{"arxiv_id":"1908.10866","incoming":{"papers":5,"sentences":5,"groups":[{"kind":"contests","label":"Contests it","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2607.24531","title":"R-process nucleosynthesis from magnetar giant flares in neutron star--white dwarf mergers: A unified picture for peculiar long gamma-ray bursts","url":"/paper/2607.24531","section":"Introduction","sentence":"On the other hand, the tidally disrupted NS–WD merger model of [ref] and [ref] cannot account for the r-process heavy elements identified by spectroscopic features in GRB 230307A [ref] , since nucleosynthesis in a disk composed of WD debris is expected to be proton-rich and incapable of producing robust r-process yields, according to hydrodynamic simulations of NS–WD mergers [ref] .","intent_p":0.93,"contests_p":0.86}]},{"kind":"supports_this_paper","label":"Cites it as support","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1908.08056","title":"The Progenitors of Calcium-Strong Transients","url":"/paper/1908.08056","section":"Tidal disruptions of white dwarfs by neutron stars","sentence":"Much of the escaping material is made up of unburned matter entrained into the outflow, so C/O WD disruptions are unlikely to produce CaSTs due to the high O abundances in the ejecta [ref] .","intent_p":0.97,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1909.10810","title":"Detectability of neutron star -- white dwarf coalescences by eROSITA and ART-XC","url":"/paper/1909.10810","section":"Introduction","sentence":"In [ref] the authors studied the outcome of NS-WD mergers in some details from the point of view of electromagnetic counterparts (see also a recent e-print [ref] ).","intent_p":0.8,"contests_p":null},{"arxiv_id":"2002.11975","title":"Magnetars from Neutron Star--White Dwarf Mergers: Application to Fast Radio Bursts","url":"/paper/2002.11975","section":"Magnetars from NSWD Mergers","sentence":"The explosive outcomes of NSWD mergers have been explored in the literature [ref] , but the final remnants of these events have been little investigated [ref] .","intent_p":0.97,"contests_p":null}]}],"unlabelled_sentences":1},"outgoing":{"papers":3,"sentences":4,"groups":[{"kind":"data_used","label":"Uses data or values from","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1804.01538","title":"The demographics of neutron star - white dwarf mergers: rates, delay-time distributions and progenitors","url":"/paper/1804.01538","section":"Rate estimates","sentence":"By using the galactic merger rate of $1-2·10^-4 yr^-1$ from our population synthesis studies of NS-WD mergers [ref] , the galactic blue luminosity of $1.7·10^10L_B,⊙$ [ref] and the blue luminosity for the local universe $1.98·10^8 L_B,⊙/Mpc^3$ [ref] , we find that LSST will detect between $10$ and $70$ transients per year within its field of view.","intent_p":1.0,"contests_p":null},{"arxiv_id":"0912.0201","title":"LSST Science Book, Version 2.0","url":"/paper/0912.0201","section":"Rate estimates","sentence":"With the $5$-$σ$ magnitude limits for single-visit detections of $24.0$ and $24.7$ in I and R bands, respectively [ref] , LSST will be able to detect such transients within $15$ days past the peak up to a distance of $250 Mpc$.","intent_p":0.98,"contests_p":null}]},{"kind":"supports_this_paper","label":"Cites as support","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1804.01538","title":"The demographics of neutron star - white dwarf mergers: rates, delay-time distributions and progenitors","url":"/paper/1804.01538","section":"Discussion and summary","sentence":"As we show in [ref] and discuss above, the rates of NS-WD mergers could be sufficiently high as to be observed by LSST.","intent_p":0.96,"contests_p":null}]},{"kind":"background","label":"Cites as background","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2001.02947","title":"Type Ia Supernova Sub-classes and Progenitor Origin","url":"/paper/2001.02947","section":"Discussion and summary","sentence":"Over the last two decades several classes of fast-evolving SNe had been identified [ref] .","intent_p":0.9,"contests_p":null}]}],"unlabelled_sentences":0},"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/1908.10866"}}