# Differential number counts at 24um (Spitzer MIPS) # See Bethermin, Dole, Beelen, Aussel 2009 "Spitzer Deep and Wide Legacy Mid- and Far-Infrared Number Counts and Lower Limits of Cosmic Infrared Background" (submitted A&A) for details # Smin Smax | dNdS*S^2.5 sig_poiss sig_clus sig_tot| Sused # mJy | Jy^2.5.sr^-1 | deg^2 0.040 0.035 0.044 17.6 1.0 1.1 1.3 0.2 0.050 0.044 0.056 21.5 1.0 1.2 1.4 0.2 0.064 0.056 0.071 28.2 1.2 1.5 1.8 0.2 0.081 0.071 0.090 36.2 1.5 1.9 2.4 0.2 0.102 0.090 0.114 52.7 1.3 1.9 2.9 0.6 0.130 0.114 0.145 64.1 1.0 1.7 3.1 3.4 0.164 0.145 0.184 78.8 1.1 2.2 3.8 3.4 0.208 0.184 0.233 89.8 1.3 2.8 4.5 3.4 0.264 0.233 0.295 96.5 1.5 3.3 5.1 3.4 0.335 0.295 0.374 102.7 0.7 1.7 4.4 37.2 0.424 0.374 0.474 94.7 0.6 1.5 4.1 46.1 0.538 0.474 0.601 83.2 0.5 1.4 3.6 53.6 0.681 0.601 0.762 74.4 0.6 1.4 3.3 53.6 0.863 0.762 0.965 66.7 0.7 1.4 3.0 53.6 1.094 0.965 1.223 59.7 0.7 1.5 2.8 53.6 1.387 1.223 1.550 55.0 0.9 1.6 2.7 53.6 1.758 1.550 1.965 53.1 1.0 1.7 2.7 53.6 2.228 1.965 2.490 51.1 1.2 1.9 2.8 53.6 2.823 2.490 3.156 51.5 1.4 2.2 3.0 53.6 3.578 3.156 4.000 51.0 1.7 2.5 3.2 53.6 5.807 4.000 7.615 50.0 1.5 2.7 3.3 53.6 11.055 7.615 14.496 44.3 2.3 3.4 3.9 53.6 21.045 14.496 27.595 35.2 3.3 4.3 4.5 53.6 40.063 27.595 52.531 39.5 5.6 7.3 7.5 53.6 76.265 52.531 100.000 39.4 9.0 11.1 11.2 53.6