We present the results of a search for long-duration gravitational wave transients in the data of the LIGO Hanford and LIGO Livingston second generation detectors between September 2015 and January 2016, with a total observational time of 49 d. The search targets gravitational wave transients of 10-500 s duration in a frequency band of 24-2048 Hz, with minimal assumptions about the signal waveform, polarization, source direction, or time of occurrence. No significant events were observed. As a result we set 90% confidence upper limits on the rate of long-duration gravitational wave transients for different types of gravitational wave signals. We also show that the search is sensitive to sources in the Galaxy emitting at least similar to 10-8 M(circle dot)c(2) in gravitational waves.

All-sky search for long-duration gravitational wave transients in the first Advanced LIGO observing run / Abbott, B.p., Abbott, R., Abbott, T.d., Abernathy, M.r., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R.x., Adya, V.b., Affeldt, C., Agathos, M., Agatsuma, K., Aggarwal, N., Aguiar, O.d., Aiello, L., Ain, A., Ajith, P., Allen, B., et al.. - In: CLASSICAL AND QUANTUM GRAVITY. - ISSN 0264-9381. - 35:6(2018), p. 065009. [10.1088/1361-6382/aaab76]

All-sky search for long-duration gravitational wave transients in the first Advanced LIGO observing run

Astone, P;Di Pace, S;Di Palma, I;Drago, M;Frasca, S;Leaci, P;Majorana, E;Mangano, V;Mezzani, F;Naticchioni, L;Palomba, C;Pannarale, F;Rapagnani, P;Ricci, F;Salemi, F;Di Giovanni, M
2018

Abstract

We present the results of a search for long-duration gravitational wave transients in the data of the LIGO Hanford and LIGO Livingston second generation detectors between September 2015 and January 2016, with a total observational time of 49 d. The search targets gravitational wave transients of 10-500 s duration in a frequency band of 24-2048 Hz, with minimal assumptions about the signal waveform, polarization, source direction, or time of occurrence. No significant events were observed. As a result we set 90% confidence upper limits on the rate of long-duration gravitational wave transients for different types of gravitational wave signals. We also show that the search is sensitive to sources in the Galaxy emitting at least similar to 10-8 M(circle dot)c(2) in gravitational waves.
2018
LIGO-Virgo; gravitational waves; long duration transient
01 Pubblicazione su rivista::01a Articolo in rivista
All-sky search for long-duration gravitational wave transients in the first Advanced LIGO observing run / Abbott, B.p., Abbott, R., Abbott, T.d., Abernathy, M.r., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R.x., Adya, V.b., Affeldt, C., Agathos, M., Agatsuma, K., Aggarwal, N., Aguiar, O.d., Aiello, L., Ain, A., Ajith, P., Allen, B., et al.. - In: CLASSICAL AND QUANTUM GRAVITY. - ISSN 0264-9381. - 35:6(2018), p. 065009. [10.1088/1361-6382/aaab76]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1655845
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