{"paper":{"title":"Probing $\\Lambda$CDM cosmology with the Evolutionary Map of the Universe survey","arxiv_id":"1810.06672","primary_cat":"astro-ph.CO","submitted_at":"2018-10-15T20:37:59+00:00","version_compiled":"v2"},"notice":"Every quoted sentence is the authors' text from the arXiv listing abstract. Labels and probabilities are the outputs of classifier-1.13.0 on the question bank abstract-p1-20260923, exactly as returned. 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design sensitivities.","hedge":{"p":0.59,"label":"asserted"},"own_p":0.85,"main_claim_p":0.05,"quantitative":false,"quantitative_p":0.06,"role_probabilities":{"gap":0.0,"method":0.26,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.74,"interpretation":0.0}},{"i":2,"p":0.86,"id":"s2","own":true,"role":"method","text":"We also include a multi-tracer analysis, distinguishing between star-forming galaxies and galaxies with an active galactic nucleus, to further improve EMU's potential.","hedge":{"p":0.92,"label":"asserted"},"own_p":0.85,"main_claim_p":0.03,"quantitative":false,"quantitative_p":0.04,"role_probabilities":{"gap":0.0,"method":0.86,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.14,"interpretation":0.0}},{"i":3,"p":1.0,"id":"s3","own":true,"role":"result","text":"We find that EMU could measure the dark energy equation of state parameters around 35\\% more precisely than existing constraints, and that the 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