1.2k citations · 14.2k across the 129 of their papers we have counts for
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gr-qc2010★ 1.1k cited
Sensitivity Studies for Third-Generation Gravitational Wave Observatories
S. Hild, M. Abernathy, F. Acernese +136
Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope, a…
astro-ph.CO2010★ 23 cited
Gravitational waves from intermediate-mass black holes in young clusters
M. Mapelli, C. Huwyler, L. Mayer +2
Massive young clusters (YCs) are expected to host intermediate-mass black holes (IMBHs) born via runaway collapse. These IMBHs are likely in binaries and can undergo mergers with o…
astro-ph.CO2010★ 154 cited
Measuring the parameters of massive black hole binary systems with Pulsar Timing Array observations of gravitational waves
Alberto Sesana, Alberto Vecchio
The observation of massive black hole binaries (MBHBs) with Pulsar Timing Arrays (PTAs) is one of the goals of gravitational wave astronomy in the coming years. Massive (>10^8 sola…