Abstract
I present bounds on Dark Matter (DM) in the MeV to GeV mass range, obtained by using X-ray measurements from the Integral, XMM-Newton and other telescopes. A crucial element, which allows to derive bounds competitive or stronger than existing ones from other techniques, resides in the inclusion of the contribution from inverse Compton scattering on galactic radiation fields and on the CMB. This contribution is based on [1,2], to which I refer for additional details.
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