Relation of dust temperature versus dust luminosity for local (left panel), and higher redshift LIRGs and ULIRGs (right panel). Red squares represent ULIRGs, and blue triangles – LIRGs from the ADF–S sample (empty symbols represent object without Herschel data). Left panel: open magenta circles denote Pereira-Santaella et al. (2015) sample of LIRGs, open green triangles stand for Symeonidis et al. (2013), black “x-s” – U et al. (2012) sample of LIRGs and ULIRGs, and open cyan squares – Clements et al. (2010) sample of ULIRGs at redshift range z < 1. Right panel: open magenta traingles represent Santos et al. (2015) sample of LIRGs and ULIRGs, black “x-s” – LIRGs and ULIRGs from da Cunha et al. (2015), and green open circles represent Yan et al. (2014) ULIRGs sample. The errorbars of da Cunha et al. (2015) data were not shown since they are very large and make the plot unreadable.