Multimessenger astronomy with a kHz-band gravitational-wave observatory

@article{Sarin2021MultimessengerAW,
  title={Multimessenger astronomy with a kHz-band gravitational-wave observatory},
  author={Nikhil Sarin and Paul D. Lasky},
  journal={Publications of the Astronomical Society of Australia},
  year={2021},
  volume={39}
}
  • N. SarinP. Lasky
  • Published 21 October 2021
  • Physics
  • Publications of the Astronomical Society of Australia
Abstract Proposed next-generation networks of gravitational-wave observatories include dedicated kilohertz instruments that target neutron star science, such as the proposed Neutron Star Extreme Matter Observatory, NEMO. The original proposal for NEMO highlighted the need for it to exist in a network of gravitational-wave observatories to ensure detection confidence and sky localisation of sources. We show that NEMO-like observatories have significant utility on their own as coincident… 
1 Citations

Analytic models of the spectral properties of gravitational waves from neutron star merger remnants

Theodoros Soultanis, 2, ∗ Andreas Bauswein, 4 and Nikolaos Stergioulas Heidelberg Institute for Theoretical Studies, Schloss-Wolfsbrunnenweg 35, 69118 Heidelberg, Germany Max-Planck-Institut für

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