Galactic Diffuse Emission Spectrum between 0.5 and 8.0 MeV and between 30 keV and 8 MeV for the search of PBH Dark Matter

Spectra and response files of the soft gamma-ray spectrum from Inverse Compton scattering in the Milky Way between 0.5 and 8.0 MeV, measured with INTEGRAL/SPI. The fluxes have been extracted with spimodfit assuming GALPROP v56 models according to Voyager 1, AMS-02, and Fermi/LAT data, plus different variants to change the interstellar radiation field, the diffusion properties, or the cosmic-ray halo size. In particular: voyager: propagation model of Bisschoff et al. (2019), Table 2 voyager_Dg10001: \(\delta_1 = 0\) voyager_Dg1Dg205: \(\delta_1 = \delta_2 = 0.5\) voyager_ISRFopt10: factor 10 stronger optical ISFR voyager_z8kpc_KL: thick halo with 8 kpc half-thickness In addition, there are spectra from 30 keV to 8 MeV (spec_0030-8000keV_<name>.fits), separated into: CV: spectrum of unresolved point sources in the Galactic plane, mostly cataclysmic variables (strong systematics) IC: spectrum of Inverse Compton scattering of cosmic ray GeV electrons (see above) positronium: spectrum of positronium decay (annihilation of electrons with positrons after intermediate bound state) NFW: spectrum of dark matter contributions that would follow a Navarro Frenk White density profile (mostly consistent with zero) total: spectrum of the above combined