Selected stages for helium-core white dwarf models with stellar masses in the range 0.22-0.52 M_sun resulting from high-metallicity progenitors. Details are given in Althaus, Panei, Romero, et al. 2009, A&A , 502, 207. The calculated He-core WD sequences have masses of 0.220, 0.250, 0.303, 0.358, 0.400, 0.452, 0.513, 0.522 M_sun. UBVRIJHKL and Hubble (with High Resolution Channel) filters for He-core WDs with progenitors with Z=0.03 are provided. Each file refers to a specific evolutionary sequence characterized by a given metallicity, stellar mass, and filter. For instance, z.03.22047.UBVRIJHKL stands for a 0.22047 M_o sequence models with Z=0.03 and UBVRIJHKL filters. Color and magnitudes are based on detailed non-gray model atmospheres that explicitely include Lyman alpha quasi-molecular opacity and computed by Rene Rohrmann (see Rohrmann et al. 2011 for details). As an example, the figure below shows a selected color-color diagram for our sequences (selected effective temperature are labeled along the curves):