{"arxiv_id":"1401.7986","incoming":{"papers":4,"sentences":7,"groups":[{"kind":"data_used","label":"Uses its data or values","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1405.0010","title":"Diversity Of Short Gamma-Ray Burst Afterglows From Compact Binary Mergers Hosting Pulsars","url":"/paper/1405.0010","section":"Introduction","sentence":"Compact binaries are expected to receive large “natal kicks\" due to asymmetries manifested by the mechanisms of NS/BH formation, resulting in mean velocities of $≈180$ km s$^-1$ for NS/NS binaries and $≈120$ km s$^-1$ for NS/BH binaries [ref] .","intent_p":0.87,"contests_p":null}]}],"unlabelled_sentences":6},"outgoing":{"papers":8,"sentences":14,"groups":[{"kind":"data_used","label":"Uses data or values from","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1407.6012","title":"The Relation Between SFR and Stellar Mass for Galaxies at 3.5 $\\le z\\le$ 6.5 in CANDELS","url":"/paper/1407.6012","section":"Instrumental, Geometrical, and Observational Biases","sentence":"In this calculation, we have assumed the metallicity of stars formed at a given redshift tracks the gas-phase metallicity in [ref] , and have adopted a dust optical depth of $τ=0.1$ (calibrated to match CANDELS observations of the stellar mass – F160W relation from $z=0.6$ to $z≈6$, for $M_∗< 10^10$; [ref] ).","intent_p":0.85,"contests_p":null}]},{"kind":"background","label":"Cites as background","papers":3,"sentences":3,"quotes":[{"arxiv_id":"1308.2964","title":"The Formation of Eccentric Compact Binary Inspirals and the Role of Gravitational Wave Emission in Binary-Single Stellar Encounters","url":"/paper/1308.2964","section":"Introduction","sentence":"Finally, mergers which statistically trace the globular cluster distribution around galaxies [ref] would result in very different interpretations for the offsets than if mergers traced the galactic potential [ref] .","intent_p":0.86,"contests_p":null},{"arxiv_id":"1311.2603","title":"Short-Duration Gamma-Ray Bursts","url":"/paper/1311.2603","section":"Introduction","sentence":"These include mergers of compact stellar remnants (i.e., combinations of neutron stars and black holes) via gravitational radiation, accretion-induced collapse of neutron stars, magnetar flaring, and magnetar formation through binary white dwarf mergers or white dwarf accretion-induced collapse [ref] .","intent_p":0.98,"contests_p":null},{"arxiv_id":"1302.4741","title":"The Host Galaxies of Long-Duration Gamma-Ray Bursts","url":"/paper/1302.4741","section":"Introduction","sentence":"Long gamma-ray bursts, with $T_90$ (the time for 90% of their photons to be received) greater than 2s, have been associated with Type Ic supernovae ( [ref] ; see also references in [ref] ).","intent_p":0.87,"contests_p":null}]}],"unlabelled_sentences":10},"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/1401.7986"}}