Resolved 1.1 mm EBL computed from the best-fit Schechter function to the differential number counts. The green, red, purple and brown lines are from the number counts estimated by Fujimoto et al. (2016), Ono et al. (2014), Hatsukade et al. (2016), and Carniani et al. (2015) respectively. The blue line and shaded region show the results from this work and the associated uncertainty. The solid lines represent the model above the detection limits, and the dashed lines show the extrapolation below these limits. The gray shaded region shows the 1.1 mm cosmic infrared background measured by COBE (Fixsen et al. 1998).