{"arxiv_id":"1011.3076","incoming":{"papers":6,"sentences":14,"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1106.1066","title":"Implications of CoGeNT's New Results For Dark Matter","url":"/paper/1106.1066","section":"CoGeNT's Spectrum and Elastically Scattering Dark Matter","sentence":"In our calculations, we adopt the Helm form factor with parameters as described in our previous work [ref] .","intent_p":0.95,"contests_p":null},{"arxiv_id":"1110.5338","title":"Toward A Consistent Picture For CRESST, CoGeNT and DAMA","url":"/paper/1110.5338","section":"CoGeNT's Event Spectrum","sentence":"In our calculations, we adopt the Helm form factor with parameters as described in our previous work [ref] .","intent_p":0.89,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":3,"sentences":6,"quotes":[{"arxiv_id":"1106.1066","title":"Implications of CoGeNT's New Results For Dark Matter","url":"/paper/1106.1066","section":"Summary and Conclusions","sentence":"The possibility that the excess of low energy events as originally reported by the CoGeNT collaboration last year [ref] is the result of elastically scattering dark matter particles has received a great deal of attention [ref] .","intent_p":0.85,"contests_p":null},{"arxiv_id":"1102.0492","title":"The Galactic Center Region Gamma Ray Excess from A Supersymmetric Leptophilic Higgs Model","url":"/paper/1102.0492","section":"Introduction","sentence":"The astrophysical and particle physics implications of this finding are discussed in Refs. [ref] .","intent_p":0.81,"contests_p":null},{"arxiv_id":"1103.2377","title":"Constraining the Milky Way Dark Matter Density Profile with Gamma-Rays with Fermi-LAT","url":"/paper/1103.2377","section":"Conclusions","sentence":"Indeed, several approaches have been proposed to determine DM particle properties by using future indirect WIMP DM-induced signals of gamma-rays or neutrinos, direct detection searches, collider information or their combination [ref] .","intent_p":0.87,"contests_p":null}]}],"unlabelled_sentences":6},"outgoing":{"papers":17,"sentences":25,"groups":[{"kind":"data_used","label":"Uses data or values from","papers":5,"sentences":5,"quotes":[{"arxiv_id":"1002.1028","title":"New results from DAMA/LIBRA","url":"/paper/1002.1028","section":"Introduction","sentence":"According to the most recent DAMA/LIBRA results, which make use of over 1.17 ton-years of data, they observe a modulation with a significance of 8.9$σ$, and with a phase consistent with that predicted for elastically scattering dark matter [ref] .","intent_p":0.9,"contests_p":null},{"arxiv_id":"0712.1645","title":"New limits on spin-independent and spin-dependent couplings of low-mass WIMP dark matter with a germanium detector at a threshold of 220 eV","url":"/paper/0712.1645","section":"CoGeNT and Elastically Scattering Dark Matter","sentence":"Over the energy range of the CoGeNT signal (approximately 0.4 to 2 keVee, where keVee denotes keV electron equivalent), the quenching factors for germanium have been well measured [ref] and are described by $Q_Ge(E_Recoil=3 keV)=0.218$, and with the energy dependence predicted by the Lindhard theory (see Ref. [ref] ).","intent_p":0.94,"contests_p":null},{"arxiv_id":"1007.1005","title":"A Consistent Dark Matter Interpretation For CoGeNT and DAMA/LIBRA","url":"/paper/1007.1005","section":"CoGeNT and Elastically Scattering Dark Matter","sentence":"Over the energy range of the CoGeNT signal (approximately 0.4 to 2 keVee, where keVee denotes keV electron equivalent), the quenching factors for germanium have been well measured [ref] and are described by $Q_Ge(E_Recoil=3 keV)=0.218$, and with the energy dependence predicted by the Lindhard theory (see Ref. [ref] ).","intent_p":0.94,"contests_p":null},{"arxiv_id":"astro-ph/0611671","title":"The RAVE Survey: Constraining the Local Galactic Escape Speed","url":"/paper/astro-ph/0611671","section":"CoGeNT and Elastically Scattering Dark Matter","sentence":"We will consider values of $v_0$ over a range of 180 to 320 km/s and values of the galactic escape velocity between 460 and 640 km/s [ref] .","intent_p":0.85,"contests_p":null},{"arxiv_id":"hep-ph/0608035","title":"Model Independent Form Factors for Spin Independent Neutralino-Nucleon Scattering from Elastic Electron Scattering Data","url":"/paper/hep-ph/0608035","section":"CoGeNT and Elastically Scattering Dark Matter","sentence":"Here, $c ≈1.23 A^1/3 -0.60$ fm, $a ≈0.523$ fm, and $s ≈0.9$ fm have been determined by fits to nuclear physics data [ref] .","intent_p":0.98,"contests_p":null}]}],"unlabelled_sentences":20},"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/1011.3076"}}