FIGURE 3: Fig_3_pass7_front.txt: 100 lines, one for each energy. The first entry of each line is the energy (in MeV) and the remaining 1025 entries show the window beam function W_l^beam, for each multipole between 1 and 1025, for the P7REP_ULTRACLEAN_V15 data selection (front only). Fig_3_pass7_back.txt: same as Fig_3_pass7_front.txt but for the P7REP_ULTRACLEAN_V15 data selection (back only). Fig_3_pixel.txt: 4097 lines. The first entry indicates the angular multipole and the same the corresponding pixel windom function W_l^pixel for a Healpix map with Nside=1024. Energy_bins.txt: the file describes the 13 energy bins used in the analysis. The first column is the lower bound of the bin, the second the upper bound and the third is the arithmetic mean of the two. All energies are in GeV. Cl_p7_xFGL_default_y_z.txt: these files contain the binned auto- and cross-APS for the default data selection and default masks. x stands for either 2 or 3 and it indicates which mask is used (either the one covering 2FGL or 3FGL sources). y and z label the energy bins, z=y for the auto-APS and z>y for the cross-APS. Each file contains 20 lines, one for each bin in multipole. The first column indicates the lower bound of the multipole bin and the second the upper bound. The fourth column is the measured APS and the fifth its estimated error. Both are expressed in cm^-4 s^-2 sr^-1. The files have been used for Figs. 6, 7, 9, 29 and 30 in the paper. CP_p7_3FGL_default.txt: the file contains four blocks. Each block is a symmetric 13x13 matrix. The first contains the best-fit Poissonian APS from the binned APS in Cl_p7_3FGL_default_y_z.txt, for all the possible combinations of the 13 energy bins. The second block shows its estimated errors. Both are measured in cm^-4 s^-2 sr^-1. They are used in Figs. 8, 31 and 32 and showed in Tab. 1 in the paper. The third block contains the chi squared of the best-fit, defined as in Eq. 9 and used to build the histogram in Fig. 10. The fourth block provides the significance of the detection of APS, defined as explained in Sec. V A. Both the significance and the best-fit chi squared are also displayed in Tab. 1. CP_p7_2FGL_default.txt: same as for CP_p7_3FGL_default.txt but for the default 2FGL mask. FIGURE 12 (left panel): Cl_p7_3FGL_no_foreground_cleaning_3_3.txt: the file has 20 lines, one for each multipole bin. The first column is the lower edge of th multipole bin and the second the upper one. The fourth column contains the best-fit APS, measured in cm^-4 s^-2 sr^-1 for the case without foreground cleaning. The following 13 column contain the covariance of the specific multipole bin with all the other multipole bins. The covariance is used for the right panel of Fig. 13. FIGURE 12 (right panel): CP_p7_3FGL_lmin150.txt: the file has the same structure as CP_p7_3FGL_default.txt but contains the best-fit Poissonian APS in the case the fit is performed only above an angular multipole of 143. FIGURE 13 (left panel): Cl_p7_3FGL_default_3_3_full_covariance.txt: the file has the same structure as cl_p7_3FGL_no_foreground_cleaning_3_3.txt but it refers to the default data selection (thus, with foreground cleaning) and the default mask around 3FGL srouces. FIGURE 14: Cl_p8_front_3FGL_default_3_3.txt: the file has the same structure as Cl_p7_3FGL_default_3_3.txt but it contains the binned APS for the Pass 8 front data selection. Cl_p8_PSF3_3FGL_default_3_3.txt: the same as Cl_p8_front_default_3_3.txt but for the Pass 8 PSF3 data selection. FIGURE 15: CP_p8_front_3FGL_default.txt: the file has the same structure as CP_p7_3FGL_default.txt but for the Pass 8 front data selection. Note that only the auto-APS is provided and that there is no best-fit chi squared or significance. CP_p8_PSF3_3FGL_default.txt: the same as CP_p8_PSF3_3FGL_default.txt but for the Pass 8 PSF3 data selection. FIGURE 16 (left panel): Cl_p7_3FGL_front_and_back_3_3.txt: the file has the same structure as Cl_p7_3FGL_default_3_3.txt but it contains the binned APS for the data set including both front- and back-converting events. FIGURE 16 (right panel): CP_p7_3FGL_front_and_back.txt: the file has the same structure as CP_p7_3FGL_default.txt but it contains the best-fit Poissonian PAS for the data set including both front- and back-converting events. Note that only the auto-APS is included. FIGURE 17 (left panel): Cl_p7_3FGL_1degmask_3_3.txt: the file has the same structure as Cl_p7_3FGL_default_3_3.txt but it contains the binned APS for the 1-deg mask. Cl_p7_3FGL_2degmask_3_3.txt: same as Cl_p7_3FGL_1degmask_3_3.txt but for the 2-deg mask. FIGURE 17 (right panel): CP_p7_3FGL_2degmask.txt: the file has the same structure as CP_p7_3FGL_default.txt but it contains the best-fit Poissonian APS for the case with the 2-deg mask. No significance is provided. CP_p7_3FGL_3p5degmask.txt: the file has the same structure as CP_p7_3FGL_default.txt but it contains the best-fit Poissonian APS for the case with the 3.5-deg mask. Only the auto-APS is provided. FIGURE 18: CP_p7_2FGL_large_energy_bins.txt: the file has the same structure as CP_p7_2FGL_default.txt but it refers to the best-fit Poissonian APS in 5 large energy bins, which are defined in Large_energy_bins.txt FIGURE 25 (left panel): Exclusion_limits_ann_b_conservative.txt: the file contains 60 triplets of lines, one for each of the 60 values of DM mass considered. For each mass, the first line refers to the REF scenario, the second to the MAX scenario and the third to the MIN scenario. The first column is the DM mass (in GeV) and the second is the exclusion limit on the log10 of the annihilation cross section (expressed in cm^3 s^-1) for the case of Mmin=10^-6 solar masses. The third and fourth columns indicate which energy bin produce the exclusion limit. The fifth, sixth and sevent column provide the same information but in the case of Mmin=1 solar mass. The eighth, nineth and tenth refer to a Mmin=10^-12 solar masses. FIGURE 25 (right panel): Exclusion_limits_decay_b_conservative.txt: the file has the same structure as Exclusion_limits_ann_b_conservative.txt but it contains the lower limit on the decay lifetime in the case of decaying DM. The decay lifetime is measured in s. FIGURE 28 (left panel): Exclusion_limits_ann_b_2components.txt: the file contains 60 triples of lines, one for each of the 60 values of DM mass considered. For each mass, the first line refers to the REF scenario, the second to the MAX scenario and the third to the MIN one. The first mass is the DM mass (in GeV) and the second is the exclusion limit on the log10 of the annihilation cross section (measured in cm^3 s^-1) for the case of Mmin=10^-6 solar masses. The third column indicates the chi squared of the best fit when data are fitted in terms of the 2-component model and the DM candidate has a mass equal to the value indicated in the first column and an annihilation cross section equal to the value indicated in the second column. The fourth and fifth columns contain the same information but for a Mmin=1 solar mass. The sixth and seventh columns refer to the case with Mmin=10^-12 solar masses. FIGURE 28 (right panel): Exclusion_limits_decay_b_2components.txt: the file has the same structure as Exclusion_limits_ann_b_2components.txt but it contains the lower limit on the decay lifetime in the case of decaying DM. The decay lifetime is measured in s. FIGURE 35: Exclusion_limits_ann_tau_conservative.txt: same as Exclusion_limits_ann_b_conservative.txt but for the tau annihilation channel. Exclusion_limits_decay_tau_conservative.txt: same as Exclusion_limits_decay_b_conservative.txt but for the tau decay channel. FIGURE 36: Exclusion_limits_ann_mu_conservative.txt: same as Exclusion_limits_ann_b_2components.txt but for the mu annihilation channel. Exclusion_limits_decay_mu_conservative.txt: same as Exclusion_limits_decay_b_2components.txt but for the mu decay channel. FIGURE 38: Exclusion_limits_ann_tau_2components.txt: same as Exclusion_limits_ann_b_2components.txt but for the tau annihilation channel. Exclusion_limits_decay_tau_2components.txt: same as Exclusion_limits_decay_b_2components.txt but for the tau decay channel. FIGURE 39: Exclusion_limits_ann_mu_2components.txt: same as Exclusion_limits_ann_b_2components.txt but for the mu annihilation channel. Exclusion_limits_decay_mu_2components.txt: same as Exclusion_limits_decay_b_2components.txt but for the mu decay channel.