{"arxiv_id":"astro-ph/9911167","incoming":{"papers":4,"sentences":5,"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2511.16658","title":"Prospects for Neutrino Observation and Mass Measurement from Binary Neutron Star Mergers","url":"/paper/2511.16658","section":"Background mitigation","sentence":"The time delay of a neutrino emitted at the moment of neutron star coalescence at redshift $z$, relative to the gravitational wave signal of coalescence, is given by [ref] [equation] where $m_ν$ is the mass of the neutrino mass eigenstate under consideration and $E_ν(z')=(1+z') E_ν$, with $E_ν$ being the neutrino energy at Earth.","intent_p":0.86,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1806.08611","title":"Relations between physical observables: what is better?","url":"/paper/1806.08611","section":"Introduction","sentence":"Despite the fact that some proposals of new distance indicators with ultra-relativistic particles emitted from the source have been recently investigated from the theoretical point of view [ref] , most of the cosmological distance tools involve massless particles which travel from the source to the observer's laboratory.","intent_p":0.92,"contests_p":null},{"arxiv_id":"1604.03543","title":"On the time delay between ultra-relativistic particles","url":"/paper/1604.03543","section":"Introduction","sentence":"The idea of using time delays between UR particles as a cosmological probe is more recent [ref] (see also the short review [ref] ).","intent_p":0.98,"contests_p":null}]}],"unlabelled_sentences":2},"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":null,"_links":{"html":"https://pith.science/paper/astro-ph/9911167"}}