{"arxiv_id":"1503.03501","incoming":{"papers":12,"sentences":17,"groups":[{"kind":"data_used","label":"Uses its data or values","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2511.03793","title":"Hot accretion onto spiral galaxies: the origin of extended and warped HI discs","url":"/paper/2511.03793","section":"Misaligned hot inflows","sentence":"We assume the average $λ_hot ≈0.06-0.08$ found in cosmological simulations ( [ref] ), a factor of $≈2$ larger than the mean spin of the halo.","intent_p":1.0,"contests_p":null}]},{"kind":"supports_this_paper","label":"Cites it as support","papers":2,"sentences":3,"quotes":[{"arxiv_id":"2003.04800","title":"Observational detection of correlation between galaxy spins and initial conditions","url":"/paper/2003.04800","section":"Introduction","sentence":"Because galaxy spins tend to align with the spins of their DM haloes [ref] , it is expected that this second order quantity can be used to predict galaxy spins as well.","intent_p":0.98,"contests_p":null},{"arxiv_id":"2406.06080","title":"Probing vector chirality in the early Universe","url":"/paper/2406.06080","section":"Introduction","sentence":"This is because the spin of baryon components of a galaxy well aligns with its initial spin [ref] and host halo spin [ref] .","intent_p":1.0,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":2,"sentences":2,"quotes":[{"arxiv_id":"2509.07092","title":"Why Cosmic Voids Matter: Pristine Evolution","url":"/paper/2509.07092","section":"The Magneticum simulations","sentence":"We provide a brief overview of the suite here and refer the reader to previous works for more details [ref] , and in particular to Reference [ref] for a comprehensive description.","intent_p":0.96,"contests_p":null},{"arxiv_id":"2105.15043","title":"Testing the SZ-based tomographic approach to the thermal history of the universe with pressure-density cross-correlations: Insights from the Magneticum simulation","url":"/paper/2105.15043","section":"The Magneticum simulation","sentence":"The simulations follow a wide range of physical processes (see Refs. [ref] for details) which are important for studying the formation of active galactic nuclei (AGN), galaxies, and galaxy groups and clusters.","intent_p":0.9,"contests_p":null}]}],"unlabelled_sentences":11},"outgoing":{"papers":3,"sentences":5,"groups":[{"kind":"method_or_tool","label":"Uses the method or tool of","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1502.07358","title":"An improved SPH scheme for cosmological simulations","url":"/paper/1502.07358","section":"The Magneticum Pathfinder Simulations","sentence":"It includes various updates in the formulation of SPH regarding the treatment of the viscosity and the used kernels (see [ref] ).","intent_p":0.93,"contests_p":null}]},{"kind":"background","label":"Cites as background","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1106.0538","title":"The angular momentum of baryons and dark matter halos revisited","url":"/paper/1106.0538","section":"Introduction","sentence":"[ref] studied the different behavior of the gas and DM specific angular momentum by following the evolution of a Milky-Way-type galaxy over cosmic time.","intent_p":0.85,"contests_p":null}]}],"unlabelled_sentences":3},"claims":[],"thresholds":{"intent_p":0.8,"supports_p":0.95,"contests_p":0.7},"method":"Citing sentences come from each paper's LaTeX source; every \\cite marks the sentence and the works it cites. Pith's classifier typed each sentence. A label is shown at intent probability 0.8 or more (0.95 for support), a contest at 0.7 or more. Measured accuracy against two blind model families is at https://pith.science/accuracy. The quoted sentences are the citing authors' own.","held_up":{"arxiv_id":"1503.03501","kind":"model","paper_version":2,"prompt_version":"held-up-v3.5","generated_at":"2026-10-27T16:24:58+00:00","loaded_at":"2026-10-28T01:02:43.435873+00:00","evidence":"some","account":[],"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":4,"entries":[{"p":0.8,"quote":null,"citing":[{"self":false,"year":2018,"title":"Comparing galaxy morphology in hydrodynamical simulation and in semi-analytic model","arxiv_id":"1812.03645"}],"verified":true,"paraphrase":"Followed the divider adopted by this paper to define galaxies with kinematic bulge-to-total ratio below 0.6 as late-type and above 0.6 as early-type."},{"p":0.8,"quote":null,"citing":[{"self":false,"year":2017,"title":"Flux-ratio anomalies from discs and other baryonic structures in the Illustris simulation","arxiv_id":"1707.07680"}],"verified":true,"paraphrase":"Followed this paper to consider galaxies with more than 40 percent of stars in the thin disc as kinematics-selected disc galaxies."}],"papers_all":9,"self_papers":2,"self_entries":[{"p":1.0,"quote":null,"citing":[{"self":true,"year":2017,"title":"The Morphology-Density-Relation: Impact on the Satellite Fraction","arxiv_id":"1702.06546"}],"verified":true,"paraphrase":"Followed this paper to calculate, for each galaxy, the b-value as the y-intercept of the linear relation in the log-log stellar mass versus stellar angular momentum plane."},{"p":0.97,"quote":null,"citing":[{"self":true,"year":2020,"title":"Kinematics of Simulated Galaxies II: Probing the Stellar Kinematics of Galaxies out to Large Radii","arxiv_id":"2001.02237"}],"verified":true,"paraphrase":"Followed this paper to classify its galaxies by b-value into disk, intermediate and spheroidal categories."}]}],"counts":{"by_kind":{"extends":1,"contests":1,"data_used":7,"comparison":5,"method_or_tool":9,"supports_this_paper":6},"dropped":{"relied_on":0,"unknown_ids":0,"account_lines":0,"contest_vetoed":0,"below_threshold":0,"contest_drawback":0,"contest_without_basis":0,"contest_not_one_sentence":0,"contest_on_group_citation":0},"papers_read":7,"self_papers":43,"citing_papers":112,"sentences_read":7,"citing_sentences":190,"unambiguous_read":7,"typed_independent":14,"independent_papers":69,"by_kind_independent":{"data_used":4,"comparison":3,"method_or_tool":3,"supports_this_paper":4}},"input_sha256":"1851e90f9cee2eafc616c5daa1964bb26154891bb9d435f563282171b072f331","method":"For a paper with five or more citing arXiv papers, Pith selected up to 40 citing sentences its citation classifier typed, read those whose citation markers point at this paper alone, and wrote one paraphrase for each later paper in each group, each resting on one sentence. A later paper is listed under a label only when the classifier gives one of its sentences that label at intent probability 0.8 or more (0.95 for support), Pith's reading of the sentence finds that the citing paper itself did it, and a second check of the paraphrase against the sentence passes. The section lists uses only: building on the paper, using its method, tool, data or values, comparing with it and citing it as support. It does not list criticism or disagreement, so their absence says nothing about how the paper has been received. Code counted the papers, wrote the summary from the listed entries, set the evidence level and linked each entry to its citing paper. Quotes are copied from the citing sentence and shown only when the citing paper's licence is CC BY, CC BY-SA or CC0; otherwise the paraphrase is shown. Papers that share an author with this one are listed apart. A paper with fewer citing papers gets a line counted by code, which names uses only: a later paper whose only label is a contest is counted as not described.","line":null,"summary":"2 later papers by other authors are listed below: 2 used its method or tool. 2 more papers by the same authors are listed: 2 used its method or tool."},"_links":{"html":"https://pith.science/paper/1503.03501"}}