Results from the First All-Sky Search for Continuous Gravitational Waves from Small-Ellipticity Sources

Apr 17, 2020
6 pages
Published in:
  • Phys.Rev.Lett. 125 (2020) 17, 171101
  • Published: Oct 23, 2020
e-Print:

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Abstract: (APS)
We present the results of an all-sky search for continuous gravitational-wave signals with frequencies in the 500–1700 Hz range targeting neutron stars with ellipticity of 10-8. The search is done on LIGO O2 data using the Falcon analysis pipeline. The results presented here double the sensitivity over any other result on the same data [B. P. Abbott (LIGO Scientific Collaboration and Virgo Collaboration), Phys. Rev. D 100, 024004 (2019)PRVDAQ2470-001010.1103/PhysRevD.100.024004, C. Palomba , Phys. Rev. Lett. 123, 171101 (2019)PRLTAO0031-900710.1103/PhysRevLett.123.171101]. The search is capable of detecting low-ellipticity sources up to 170 pc. We establish strict upper limits which hold for worst-case signal parameters. We list outliers uncovered by the search, including several which we cannot associate with any known instrumental cause.
Note:
  • This is a combined version of the article published by PRL. It includes outlier table and hardware injection table found in supplemental materials of PRL version
  • Gravitation and Astrophysics
  • gravitational radiation detector
  • gravitational radiation: emission
  • gravitational radiation: direct detection
  • data analysis method
  • statistical analysis
  • LIGO
  • neutron star
  • detector: sensitivity