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Interplay of spin-precession and higher harmonics in the parameter estimation of binary black holes
N V Krishnendu, Frank Ohme
Gravitational-wave (GW) signals from coalescing compact binaries carry enormous information about the source dynamics and are an excellent tool to probe unknown astrophysics and fu…
Black-hole kicks: a tool to measure the accuracy of gravitational-wave models
Angela Borchers, Frank Ohme
Asymmetric binary systems radiate linear momentum through gravitational waves, leading to the recoil of the merger remnant. Black-hole kicks have attracted much attention because o…
Training Strategies for Deep Learning Gravitational-Wave Searches
Marlin B. Schäfer, Ondřej Zelenka, Alexander H. Nitz +2
Compact binary systems emit gravitational radiation which is potentially detectable by current Earth bound detectors. Extracting these signals from the instruments' background nois…
Numerical Inside View of Hypermassive Remnant Models for GW170817
Wolfgang Kastaun, Frank Ohme
The first multimessenger observation attributed to a merging neutron star binary provided an enormous amount of observational data. Unlocking the full potential of this data requir…
Adding eccentricity to quasicircular binary-black-hole waveform models
Yoshinta Setyawati, Frank Ohme
The detection of gravitational-wave signals from coalescing eccentric binary black holes would yield unprecedented information about the formation and evolution of compact binaries…