{"arxiv_id":"astro-ph/0510614","incoming":{"papers":1,"sentences":1,"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2401.15787","title":"Reflecting on Accretion in Neutron Star Low-Mass X-ray Binaries","url":"/paper/2401.15787","section":"Reflection Modeling","sentence":"Additionally, ad-hoc convolution reflection models were created that piece together expected shapes in different energy bands, such as rfxconv [ref] , which generates an angle-dependent reflection spectrum from a Comptonized input spectrum by combining the reflection emission from an ionized disk interpolated from reflionx [ref] below 14 keV (using the average 2–10 keV power-law index) with Compton reflected emission from pexriv [ref] above 14 keV (using the average 12–14 keV power-law index).","intent_p":0.83,"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/0510614"}}