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This work was supported by the NSF grant OAC-1841480. S.S. is supported by the Eberly Research Funds of Penn State, The Pennsylvania State University, University Park, Pennsylvania. D.M. acknowledges the support of NSF PHY-1454389, ACI-1642391, and OAC-1841480. S.R.M thanks the LSSTC Data Science Fellowship Program, which is funded by LSSTC, NSF Cybertraining Grant #1829740, the Brinson Foundation, and the Moore Foundation; his participation in the program has benefited this work. B.S.S. is supported in part by NSF Grant No. PHY-1836779 and AST-1708146. Computations for this research were performed on the Pennsylvania State University's Institute for Computational and Data Sciences Advanced CyberInfrastructure (ICDS-ACI). We also thank the LIGO Laboratory for use of its computing facility to make this work possible.
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binary neutron stars, multi-messenger astronomy, gravitational-waves
binary neutron stars, multi-messenger astronomy, gravitational-waves
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 1 | |
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| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
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