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Gravitational-wave posterior sample data injected with the waveform model IMRPhenomDNRTv2 (PhenDNRTv2) and recovered with the models: IMRPhenomDNRT (PhenDNRT), PhenDNRTv2, SEOB-NRv4ROMNRTidalv2 (SEOBNRTv2) and TaylorF2.
High Energy Astrophysical Phenomena (astro-ph.HE), Nuclear Theory (nucl-th), Physics and Astronomy (miscellaneous), Nuclear Theory, ddc:530, ddc:520, Institut für Physik und Astronomie, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics - High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena (astro-ph.HE), Nuclear Theory (nucl-th), Physics and Astronomy (miscellaneous), Nuclear Theory, ddc:530, ddc:520, Institut für Physik und Astronomie, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics - High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology
| 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). | 18 | |
| 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. | Top 10% |
| views | 4 |

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