  The Local Volume Complete Cluster Survey (LoVoCCS) is an on-going program to
observe nearly a hundred low-redshift X-ray-luminous galaxy clusters (redshifts
$0.03<z<0.12$ and X-ray luminosities in the 0.1-2.4 keV band $L_{{\rm
X500c}}>10^{44}$ erg/s) with the Dark Energy Camera (DECam), capturing data in
$u,g,r,i,z$ bands with a $5\sigma$ point source depth of approximately 25-26th
AB magnitudes. Here, we map the aperture masses in 58 galaxy cluster fields
using weak gravitational lensing. These clusters span a variety of dynamical
states, from nearly relaxed to merging systems, and approximately half of them
have not been subject to detailed weak lensing analysis before. In each cluster
field, we analyze the alignment between the 2D mass distribution described by
the aperture mass map, the 2D red-sequence (RS) galaxy distribution, and the
brightest cluster galaxy (BCG). We find that the orientations of the BCG and
the RS distribution are strongly aligned throughout the interiors of the
clusters: the median misalignment angle is 19 deg within 2 Mpc. We also observe
the alignment between the orientations of the RS distribution and the overall
cluster mass distribution (by a median difference of 32 deg within 1 Mpc),
although this is constrained by galaxy shape noise and the limitations of our
cluster sample size. These types of alignment suggest long-term dynamical
evolution within the clusters over cosmic timescales.
