  Our goal is to study the gravitational effects caused by the passage of the
Large Magellanic Cloud (LMC) in its orbit on the stellar halo of the Milky Way
(MW). We employed the Gaia Data Release 3 to construct a halo tracers data set
consisting of K-Giant stars and RR-Lyrae variables. Additionally, we have
compared the data with a theoretical model to estimate the DM subhalo mass. We
have improved the characterisation of the local wake and the collective
response due to the LMC orbit. On the other hand, we have estimated for the
first time the dark subhalo mass of the Large Magellanic Cloud, of the order of
$1.7\times 10^{11}$ M$_{\odot}$, comparable to previously reported values in
the literature.
