{"arxiv_id":"astro-ph/0404451","incoming":{"papers":34,"sentences":42,"groups":[{"kind":"background","label":"Cites it as background","papers":19,"sentences":21,"quotes":[{"arxiv_id":"1608.08138","title":"Dust polarization and ISM turbulence","url":"/paper/1608.08138","section":"Introduction","sentence":"Models of MHD turbulence predict the power spectra for these different types of modes as a function of the magnitude and orientation (with respect to the background magnetic field) of the wavevector $$ [ref] .","intent_p":0.96,"contests_p":null},{"arxiv_id":"2301.13221","title":"Universal gravity-driven isothermal turbulence cascade in disk galaxies","url":"/paper/2301.13221","section":"Introduction","sentence":"Gas in galaxies is supersonically turbulent [ref] .","intent_p":0.95,"contests_p":null},{"arxiv_id":"2607.05156","title":"Emergence of high-mass stars in complex fiber networks (EMERGE) VI. Turbulence dissipation and the formation of dense fibers","url":"/paper/2607.05156","section":"Signatures of turbulence dissipation and intermittency","sentence":"Following the [ref] model of turbulence, the energy injected at large scales is progressively transferred to smaller scales, until it dissipates by viscosity at much smaller scales [ref] .","intent_p":0.95,"contests_p":null},{"arxiv_id":"2607.09464","title":"Characterising the Kinematics and Evolution of Young Stellar Groups within 1 kpc of the Sun Using Gaia DR3","url":"/paper/2607.09464","section":"Introduction","sentence":"Investigating these motions helps us unravel the complex physical processes governing the lifecycle of molecular clouds and their role in shaping the Galactic environment [ref] .","intent_p":0.98,"contests_p":null},{"arxiv_id":"1111.2329","title":"Multifluid magnetohydrodynamic turbulence in weakly ionised astrophysical plasmas","url":"/paper/1111.2329","section":"Introduction","sentence":"It is generally believed that molecular clouds are turbulent (see the reviews of [ref] ).","intent_p":0.92,"contests_p":null}]}],"unlabelled_sentences":21},"outgoing":{"papers":0,"sentences":0,"groups":[],"unlabelled_sentences":0},"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":"astro-ph/0404451","kind":"model","paper_version":1,"prompt_version":"held-up-v3.5","generated_at":"2026-10-27T08:58:04+00:00","loaded_at":"2026-10-28T01:02:04.737494+00:00","evidence":"some","account":[],"groups":[{"kind":"data_used","label":"Uses its data or values","papers":1,"entries":[{"p":0.87,"quote":null,"citing":[{"self":false,"year":2022,"title":"R-process Rain from Binary Neutron Star Mergers in the Galactic Halo","arxiv_id":"2205.03913"}],"verified":true,"paraphrase":"Used this paper's outer scale of about 100 pc, together with an RMS turbulence velocity, to estimate a turbulent diffusion coefficient of about 1 kpc^2 per Gyr."}],"papers_all":3,"self_papers":0,"self_entries":[]}],"counts":{"by_kind":{"data_used":3,"comparison":1},"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":11,"self_papers":4,"citing_papers":229,"sentences_read":12,"citing_sentences":283,"unambiguous_read":12,"typed_independent":4,"independent_papers":225,"by_kind_independent":{"data_used":3,"comparison":1}},"input_sha256":"09cdb1a2577d1bf0dcc1a5fe2954784ce99237fffda211a347d355d633ce2bfa","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":"1 later paper by other authors is listed below: 1 used its data or values."},"_links":{"html":"https://pith.science/paper/astro-ph/0404451"}}