{"arxiv_id":"2305.00988","incoming":{"papers":3,"sentences":3,"groups":[{"kind":"background","label":"Cites it as background","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2401.12276","title":"Characterization of K2-167 b and CALM, a new stellar activity mitigation method","url":"/paper/2401.12276","section":"Introduction","sentence":"There have been recent developments in using advanced flexible models like Gaussian Process (GP) regression to model quasi-periodic stellar activity signals and reveal planet signals [ref] .","intent_p":0.97,"contests_p":null}]}],"unlabelled_sentences":2},"outgoing":{"papers":3,"sentences":8,"groups":[{"kind":"background","label":"Cites as background","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1711.01318","title":"Improving Exoplanet Detection Power: Multivariate Gaussian Process Models for Stellar Activity","url":"/paper/1711.01318","section":"Introduction","sentence":"These techniques range in complexity, beginning with using a GP as a correlated red noise filter [ref] to leveraging information from ancillary photometery to further constrain the GP trained on the RVs [ref] , to jointly modeling spectrosphic activity indicators and RVs with a multidimensional GP in order to constrain the activity signals [ref] .","intent_p":0.94,"contests_p":null}]}],"unlabelled_sentences":7},"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/2305.00988"}}