{"arxiv_id":"gr-qc/0204090","incoming":{"papers":47,"sentences":57,"groups":[{"kind":"data_used","label":"Uses its data or values","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1203.6603","title":"Compact binary coalescence parameter estimations for 2.5 post-Newtonian aligned spinning waveforms","url":"/paper/1203.6603","section":"Sensitivity curves","sentence":"The sensitivity curve used here for advanced LIGO [ref] , with $f_0=215$Hz, is","intent_p":0.9,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":29,"sentences":33,"quotes":[{"arxiv_id":"1701.00418","title":"Identifying the QCD Phase Transitions via the Gravitational Wave Frequency","url":"/paper/1701.00418","section":"Introduction","sentence":"The potential high-frequency sources sought by earth-based gravitational-wave detectors, such as LIGO, VIRGO, GEO600, TAMA300, include not only the BH/BH merger and ringdown, as the source of the gravitational-wave event GW150914 [ref] , but also the tidal disruption of a neutron star (NS) by its companion BH in NS/BH binaries, spinning NSs, type-II supernovae, proto-neutron-stars produced by the accretion-induced collapse of white dwarf stars, etc., for more details about the gravitational-wave sources, see, e.g., Refs. [ref] .","intent_p":0.84,"contests_p":null},{"arxiv_id":"2606.18184","title":"Beyond Plane Waves: Coherent Network Response to Collimated Gravitational-Wave Wavepackets","url":"/paper/2606.18184","section":"Introduction","sentence":"In all cases, the detector response is typically modeled for an incoming plane wave, with the measured strain given by projecting the metric perturbation onto the interferometer tensor response [ref] .","intent_p":0.91,"contests_p":null},{"arxiv_id":"1709.09810","title":"Comparison of gravitational waves from central engines of gamma-ray bursts: neutrino-dominated accretion flows, Blandford-Znajek mechanisms, and millisecond magnetars","url":"/paper/1709.09810","section":"Results","sentence":"Before the central BHs or magnetars are born to power GRBs, the compact binary mergers and collapsars are also important GW sources [ref] .","intent_p":0.98,"contests_p":null},{"arxiv_id":"1308.1397","title":"Inadequacies of the Fisher Information Matrix in gravitational-wave parameter estimation","url":"/paper/1308.1397","section":"Introduction","sentence":"By 2015, the first generation of gravitational wave detectors capable of detecting astrophysical sources will become operational [ref] .","intent_p":0.98,"contests_p":null},{"arxiv_id":"0903.4160","title":"Limits on high-frequency gravitational wave background from its interplay with large scale magnetic fields","url":"/paper/0903.4160","section":"Introduction","sentence":"Although most astrophysical sources radiate gravitational waves at much lower frequencies $ν≲10^3 Hz$ [ref] , the high frequencies might contain gravitational wave signal coming from the very early Universe as well as some other sources and mechanisms such as cosmic strings, evaporation of light primordial black holes and effects associated with presence of higher dimensions [ref] .","intent_p":0.97,"contests_p":null}]}],"unlabelled_sentences":23},"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":"gr-qc/0204090","kind":"model","paper_version":1,"prompt_version":"held-up-v3.5","generated_at":"2026-10-27T23:35:46+00:00","loaded_at":"2026-10-28T01:04:38.610329+00:00","evidence":"thin","account":[],"groups":[{"kind":"data_used","label":"Uses its data or values","papers":1,"entries":[{"p":0.9,"quote":null,"citing":[{"self":false,"year":2012,"title":"Compact binary coalescence parameter estimations for 2.5 post-Newtonian aligned spinning waveforms","arxiv_id":"1203.6603"}],"verified":true,"paraphrase":"Used this paper's sensitivity curve for advanced LIGO, with f0=215 Hz, in its own work."}],"papers_all":1,"self_papers":0,"self_entries":[]}],"counts":{"by_kind":{"data_used":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":19,"self_papers":0,"citing_papers":49,"sentences_read":19,"citing_sentences":59,"unambiguous_read":19,"typed_independent":1,"independent_papers":49,"by_kind_independent":{"data_used":1}},"input_sha256":"6dd47b9483610884d51fd58388a409843206ef17e36c35011872931b0209a07c","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/gr-qc/0204090"}}