{"paper":{"title":"Reconstructing Dark Matter Properties via Gamma-Rays with Fermi-LAT","arxiv_id":"1012.0217","primary_cat":"astro-ph.HE","submitted_at":"2010-12-01T15:29:27+00:00","version_compiled":"v1"},"notice":"Every quoted sentence is the authors' text from the arXiv listing abstract. Labels and probabilities are the outputs of classifier-1.13-20260917 on the question bank abstract-p1-20260923, exactly as returned. 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positrons generated in Dark Matter annihilations off the interstellar photon background.","hedge":{"p":0.98,"label":"asserted"},"own_p":0.79,"main_claim_p":0.03,"quantitative":false,"quantitative_p":0.05,"role_probabilities":{"gap":0.0,"method":0.92,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.08,"interpretation":0.0}},{"i":2,"p":0.76,"id":"s2","own":true,"role":"result","text":"We show that the addition of this contribution is crucial in the case of annihilations into e^+ e^- and mu^+ mu^- pairs.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.79,"main_claim_p":0.08,"quantitative":false,"quantitative_p":0.08,"role_probabilities":{"gap":0.0,"method":0.02,"result":0.76,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.02,"interpretation":0.2}},{"i":3,"p":0.97,"id":"s3","own":true,"role":"method","text":"In addition to the diffuse galactic and extragalactic background, we also consider the full catalog of high-energy gamma-ray point sources detected by Fermi.","hedge":{"p":0.98,"label":"asserted"},"own_p":0.59,"main_claim_p":0.02,"quantitative":false,"quantitative_p":0.08,"role_probabilities":{"gap":0.0,"method":0.97,"result":0.0,"background":0.01,"limitation":0.0,"future_work":0.0,"contribution":0.02,"interpretation":0.0}},{"i":4,"p":0.87,"id":"s4","own":true,"role":"contribution","text":"The impact of the degeneracies between the different Dark Matter annihilation channels has been studied.","hedge":{"p":0.78,"label":"asserted"},"own_p":0.8,"main_claim_p":0.03,"quantitative":false,"quantitative_p":0.04,"role_probabilities":{"gap":0.0,"method":0.12,"result":0.01,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.87,"interpretation":0.0}},{"i":5,"p":0.99,"id":"s5","own":true,"role":"result","text":"We find that for Dark Matter masses below ~200 GeV and for typical thermal annihilation cross sections, it will be possible to obtain stringent bounds on the Dark Matter 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