Comparison of total dust luminosity estimated using different wavelength range for 686 ELAIS N1 galaxies with PACS green and PACS red measurements with S/N ≽ 1.5, SPIRE 250, and SPIRE 350 S/N ≽ 3 and at least six UV–NIR measurements; panel a: results of SED fitting based on the full sets of data (x-axis) are compared with L_dust estimated based on the UV–NIR data only (y-axis); panle b: results of SED fitting based on the full sets of data (x-axis) compared to estimates from PACS and SPIRE data only (y-axis); and panel c: results of SED fitting based on the UV–NIR data ( x-axis) vs. estimates from PACS and SPIRE data only (y-axis). Blue solid lines represent 1:1 relations, while red dashed lines correspond to linear fits to the data. Pearson product-moment correlation coefficient is given as an r value. Δ represents the mean difference between x-axis and y-axis values and the standard deviation of that difference.