Emission measure weighted gas mass density (top panel), temperature (middle panel), and metallicity (bottom panels) profiles together with their percentage deviations (corresponding bottom rows; see Eq. (3)) of halos located in different LSE in increasing halo-mass bins from left to right. The different cosmic environments considered here are filaments (green), filament-void transition region (red), and voids and walls (purple). The shaded regions show the 16th to 84th percentile distributions.