{"paper":{"title":"AI-assisted super-resolution cosmological simulations II: Halo substructures, velocities and higher order statistics","arxiv_id":"2105.01016","primary_cat":"astro-ph.CO","submitted_at":"2021-05-03T17:08:21+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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into the deeply non-linear regime where complex structure formation processes take place.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.84,"main_claim_p":0.06,"quantitative":true,"quantitative_p":0.98,"role_probabilities":{"gap":0.0,"method":0.89,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.11,"interpretation":0.0}},{"i":2,"p":0.97,"id":"s2","own":true,"role":"method","text":"We validate the SR model by deploying the model in 10 test simulations of box size 100 Mpc/h, and examine the matter power spectra, bispectra and 2D power spectra in redshift space.","hedge":{"p":0.93,"label":"asserted"},"own_p":0.96,"main_claim_p":0.04,"quantitative":true,"quantitative_p":0.96,"role_probabilities":{"gap":0.0,"method":0.97,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.03,"interpretation":0.0}},{"i":3,"p":1.0,"id":"s3","own":true,"role":"result","text":"We find the generated SR field matches the true HR result at percent level down to scales of k ~ 10 h/Mpc.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.97,"main_claim_p":0.26,"quantitative":true,"quantitative_p":0.98,"role_probabilities":{"gap":0.0,"method":0.0,"result":1.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.0,"interpretation":0.0}},{"i":4,"p":0.76,"id":"s4","own":true,"role":"contribution","text":"We also identify and inspect dark matter halos and their substructures.","hedge":{"p":0.96,"label":"asserted"},"own_p":0.95,"main_claim_p":0.03,"quantitative":false,"quantitative_p":0.04,"role_probabilities":{"gap":0.0,"method":0.2,"result":0.04,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.76,"interpretation":0.0}},{"i":5,"p":0.98,"id":"s5","own":true,"role":"result","text":"Our SR model generate visually authentic small-scale structures, that cannot be resolved by the LR input, and are in good statistical agreement with the real HR results.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.92,"main_claim_p":0.2,"quantitative":false,"quantitative_p":0.36,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.98,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.0,"interpretation":0.02}},{"i":6,"p":0.88,"id":"s6","own":true,"role":"result","text":"The SR model performs satisfactorily on the halo occupation distribution, halo correlations in both real and redshift space, and the pairwise velocity distribution, matching the HR results with comparable scatter, thus demonstrating its potential in making mock halo catalogs.","hedge":{"p":0.99,"label":"asserted"},"own_p":0.96,"main_claim_p":0.22,"quantitative":true,"quantitative_p":0.63,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.88,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.0,"interpretation":0.12}},{"i":7,"p":0.97,"id":"s7","own":false,"role":"interpretation","text":"The SR technique can be a powerful and promising 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