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{"references": ["S. Klimenko et al., Coherent method for detection of gravitational wave bursts, Class. Quantum Grav. 25, 114029 (2008)", "S. Klimenko et al., Localization of gravitational wave sources with networks of advanced detectors, Phys. Rev. D 83, 102001 (2011)", "S. Klimenko, G. Vedovato, M. Drago, F. Salemi, V. Tiwari, G.A. Prodi, C. Lazzaro, K. Ackley, S. Tiwari, C.F. Da Silva, and G. Mitselmakher, Method for detection and reconstruction of gravitational wave transients with networks of advanced detectors, Phys. Rev. D 93, 042004 (2016)"]}
This release marks the first public version of cWB ( cWB-6.3.0 ): it is fully compatible (i.e. in terms of results) with the version ( wat-6.2.6 ) used for the analysis of the LIGO and Virgo data collected during the Second Observational run O2. While all search algorithms are substantially unchanged, the whole pipeline insfrastructure has been upgraded and now uses ROOT6 instead of ROOT5. See https://gwburst.gitlab.io/ for more details. Public git repository: https://gitlab.com/gwburst/public/library
search pipeline, gravitational-waves, burst
search pipeline, gravitational-waves, burst
| 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). | 6 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Top 10% | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| 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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