Scientific note

Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries

We present IMRPhenomXHM NSBH and SEOBNRv5HM ROM NRTidalv3 NSBH, the first two frequency-domain models for gravitational-wave signals from quasi-circular, aligned-spin neutron star--black hole (NSBH) binaries including higher-order modes...