-----> 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