Fig. A.1.
Projected stellar luminosity (left panels) and gas density (right panels) of the environment of the host galaxy ID 404871 (top panels) and ID 138 (bottom panels) at redshift z = 0. Top panels: stellar objects (1)–(3) close to ID 404871 (the white circle marks the host galaxy) are explained in the figure legend. Bottom panels: stellar objects (1) and (2) are identified as DMF substructures of the host galaxy ID 138 (the white circle as above). The luminous galaxy in the lower-right corner is a foreground galaxy, which has a 3D separation of 1626 kpc to the galaxy ID 138. Credits: http://www.illustris-project.org/explorer/ [13.08.2018].
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