Fig. 7.From: Dusty Universe viewed by AKARI far infrared detectorThe SFR vs stellar mass relation for ADF–S (U)LIRG sample (black circles). The variable size of points represents the difference in redshift (increasing size from z equal to 0.09 to 0.98). We overplot the Howell et al. (2010) GOALS sample (open triangles), and U et al. (2012) (U)LIRG sample (open squares). The two solid black lines correspond to the SFR-Mstar observation from Elbaz et al. (2007). The dashed line indicates the SFR—stellar mass relation for star-forming galaxies at z ~ 2 defined by Daddi et al. (2007).Back to article page