{"arxiv_id":"1007.4815","incoming":{"papers":8,"sentences":10,"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":4,"sentences":6,"quotes":[{"arxiv_id":"2307.05714","title":"Strong Lensing and $H_0$","url":"/paper/2307.05714","section":"Supernova time delay cosmography: the “Refsdal” case study","sentence":"First, it was decided to consider only the two models that are based on codes designed to do high-precision cosmography, glee [ref] and glafic [ref] , weighted by their agreement with observables independent of , yielding $H_0=66.6^+4.1_-3.3$ .","intent_p":0.95,"contests_p":null},{"arxiv_id":"2604.02418","title":"Supernova 2025wny: High-angular resolution Keck/NIRC2 observations and preliminary lens modeling","url":"/paper/2604.02418","section":"Lens modeling methodology","sentence":"In this work, we make use of two well-established, independent, lens modeling algorithms, [ref] and Glee [ref] .","intent_p":1.0,"contests_p":null},{"arxiv_id":"2605.05318","title":"HOLISMOKES XXI: Detecting strongly lensed type Ia supernovae from time series of multi-band LSST-like imaging data -- Part II","url":"/paper/2605.05318","section":"Summary of the datasets","sentence":"The lensing configurations are generated using our -based [ref] simulation pipeline [ref] .","intent_p":0.99,"contests_p":null},{"arxiv_id":"2608.27566","title":"TDCOSMO. XXVII. JWST-based Lens Models and H$_0$ Measurement of WFI2033, HE0435, and PG1115","url":"/paper/2608.27566","section":"Comparison with previous work","sentence":"As a reminder many things have changed between the two analyses: i) we used Lenstronomy [ref] instead of GLEE [ref] ; ii) we used JWST NIRCam imaging instead of HST/Keck-AO imaging; iii) we reconstructed the PSF using the STARRED and PSFr algorithms; iv) we used stellar velocity dispersion from JWST NIRSpec spectra, instead of ground based measurements; v) we used new estimates of the external convergence based on Euclid Flagship simulations instead of Millennium based ones.","intent_p":0.8,"contests_p":null}]},{"kind":"data_used","label":"Uses its data or values","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2512.03239","title":"(Re)solving the Complex Multiscale Morphology and V-shaped Spectral Energy Distribution of a Newly Discovered Strongly Lensed Little Red Dot in A383","url":"/paper/2512.03239","section":"Lens Model","sentence":"We adopt the average magnification from the two parametric reconstructions provided; [ref] and [ref] .","intent_p":0.81,"contests_p":null}]},{"kind":"comparison","label":"Compares with it","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1907.06830","title":"Strong gravitational lensing of explosive transients","url":"/paper/1907.06830","section":"Discovery of SN Refsdal.","sentence":"From the observation, the time delay between S1 and SX is measured to $∼350$ days, which is in excellent agreement with several model predictions, in particular those made with glafic [ref] and GLEE [ref] .","intent_p":0.86,"contests_p":null}]}],"unlabelled_sentences":2},"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/1007.4815"}}