Examples of the SEDs of galaxies in the ANWS. Filled circles indicate observed data points from GALEX UV to AKARI MIR. All objects are detected in S11, except in cases where objects were not detected in the AKARI L15 and L18 bands (Id: 1881, 1266, 1882, 1216, 65, 1264, and 1332), in which cases no points are shown. Overplotted lines represent the best-fit SEDs: the blue solid lines indicate SEDs from Bruzual & Charlot (2003) and the red solid lines indicate infrared galaxy templates of Chary & Elbaz (2001). Each SED fit lists the object Id on top left; stellar age (years), stellar mass ( M _☉), and total L _IR ( L _☉) in units of dex, from left to right, respectively. Each row shows a set of four objects that are representative of our classification scheme (described in Table 4): weak-MXG, intermediate-MXG, weak-SFG, dusty-SFG, and blue-SFG, from top to bottom.