{"arxiv_id":"1207.2527","incoming":{"papers":19,"sentences":20,"groups":[{"kind":"background","label":"Cites it as background","papers":8,"sentences":8,"quotes":[{"arxiv_id":"2607.26347","title":"Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters","url":"/paper/2607.26347","section":"Production pathways of Mo and Ru","sentence":"The weak component of the r-process is associated with the neutrino-driven winds from CCSNe and electron-capture supernovae [ref] .","intent_p":0.82,"contests_p":null},{"arxiv_id":"1401.2166","title":"Implications of GRB 130603B and its macronova for r-process nucleosynthesis","url":"/paper/1401.2166","section":"Introduction","sentence":"Traditionally, core-collapse supernovae have been considered as the favored production site [ref] , see [ref] for a recent review.","intent_p":0.94,"contests_p":null},{"arxiv_id":"2009.10059","title":"Near-critical supernova outflows and their neutrino signatures","url":"/paper/2009.10059","section":"Introduction","sentence":"It has been actively studied in the context of the nucleosynthesis calculations [ref] , including possible sterile neutrino effects [ref] .","intent_p":0.98,"contests_p":null},{"arxiv_id":"1301.0911","title":"An Outlook on Nuclear Physics","url":"/paper/1301.0911","section":"r-process nucleosynthesis","sentence":"Our present understanding of neutrino-driven winds was summarized in Ref. [ref] .","intent_p":0.98,"contests_p":null},{"arxiv_id":"1508.00785","title":"Supernova Neutrinos: Production, Oscillations and Detection","url":"/paper/1508.00785","section":"Neutrino-driven outflows from proto-neutron stars","sentence":"This wind is discussed as a potentially important site of heavy-element formation (for recent reviews, see Refs. [ref] ).","intent_p":0.97,"contests_p":null}]}],"unlabelled_sentences":12},"outgoing":{"papers":7,"sentences":13,"groups":[{"kind":"background","label":"Cites as background","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1206.2503","title":"Explosion Mechanisms of Core-Collapse Supernovae","url":"/paper/1206.2503","section":"Introduction","sentence":"This leads to a stalled shock, and it remains an open question how it re-accelerates and produces a successful explosion (see Refs. [ref] ).","intent_p":0.94,"contests_p":null},{"arxiv_id":"1204.5379","title":"Light Sterile Neutrinos: A White Paper","url":"/paper/1204.5379","section":"Additional ingredients","sentence":"The existence of sterile neutrinos remains an open question and it has been used to explain anomalies in some detector experiments [ref] .","intent_p":0.92,"contests_p":null}]}],"unlabelled_sentences":11},"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":"1207.2527","kind":"model","paper_version":1,"prompt_version":"held-up-v3.5","generated_at":"2026-10-27T20:22:27+00:00","loaded_at":"2026-10-28T01:03:47.895948+00:00","evidence":"some","account":[],"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":1,"entries":[{"p":0.96,"quote":null,"citing":[{"self":false,"year":2023,"title":"Proto-Neutron Star Convection and the Neutrino-Driven Wind: Implications for the r-Process","arxiv_id":"2302.01249"}],"verified":true,"paraphrase":"Treated the post-shock outflow behavior following this paper, holding density constant for the first second post-shock with velocity dropping as r^2."}],"papers_all":1,"self_papers":0,"self_entries":[]}],"counts":{"by_kind":{"comparison":1,"method_or_tool":1,"supports_this_paper":3},"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":14,"self_papers":11,"citing_papers":67,"sentences_read":15,"citing_sentences":74,"unambiguous_read":15,"typed_independent":4,"independent_papers":56,"by_kind_independent":{"comparison":1,"method_or_tool":1,"supports_this_paper":2}},"input_sha256":"7bddc3d97192fa675c6effbf50261c7ce7acc5fe1cb066acd98fc9a73a7f1f9c","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 method or tool."},"_links":{"html":"https://pith.science/paper/1207.2527"}}