-----> READ ME TO USE THE IDL SAVE FROM BETHERMIN ET AL. (2011) MODEL (A&A 529 A4) The different files contain: - dndsnudz_arr_final.save contains the total contribution. - dndsnudz_arr_lensed_final.save contains the contribution of the strongly-lensed sources (magnification greater than 2). - dndsnudz_arr_unlensed_final.save contains the contribution of non-lensed sources. Array contain in the ILD SAVE file: - LAMBDA: vector of wavelengths (in microns). - SNU: vector of fluxesssss (un Jy). - Z: vector of redshift - DNDSNUDZ_ARR: array containing dN/dS/dz (in gal/Jy/sr). The first dimension corresponds to Snu, the second to Z, the third to LAMBDA. The fourth dimension corresponds to the index of the realization of the model (taken randomly in the Markov chain). If you use the mean model files, there is a single realization corresponding to the mean parameters given in the Table 1 of the paper. The different wavelength correspond to different large band filters. 24: MIPS 24 70: MIPS 70 160: MIPS 160 250: SPIRE 250 350: SPIRE 350 500: SPIRE 500 1100: Generic filter with lambda/dlambda = 3 centered on 1.1 mm. 15: ISO 15 microns 60: IRAS 60 75: PACS 75 110: PACS 110 165: PACS 165 1200: MAMBO 355,550,840,1380,2100,3000: Planck filters