Application of a Hough Search for Continuous Gravitational Waves on Data from the Fifth LIGO Science Run

• Published in: NASA Center for AeroSpace Information (CASI). Journal Articles
• Main Authors: Aasi, J, Abadie, J, Affeldt, C, Agathos, M, Aggarwal, N, Aguiar, O D, Ajith, P, Allen, B, Allocca, A, Ceron, E A, Amariutei, D, Anderson, R A, Abbott, B P, Blackburn, L, Camp, J B, Gehrels, N, Graff, P B, Kanner, J B, Abbott, R, Abbott, T, Abernathy, M R, Accadia, T, Adams, C, Adams, T, Adhikari, R X
• Format: Journal Article
• Language: English
• Published: Hampton NASA/Langley Research Center 21.04.2014
• Subjects: Gravitation; Gravitational waves; Hough transformation; Searching

We report on an all-sky search for periodic gravitational waves in the frequency range 50-1000 Hertz with the first derivative of frequency in the range −8.9 × 10(exp −10) Hertz per second to zero in two years of data collected during LIGO's fifth science run. Our results employ a Hough transform technique, introducing a chi(sup 2) test and analysis of coincidences between the signal levels in years 1 and 2 of observations that offers a significant improvement in the product of strain sensitivity with compute cycles per data sample compared to previously published searches. Since our search yields no surviving candidates, we present results taking the form of frequency dependent, 95% confidence upper limits on the strain amplitude h(sub 0). The most stringent upper limit from year 1 is 1.0 × 10(exp −24) in the 158.00-158.25 Hertz band. In year 2, the most stringent upper limit is 8.9 × 10(exp −25) in the 146.50-146.75 Hertz band. This improved detection pipeline, which is computationally efficient by at least two orders of magnitude better than our flagship Einstein@Home search, will be important for 'quicklook' searches in the Advanced LIGO and Virgo detector era.