype. The Multi-Site Spectroscopic Telescope (MSST)
is a virtual instrument and is also the name of a collaboration that aims to
open up a new observational window to provide access to a mode identification
for and an asteroseismological analysis of the pulsating sdB star PG 1605+072.
Although the primary aim is to obtain time resolved spectroscopy it also
includes the most extended photometric monitoring campaign for PG 1605+072.
