Document Type
Article
Publication Date
1-5-2009
Abstract
A search for periodic gravitational waves, from sources such as isolated rapidly spinning neutron stars, was carried out using 510 h of data from the fourth LIGO science run (S4). The search was for quasimonochromatic waves in the frequency range from 50 to 1500 Hz, with a linear frequency drift ḟ (measured at the solar system barycenter) in the range -f/τ<ḟ
Journal Title
Physical Review D - Particles, Fields, Gravitation and Cosmology
Volume
79
Issue
2
DOI
https://doi.org/10.1103/PhysRevD.79.022001
First Department
Physics
Recommended Citation
Abbott, B.; Abbott, R.; Adhikari, R.; Ajith, P.; Allen, B.; Allen, G.; Amin, R.; Anderson, D. P.; Anderson, S. B.; Anderson, W. G.; Arain, M. A.; Araya, M.; Armandula, H.; Armor, P.; Aso, Y.; Aston, S.; Aufmuth, P.; Aulbert, C.; Babak, S.; Ballmer, S.; Bantilan, H.; Barish, B. C.; Barker, C.; Barker, D.; Barr, B.; Barriga, P.; Barton, M. A.; Bastarrika, M.; Bayer, K.; Betzwieser, J.; Beyersdorf, P. T.; and Summerscales, Tiffany Z., "Einstein@Home Search for Periodic Gravitational Waves in LIGO S4 Data" (2009). Faculty Publications. 1999.
https://digitalcommons.andrews.edu/pubs/1999
Acknowledgements
Retrieved March 8, 2021 from https://journals.aps.org/prd/abstract/10.1103/PhysRevD.79.022001
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