{"arxiv_id":"2210.07560","incoming":{"papers":6,"sentences":19,"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":1,"sentences":2,"quotes":[{"arxiv_id":"2407.07847","title":"Litmus tests of the flat $\\Lambda$CDM model and model-independent measurement of $H_0r_\\mathrm{d}$ with LSST and DESI","url":"/paper/2407.07847","section":"Mock Data Generation","sentence":"The procedure encompasses four primary stages, depicted in Figure 4 of [ref] .","intent_p":0.9,"contests_p":null}]},{"kind":"data_used","label":"Uses its data or values","papers":1,"sentences":3,"quotes":[{"arxiv_id":"2407.07847","title":"Litmus tests of the flat $\\Lambda$CDM model and model-independent measurement of $H_0r_\\mathrm{d}$ with LSST and DESI","url":"/paper/2407.07847","section":"Mock Data Generation","sentence":"The covariance matrix corresponds to the combined statistical and systematic errors, where the latter encompasses all individual systematics, detailed in Table 3 of [ref] .","intent_p":0.97,"contests_p":null}]},{"kind":"comparison","label":"Compares with it","papers":2,"sentences":2,"quotes":[{"arxiv_id":"2306.05819","title":"Binning is Sinning: Redemption for Hubble Diagram using Photometrically Classified Type Ia Supernovae","url":"/paper/2306.05819","section":"Conclusion","sentence":"While our unbiased results are encouraging, we note that [ref] reported a significant cosmology bias using an unbinned HD from a simulated LSST data sample of pure SNe Ia.","intent_p":0.83,"contests_p":null},{"arxiv_id":"2407.07847","title":"Litmus tests of the flat $\\Lambda$CDM model and model-independent measurement of $H_0r_\\mathrm{d}$ with LSST and DESI","url":"/paper/2407.07847","section":"Mock Data Generation","sentence":"While the analysis by [ref] relies solely on SNIa with spectroscopically confirmed host redshifts, [ref] broadens the scope by including a comprehensive end-to-end analysis that incorporates both spectroscopic and photometric redshifts of host galaxies.","intent_p":0.96,"contests_p":null}]}],"unlabelled_sentences":12},"outgoing":{"papers":3,"sentences":5,"groups":[{"kind":"extends","label":"Builds on","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2111.06858","title":"SNIa-Cosmology Analysis Results from Simulated LSST Images: from Difference Imaging to Constraints on Dark Energy","url":"/paper/2111.06858","section":"Analysis","sentence":"This analysis is similar to the recent DC2-SNIa cosmology analysis in [ref] , except here we include DDF and use photo-$z$ information.","intent_p":0.9,"contests_p":null}]},{"kind":"data_used","label":"Uses data or values from","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2111.06858","title":"SNIa-Cosmology Analysis Results from Simulated LSST Images: from Difference Imaging to Constraints on Dark Energy","url":"/paper/2111.06858","section":"High-$z$ data :","sentence":"We adopt the detection efficiency vs. signal-to-noise ratio (SNR) from the DC2 analysis as shown in Fig. 9 of [ref] .","intent_p":0.98,"contests_p":null}]}],"unlabelled_sentences":3},"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/2210.07560"}}