  We report on the progress of our five-year program for astrometric monitoring
of magnetars using high-resolution NIR observations using the laser guide star
adaptive optics (LGS-AO) supported NIRC2 camera on the 10-meter Keck telescope.
We have measured the proper motion of two of the youngest magnetars,
SGR\,1806$-$20 and SGR\,1900+14, which have counterparts with K $\sim$21\,mag,
and have placed a preliminary upper limit on the motion of the young
AXP\,1E\,1841$-$045. The precision of the proper motion measurement is at the
milliarcsecond per year level. Our proper motion measurements now provide
evidence to link SGR\,1806$-$20 and SGR\,1900+14 with neighboring young star
clusters. At the distances of these magnetars, their proper motion corresponds
to transverse space velocities of $350\pm100\,\mathrm{km\,s^{-1}}$ and
$130\pm30\,\mathrm{km\,s^{-1}}$ respectively. The upper limit on the proper
motion of AXP\,1E\,1841$-$045 is $160\,\mathrm{km\,s^{-1}}$. With the sample of
proper motions available, we conclude that the kinematics of the magnetar
family are not distinct from that of pulsars.
