{"arxiv_id":"0908.3283","incoming":{"papers":27,"sentences":36,"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":2,"sentences":3,"quotes":[{"arxiv_id":"2104.04442","title":"Probing modified gravitational-wave propagation through tidal measurements of binary neutron star mergers","url":"/paper/2104.04442","section":"Degeneracy between luminosity distance and binary orientation","sentence":"We carry out a Monte Carlo simulation in which we consider $10^3$ BNSs at $z=1$ with the angle parameters randomly drawn from a uniformly distribution in $cosθ_s$, $ϕ_s$, $cosθ_L$ and $ϕ_L$ [ref] .","intent_p":0.89,"contests_p":null},{"arxiv_id":"1903.03909","title":"Equation-of-state insensitive relations after GW170817","url":"/paper/1903.03909","section":"Computation of statistical uncertainties","sentence":"(iii) Compute the combined population standard deviation $σ_N_A$, taking into account sources at varying redshifts as was done in Eq. (3) of Ref. [ref] : [equation] Here, we compute the populations' single-event uncertainties $σ_i^A(z)$ via the simple SNR scaling factor: [equation] where $ρ_i^A$ is the SNR of simulated event $i$ computed from Eq. [ref], and $ρ_GW170817^A$ and $σ_GW170817^A$ are the known SNRs and uncertainties of the GW170817 event from step (i).","intent_p":0.99,"contests_p":null}]},{"kind":"data_used","label":"Uses its data or values","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1710.04825","title":"Generalized framework for testing gravity with gravitational-wave propagation. I. Formulation","url":"/paper/1710.04825","section":"Graviton mass $μ$","sentence":"By observing $10^7M_⊙$ - $10^6M_⊙$ BH binary at 3 Gpc with LISA, one can impose a limit $m_g < 4.0×10^-26 eV$ [ref] , while observing $10^6M_⊙$ - $10^5M_⊙$ BH binary at 3 Gpc with DECIGO gives a limit $m_g < 3.7×10^-25 eV$ [ref] .","intent_p":0.85,"contests_p":null}]},{"kind":"comparison","label":"Compares with it","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1504.04300","title":"A New Method to Calculate the Stochastic Background of Gravitational Waves Generated by Compact Binaries","url":"/paper/1504.04300","section":"Results","sentence":"Fig. ([ref]) also shows for comparison the sensitivity curves for LISA, eLISA [ref] , BBO [ref] , DECIGO [ref] , ET [ref] and ALIGO [ref] .","intent_p":0.91,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":9,"sentences":9,"quotes":[{"arxiv_id":"1302.2198","title":"Tests of General Relativity and Alternative theories of gravity using Gravitational Wave observations","url":"/paper/1302.2198","section":"Possible bounds on Brans-Dicke theory","sentence":"This includes the effect of LISA noise PSD [ref] , effect of nonprecessing spins [ref] and effect of orbital eccentricity [ref] .","intent_p":0.92,"contests_p":null},{"arxiv_id":"1704.07561","title":"Constraining nonperturbative strong-field effects in scalar-tensor gravity by combining pulsar timing and laser-interferometer gravitational-wave detectors","url":"/paper/1704.07561","section":"Introduction","sentence":"In this paper, we investigate the extent to which pulsar timing and ground-based gravitational-wave (GW) observations can constrain these phenomena (space-based GW experiments [ref] are beyond the scope of this paper).","intent_p":0.93,"contests_p":null},{"arxiv_id":"1606.08462","title":"Graviton Mass Bounds","url":"/paper/1606.08462","section":"Introduction and Summary","sentence":"Some previous work has been done to categorize different bounds on the mass of the graviton in [ref] .","intent_p":0.86,"contests_p":null},{"arxiv_id":"2003.00286","title":"Probing Einstein-dilaton Gauss-Bonnet Gravity with the inspiral and ringdown of gravitational waves","url":"/paper/2003.00286","section":"Conclusion and Discussion","sentence":"This string-inspired theory predicts the scalarization of BHs [ref] , calling forth “fifth force\" interactions between orbiting BHs in a binary system and giving rise to scalar dipole radiation that predicts an increased rate of inspiral between them.","intent_p":0.94,"contests_p":null},{"arxiv_id":"1802.06977","title":"Multiband Gravitational-Wave Astronomy: Observing binary inspirals with a decihertz detector, B-DECIGO","url":"/paper/1802.06977","section":"Introduction","sentence":"Some previous studies of parameter estimation in the DECIGO mission can be found in Refs. [ref] .","intent_p":0.98,"contests_p":null}]}],"unlabelled_sentences":22},"outgoing":{"papers":3,"sentences":4,"groups":[{"kind":"comparison","label":"Compares with","papers":1,"sentences":1,"quotes":[{"arxiv_id":"0906.3602","title":"Bounding the mass of the graviton with gravitational waves: Effect of spin precessions in massive black hole binaries","url":"/paper/0906.3602","section":"Introduction","sentence":"Although we cannot directly compare these two results, it seems that our results are consistent with the ones obtained by Stavridis and Will [ref] .","intent_p":1.0,"contests_p":null}]}],"unlabelled_sentences":3},"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/0908.3283"}}