{"arxiv_id":"1305.2124","incoming":{"papers":18,"sentences":27,"groups":[{"kind":"contests","label":"Contests it","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1306.5725","title":"Dark Matter and Pulsar Model Constraints from Galactic Center Fermi-LAT Gamma Ray Observations","url":"/paper/1306.5725","section":"Dark Matter and Pulsars Maps","sentence":"It has recently been pointed out that there are discrepancies [ref] between the gamma ray spectra calculated with (Fortran version) and [ref] (C++ version), that software analysis using interpolating functions can overestimate the energy cut-off of the gamma-ray spectra [ref] , and that not considering electroweak corrections can also create deviations between predicted DM annihilitions spectra [ref] .","intent_p":0.36,"contests_p":0.72}]},{"kind":"extends","label":"Builds on it","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1907.02488","title":"Effect of polarisation and choice of event generator on spectra from dark matter annihilations","url":"/paper/1907.02488","section":"Introduction","sentence":"[ref] , but we expand upon these works by considering a broader range of yield particles beyond photons, as well as polarised final states.","intent_p":1.0,"contests_p":null},{"arxiv_id":"1404.2067","title":"Gamma-ray and neutrino fluxes from Heavy Dark Matter in the Galactic Center","url":"/paper/1404.2067","section":"Monte Carlo uncertainty on photons flux","sentence":"Here, we focused on DM particle mass of $1$ TeV (see [ref] for the same analysis with $100 GeV$ DM annihilating into $W^+W^-$, $bb̅$, $τ^+τ^-$ or $500$ GeV DM mass in the case of $tt̅$ and further details on $1$ TeV DM mass for more channels).","intent_p":0.85,"contests_p":null}]},{"kind":"data_used","label":"Uses its data or values","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1404.2067","title":"Gamma-ray and neutrino fluxes from Heavy Dark Matter in the Galactic Center","url":"/paper/1404.2067","section":"Monte Carlo uncertainty on photons flux","sentence":"The multiplicity behavior is well approximated by the following power law relation with the DM mass: [equation] The $a$ and $b$ coefficients are given in [ref] .","intent_p":0.93,"contests_p":null}]},{"kind":"comparison","label":"Compares with it","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2307.06823","title":"Multi-TeV dark matter density in the inner Milky Way halo: spectral and dynamical constraints","url":"/paper/2307.06823","section":"VIR","sentence":"Minor differences may be explained by: 1) newly updated data by the H.E.S.S. collaboration in the region [ref] ; 2) the inclusion of the DRAGON background model instead of the simple power-law [ref] ; 3) the use of a different Monte Carlo event generator software to model the gamma-ray annihilation flux [ref] .","intent_p":0.87,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1502.05703","title":"A description of the Galactic Center excess in the Minimal Supersymmetric Standard Model","url":"/paper/1502.05703","section":"Uncertainties in the predicted photon spectrum","sentence":"We discuss here briefly sources for uncertainties in the predicted photon spectrum (see [ref] for an earlier assessment), and leave a more detailed study to a future publication.","intent_p":0.93,"contests_p":null}]}],"unlabelled_sentences":21},"outgoing":{"papers":5,"sentences":7,"groups":[{"kind":"background","label":"Cites as background","papers":3,"sentences":3,"quotes":[{"arxiv_id":"1304.6677","title":"Monte Carlo Event Generators","url":"/paper/1304.6677","section":"Monte Carlo Parton Shower","sentence":"Therefore, let us study separately the technicalities of each part as follows (read [ref] for further details):","intent_p":0.96,"contests_p":null},{"arxiv_id":"1109.5027","title":"Dark matter with photons","url":"/paper/1109.5027","section":"Introduction","sentence":"On the other hand, local DM can be detected in a direct or indirect way [ref] .","intent_p":0.94,"contests_p":null},{"arxiv_id":"1302.6871","title":"Spectral Study of the HESS J1745-290 Gamma-Ray Source as Dark Matter Signal","url":"/paper/1302.6871","section":"Introduction","sentence":"On the other hand, local DM can be detected in a direct or indirect way [ref] .","intent_p":0.94,"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/1305.2124"}}