  We present updated results of the Baksan Underground Scintillator Telescope
in search for a signal from dark matter particles annihilating in the center of
the Sun. Based on the performance of the Baksan telescope measuring upward
through-going muons with energy larger 1 GeV, we confirm the absence of
observable excess in arrival directions towards the Sun relatively the
expectations from neutrinos of atmospheric origin for 24.12 years of live time.
We conclude that the 90% C.L. upper limits on elastic scattering cross sections
of dark matter WIMP (Weakly Interactive Massive Particle) off proton are
comparable with correspondent limits of other operating neutrino telescopes.
The best value of the limit is $3 \times 10^{-4}$ picobarn in spin-dependent
(SD) interaction of WIMP on proton for mass range about $100\div200$ GeV.
