{"arxiv_id":"astro-ph/0606346","incoming":{"papers":2,"sentences":2,"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2608.13243","title":"Assessing Planetary Stability and Long-Term Habitability in Nearby Stellar Binaries: 70 Oph, 36 Oph, $\\gamma$ Leo","url":"/paper/2608.13243","section":"Habitable Zone Calculation","sentence":"To determine the habitable zone for each of our stars, we compute the flux using Equation 1 from [ref] [ref] : [equation] where $L_⋆$ is stellar luminosity, $a_p$ is semi-major axis of the planet's orbit, and $e_p$ is the planetary eccentricity.","intent_p":0.94,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2608.05500","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","url":"/paper/2608.05500","section":"Introduction","sentence":"In the first scenario, planets are perturbed to an eccentric orbit by the gravitational influence of an outer body (such as another planet or a stellar companion, known as Kozai-Lidov oscillations), secular interactions or planet-planet scattering [ref] .","intent_p":0.97,"contests_p":null}]}],"unlabelled_sentences":0},"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/0606346"}}