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:
- 2004.08334 [gr-qc]
View in:
Citations per year
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
References(39)
Figures(5)
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- [9]
- [10]
- [11]
- [12]
- [13]
- [14]
- [15]
- [16]
- [17]
- [18]
- [19]
- [20]
- [22]
- [22]
- [23]
- [24]
- [25]