{"paper":{"title":"Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on 28 model parameters in the CAMELS suite","arxiv_id":"2610.03544","primary_cat":"astro-ph.CO","submitted_at":"2026-10-02T16:27:46+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-1.13.0 on the question bank abstract-p1-20260923, exactly as returned. 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$M_{\\rm vir}$, which characterizes the radial density distribution in halos.","hedge":{"p":0.99,"label":"asserted"},"own_p":0.96,"main_claim_p":0.09,"quantitative":true,"quantitative_p":0.96,"role_probabilities":{"gap":0.0,"method":0.35,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.65,"interpretation":0.0}},{"i":2,"p":0.5,"id":"s2","own":true,"role":"method","text":"We construct a simulation-informed nonlinear model for concentration as a function of halo mass, redshift, and twenty-eight cosmological/astrophysical parameters.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.96,"main_claim_p":0.22,"quantitative":true,"quantitative_p":0.9,"role_probabilities":{"gap":0.0,"method":0.5,"result":0.01,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.49,"interpretation":0.0}},{"i":3,"p":1.0,"id":"s3","own":true,"role":"method","text":"This is done using 2048 simulations of the IllustrisTNG galaxy formation model from the CAMELS suite.","hedge":{"p":0.99,"label":"asserted"},"own_p":0.67,"main_claim_p":0.03,"quantitative":true,"quantitative_p":0.97,"role_probabilities":{"gap":0.0,"method":1.0,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.0,"interpretation":0.0}},{"i":4,"p":0.97,"id":"s4","own":true,"role":"result","text":"We extract the imprints of galaxy formation across a wide range in mass $M_{\\rm vir} \\in [10^{11}, 10^{14.5}]$ $M_{\\odot}/h$ and in redshift $z \\in [0, 3]$, finding clear mass- and redshift-dependent features in each of the different feedback mechanisms.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.97,"main_claim_p":0.18,"quantitative":true,"quantitative_p":0.98,"role_probabilities":{"gap":0.0,"method":0.02,"result":0.97,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.01,"interpretation":0.0}},{"i":5,"p":0.76,"id":"s5","own":true,"role":"contribution","text":"From our measurements, we construct a three-component phenomenological model that can include astrophysical imprints in the concentration--mass relation in a fast and simple manner.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.95,"main_claim_p":0.32,"quantitative":true,"quantitative_p":0.6,"role_probabilities":{"gap":0.0,"method":0.15,"result":0.09,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.76,"interpretation":0.0}}]},"compiled":{"main_claim":{"p":0.65,"text":"From our measurements, we construct a three-component phenomenological model that can include astrophysical imprints in the concentration--mass relation in a fast and simple manner.","location":"abstract s5","hedge_strength":{"p":1.0,"label":"asserted"}},"provenance":{"route":{"via":"TypeSafe API","model":"classifier-1.13.0","endpoint":"https://api.typesafe.ai/v1/systemone","provider":"TypeSafe"},"packing":"one request per paper","requests":1,"input_tokens":5255,"cost_usd_reported":0.0},"compiled_at":"2026-10-05","bank_version":"abstract-p1-20260923","model_version":"classifier-1.13.0","abstract_states":{"claims_first":0.04,"states_limitation":0.09,"human_participants":0.01,"controlled_comparison":0.07,"randomized_assignment":0.01,"states_quantitative_result":0.62,"compares_with_prior_results":0.09,"mentions_code_or_data_availability":0.04},"evidential_basis":{"p":1.0,"value":"simulation or computation","probabilities":{"argument":0.0,"literature":0.0,"proof_or_derivation":0.0,"analysis_of_existing_data":0.0,"observation_or_experiment":0.0,"simulation_or_computation":1.0}},"contribution_type":{"p":0.97,"value":"simulation study","probabilities":{"review":0.0,"method_or_tool":0.03,"empirical_study":0.0,"simulation_study":0.97,"theoretical_result":0.0,"dataset_or_benchmark":0.0,"position_or_commentary":0.0}},"contribution_statement":{"p":0.55,"text":"We construct a simulation-informed nonlinear model for concentration as a function of halo mass, redshift, and twenty-eight cosmological/astrophysical parameters.","location":"abstract s2"}},"coverage":{"tier":"abstract","levels_run":["P abstract"],"not_examined":["full text","figures and tables","references and citing sentences","relations to other papers"],"sources_read":["arXiv listing abstract v1"],"levels_not_run":["S sections","T body sentences","C citations","R cross-paper relations"],"sentences_examined":6,"sentences_in_abstract":6},"measured_accuracy":{"url":"https://pith.science/accuracy","measured_on":"2026-10-02","method":"two independent model families labelled a fresh random sample blind; the figure is how often the published label matches their consensus","sentence_role_agreement":0.92,"main_claim_agreement":0.908,"typed_citation_agreement":0.933,"typed_citation_agreement_95_interval":[0.917,0.945],"review_comments_accurate":0.758,"review_comments_accurate_95_interval":[0.684,0.82],"review_caught_admitted_error_found_or_related":0.448}}