{"arxiv_id":"1701.02726","incoming":{"papers":23,"sentences":25,"groups":[{"kind":"data_used","label":"Uses its data or values","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2312.00672","title":"What Makes A Discovery","url":"/paper/2312.00672","section":"The Application of the Galactic Center Gamma-Ray Excess","sentence":"Given that no direct detection signals have appeared [ref] , no pulsars have been found near the Galactic Center [ref] , and far too few low-mass X-ray binaries have been found in the Inner Galaxy [ref] , we can use this information to calculate new posterior probabilities, obtaining $P(T_DM|D) ∼0.65$ and $P(T_pulsars|D) ∼0.35$.","intent_p":0.94,"contests_p":null}]},{"kind":"supports_this_paper","label":"Cites it as support","papers":2,"sentences":2,"quotes":[{"arxiv_id":"2006.00513","title":"Indirect Detection of Dark Matter in the Galaxy","url":"/paper/2006.00513","section":"GeV Excess","sentence":"Now, while pulsars are a good candidate for the excess, we still haven't seen any of the pulsars that are contributing GCE (if they are), which is argued to be surprising given the number of low-mass X-ray binaries observed in the GC [ref] .","intent_p":0.96,"contests_p":null},{"arxiv_id":"2404.10039","title":"Neutrino and Gamma-Ray Signatures of Inelastic Dark Matter Annihilating outside Neutron Stars","url":"/paper/2404.10039","section":"Neutron Star Structure","sentence":"For instance, if a substantial population of these objects were present, it would imply a notable increase in low-mass X-ray binaries compared to observed numbers [ref] .","intent_p":0.96,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":4,"sentences":4,"quotes":[{"arxiv_id":"1803.08046","title":"Millisecond Pulsars, TeV Halos, and Implications For The Galactic Center Gamma-Ray Excess","url":"/paper/1803.08046","section":"TeV Halos and the Galactic Center GeV Excess","sentence":"At this time, the leading astrophysical interpretation of this observation is that it is generated by a large population of unresolved and centrally located millisecond pulsars [ref] .","intent_p":0.89,"contests_p":null},{"arxiv_id":"1906.02175","title":"Pseudo-Goldstone dark matter confronts cosmic ray and collider anomalies","url":"/paper/1906.02175","section":"Introduction","sentence":"A leading alternative astrophysical explanation is that the excess comes from an unresolved population of millisecond pulsars or other astrophysical sources [ref] , although arguments against the pulsar hypothesis have been presented [ref] .","intent_p":0.9,"contests_p":null},{"arxiv_id":"2301.10239","title":"Probing the pulsar explanation of the Galactic-Center GeV excess using continuous gravitational-wave searches","url":"/paper/2301.10239","section":"Introduction","sentence":"The general theme behind these studies is to devise a luminosity function to fit the observed , based on minimal assumptions [ref] or astrophysics, e.g. assuming luminosity functions identical to those from known in globular clusters [ref] , asserting that accretion-induced collapse is responsible for creating a population [ref] , or allowing emissions from low-mass X-ray binaries to compose the [ref] .","intent_p":0.93,"contests_p":null},{"arxiv_id":"2010.15129","title":"A Closer Look at CP-Violating Higgs Portal Dark Matter as a Candidate for the GCE","url":"/paper/2010.15129","section":"Introduction","sentence":"In recent years, the debate surrounding the origin of the GCE has intensified [ref] .","intent_p":0.92,"contests_p":null}]}],"unlabelled_sentences":18},"outgoing":{"papers":83,"sentences":108,"groups":[{"kind":"method_or_tool","label":"Uses the method or tool of","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1407.5583","title":"A New Determination of the Spectra and Luminosity Function of Gamma-Ray Millisecond Pulsars","url":"/paper/1407.5583","section":"Gamma-Ray Emission and LMXBs in Globular Clusters","sentence":"In analyzing the publicly available Fermi-LAT data, we have followed the same procedure as described in Ref. [ref] , except here we have adopted a MSP-like spectral shape [ref] :","intent_p":0.98,"contests_p":null},{"arxiv_id":"1606.09250","title":"The Gamma-Ray Pulsar Population of Globular Clusters: Implications for the GeV Excess","url":"/paper/1606.09250","section":"Gamma-Ray Emission and LMXBs in Globular Clusters","sentence":"In analyzing the publicly available Fermi-LAT data, we have followed the same procedure as described in Ref. 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[ref] , which contains all such LMXBs found in globular clusters, published as of 2014.","intent_p":0.95,"contests_p":null},{"arxiv_id":"1206.2395","title":"X-ray Binary Evolution Across Cosmic Time","url":"/paper/1206.2395","section":"Luminosity Function Evolution?","sentence":"For example, Ref. [ref] calculates that the X-ray emissivity of a given LMXB remains constant for about 1.5 Gyrs after formation, and then declines with an e-folding timescale of roughly 1.5 Gyrs (see also, Ref. [ref] ).","intent_p":0.86,"contests_p":null},{"arxiv_id":"astro-ph/0612058","title":"Low-Mass X-ray Binaries and Globular Clusters in Early-Type Galaxies. I. Chandra Observations","url":"/paper/astro-ph/0612058","section":"Luminosity Function Evolution?","sentence":"For example, Ref. [ref] calculates that the X-ray emissivity of a given LMXB remains constant for about 1.5 Gyrs after formation, and then declines with an e-folding timescale of roughly 1.5 Gyrs (see also, Ref. 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[ref] ), astrophysical origins for this emission have also been proposed.","intent_p":0.97,"contests_p":null},{"arxiv_id":"1401.6458","title":"Extended gamma-ray emission from Coy Dark Matter","url":"/paper/1401.6458","section":"Introduction","sentence":"Although dark matter interpretations of this signal have generated a great deal of interest (see, for example, Refs. [ref] ), astrophysical origins for this emission have also been proposed.","intent_p":0.97,"contests_p":null},{"arxiv_id":"1403.5027","title":"The Effective Hooperon","url":"/paper/1403.5027","section":"Introduction","sentence":"Although dark matter interpretations of this signal have generated a great deal of interest (see, for example, Refs. [ref] ), astrophysical origins for this emission have also been proposed.","intent_p":0.97,"contests_p":null},{"arxiv_id":"1404.0022","title":"Simplified Dark Matter Models for the Galactic Center Gamma-Ray Excess","url":"/paper/1404.0022","section":"Introduction","sentence":"Although dark matter interpretations of this signal have generated a great deal of interest (see, for example, Refs. [ref] ), astrophysical origins for this emission have also been proposed.","intent_p":0.97,"contests_p":null},{"arxiv_id":"1404.1373","title":"Flavored Dark Matter and the Galactic Center Gamma-Ray Excess","url":"/paper/1404.1373","section":"Introduction","sentence":"Although dark matter interpretations of this signal have generated a great deal of interest (see, for example, Refs. [ref] ), astrophysical origins for this emission have also been proposed.","intent_p":0.97,"contests_p":null}]}],"unlabelled_sentences":72},"claims":[{"relation":"contradicts","label":"States a conflicting result","papers":[{"arxiv_id":"1404.2318","url":"/paper/1404.2318","title":"Millisecond pulsar interpretation of the Galactic center gamma-ray excess","main_claim":"We conclude that the MSP model can explain the Galactic center $\\gamma$-ray excess self-consistently, satisfying all the current observational constraints.","p":0.95}]}],"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/1701.02726"}}