Model plot showing the contribution to the RGS spectrum of each of the xabs components that model the absorption troughs seen in NGC 985 for the observations in 2003 (upper left panel), 2013 (upper right panel), 2015a (lower left panel), and 2015b (lower right panel). For clarity, the contribution of Component D has been shifted by 1 dex in flux, the one of Component C by 2 dex, the one of Component B by 3 dex, and the one of Component A by 4 dex, whenever they have been detected.