{"arxiv_id":"2012.11616","incoming":{"papers":8,"sentences":16,"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2207.09128","title":"Redshifted 21-cm bispectrum: Impact of the source models on the signal and the IGM physics from the Cosmic Dawn","url":"/paper/2207.09128","section":"Results","sentence":"Further, we follow the convention of [ref] and [ref] to demonstrate our result in terms of spherically averaged normalized power spectrum and bispectrum that are respectively defined as $Δ^2(k) = [ k^3 P(k)/(2π^2)]$ and $Δ^3(k_1, n, cosθ) = [ k_1^3 k_2^3 B(k_1, k_2, k_3)/(2π^2)^2]$.","intent_p":0.97,"contests_p":null}]},{"kind":"data_used","label":"Uses its data or values","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2407.03523","title":"Inferring IGM parameters from the redshifted 21-cm Power Spectrum using Artificial Neural Networks","url":"/paper/2407.03523","section":"Modeling the 21-cm signal with grizzly","sentence":"For this paper, the simulations considered use the gridded dark-matter density fields and the corresponding halo lists within comoving cubes of side 500 $ℎ^-1$ Mpc, produced from the PRACE4LOFAR[Partnership for Advanced Computing in Europe: <http://www.prace-ri.eu/>] N-body simulations (for the details of the simulation, see e.g, [ref] ).","intent_p":0.8,"contests_p":null}]},{"kind":"supports_this_paper","label":"Cites it as support","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2207.09128","title":"Redshifted 21-cm bispectrum: Impact of the source models on the signal and the IGM physics from the Cosmic Dawn","url":"/paper/2207.09128","section":"Introduction","sentence":"However, the cumulative effect of radiation source clustering, non-uniform heating, and ionization of the IGM gas by those sources introduce a high level of non-Gaussianity in the CD-EoR 21-cm maps [ref] .","intent_p":0.97,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":2,"sentences":2,"quotes":[{"arxiv_id":"2102.11153","title":"The HI intensity mapping bispectrum including observational effects","url":"/paper/2102.11153","section":"Introduction","sentence":"Recent work has investigated the post-reionisation redshift space intensity mapping bispectrum analytically (see e.g. [ref] ), as well as higher-redshift studies with simulated signals [ref] .","intent_p":0.97,"contests_p":null},{"arxiv_id":"2107.14564","title":"A fast estimator for quantifying the shape dependence of the 3D bispectrum","url":"/paper/2107.14564","section":"Introduction","sentence":"Measurements of the bispectrum of the 21-cm radiation from the cosmic dawn [ref] , the epoch of reionization (e.g. [ref] ) and the post-reionization era (e.g. [ref] ) are expected to yield a wealth of information regarding the evolutionary history of the universe.","intent_p":0.84,"contests_p":null}]}],"unlabelled_sentences":11},"outgoing":{"papers":3,"sentences":6,"groups":[{"kind":"comparison","label":"Compares with","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1907.04342","title":"The 21cm bispectrum during reionization: a tracer of the ionization topology","url":"/paper/1907.04342","section":"Introduction","sentence":"[ref] independently produced similar results.","intent_p":0.94,"contests_p":null}]},{"kind":"background","label":"Cites as background","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1907.04342","title":"The 21cm bispectrum during reionization: a tracer of the ionization topology","url":"/paper/1907.04342","section":"Evolution of the bispectrum sign","sentence":"In the earlier studies [ref] , this phenomenon has been associated with the nature of the non-Gaussianity in the 21-cm signal.","intent_p":0.82,"contests_p":null}]}],"unlabelled_sentences":4},"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/2012.11616"}}