{"arxiv_id":"1402.3220","incoming":{"papers":5,"sentences":5,"groups":[{"kind":"data_used","label":"Uses its data or values","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2105.13549","title":"Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing","url":"/paper/2105.13549","section":"Photometric redshifts","sentence":"A redshift distribution is inferred for each of the deep-field galaxy phenotypes using overlapping spectroscopic [ref] , and photometric COSMOS [ref] and PAUS [ref] redshift measurements.","intent_p":0.93,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":3,"sentences":3,"quotes":[{"arxiv_id":"2103.01571","title":"J-PAS: Forecasts for dark matter - dark energy elastic couplings","url":"/paper/2103.01571","section":"Introduction","sentence":"Among the current and future spectro-photometric surveys we have PAU [ref] , J-PLUS [ref] and the future J-PAS [ref] .","intent_p":0.93,"contests_p":null},{"arxiv_id":"2007.05360","title":"The Fisher gAlaxy suRvey cOde ($\\texttt{FARO}$)","url":"/paper/2007.05360","section":"Introduction","sentence":"Examples of spectro-photometric surveys are PAU [ref] J-PLUS [ref] and the future J-PAS [ref] .","intent_p":0.87,"contests_p":null},{"arxiv_id":"1405.4769","title":"Comparison of piecewise-constant methods for dark energy","url":"/paper/1405.4769","section":"Introduction","sentence":"Huge experimental efforts have been made to better understand the expansion of the Universe, see for instance [ref] , [ref] [ref] , [ref] , [ref] for details on the surveys of Euclid, DES and PAU.","intent_p":0.98,"contests_p":null}]}],"unlabelled_sentences":1},"outgoing":{"papers":1,"sentences":1,"groups":[],"unlabelled_sentences":1},"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/1402.3220"}}