{"arxiv_id":"2009.11175","incoming":{"papers":8,"sentences":11,"groups":[{"kind":"supports_this_paper","label":"Cites it as support","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2103.00014","title":"The Quasar Feedback Survey: Discovering hidden Radio-AGN and their connection to the host galaxy ionised gas","url":"/paper/2103.00014","section":"Our sample in context","sentence":"Overall, by focusing on sources at $z≈0.1$, our survey allows for both a reasonable spatial resolution ($∼$1 kpc) and sensitivity, whilst also allowing us to build up a sample of bolometrically luminous AGN [ref] .","intent_p":0.97,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":2,"sentences":2,"quotes":[{"arxiv_id":"2603.03951","title":"The influence of galaxy mergers, black-hole growth, and gas processes on the evolution of the stellar mass-gas metallicity relation of galaxies in different cosmic environments","url":"/paper/2603.03951","section":"Introduction","sentence":"Over the last few decades, AGN have been shown to both negatively [ref] and positively [ref] impact the SFR of galaxies.","intent_p":0.86,"contests_p":null},{"arxiv_id":"2608.12482","title":"CLASSY. XV. Kinematics and Spatial Distributions of Outflows in Local Highly Star-Forming Galaxies","url":"/paper/2608.12482","section":"Introduction","sentence":"Driven by radiation pressure and mechanical energy deposited by supernovae, stellar winds [ref] , and AGN [ref] , they are observed ubiquitously at low and high redshifts [ref] .","intent_p":0.91,"contests_p":null}]}],"unlabelled_sentences":8},"outgoing":{"papers":2,"sentences":8,"groups":[{"kind":"comparison","label":"Compares with","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2003.06153","title":"Ionized outflows in local luminous AGN: what are the real densities and outflow rates?","url":"/paper/2003.06153","section":"Discussion","sentence":"* The [ref] and the [ref] studies of warm ionised outflows of low-to-moderate luminosity AGN in the local universe ($z < 0.15$).","intent_p":0.89,"contests_p":null}]},{"kind":"supports_this_paper","label":"Cites as support","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2008.11210","title":"A Catalog of 406 AGNs in MaNGA: A Connection between Radio-mode AGN and Star Formation Quenching","url":"/paper/2008.11210","section":"Introduction","sentence":"This is based both on statistical studies of large samples of SDSS-selected AGN [ref] and on a growing number of observations of individual objects in which the outflows show detailed morphological associations with the radio lobes on kpc scales (e.g. IC 5063: [ref] ; SDSS J165315.06+232943.0: [ref] ; NGC 613: [ref] ; 3C 273: [ref] ; HE 1353-1917: [ref] ; ESO 428-G14: [ref] ; NGC 5929: [ref] ; NGC 1386: [ref] ; and the targets in the sample of [ref] ).","intent_p":0.97,"contests_p":null}]}],"unlabelled_sentences":6},"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/2009.11175"}}