Simulation of HLVK Configuration for O5 and O6 Observation Runs: Gravitational Wave Detection Rates, Skymaps, and Multimessenger Parameters (November 2024 edition)
We conducted a simulation of the HLVK configuration for the upcoming O5 and O6 observing runs, estimating the expected gravitational wave (GW) detection rates based on a signal-to-noise (S/N) threshold of 10. This dataset includes skymap files and essential parameters for multimessenger studies. Add...
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| Format: | Dataset |
| Sprache: | eng |
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| Zusammenfassung: | We conducted a simulation of the HLVK configuration for the upcoming O5 and O6 observing runs, estimating the expected gravitational wave (GW) detection rates based on a signal-to-noise (S/N) threshold of 10. This dataset includes skymap files and essential parameters for multimessenger studies. Additionally, a Python script is provided to facilitate the separation of BNS, BBH, and NSBH events based on mass, with a default recommendation of setting neutron star (NS) mass to |
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| DOI: | 10.5281/zenodo.14142969 |