dc.creator | Dominguez, Alfredo Eduardo | |
dc.creator | Ortega Larcher, Walter Emanuel | |
dc.creator | Aasi, J. | |
dc.creator | Abbott, B. P. | |
dc.creator | Abbott, R. | |
dc.creator | Abbott, T. | |
dc.creator | Abernathy, M. R. | |
dc.creator | Acernese, F. | |
dc.creator | Ackley, K. | |
dc.creator | Adams, C. | |
dc.creator | Adams, T. | |
dc.creator | Adams, T. | |
dc.creator | Addesso, P. | |
dc.creator | Adhikari, R. X. | |
dc.creator | Adya, V. | |
dc.creator | Affeldt, C. | |
dc.creator | Agathos, M. | |
dc.creator | Agatsuma, K. | |
dc.creator | Aggarwal, N. | |
dc.creator | Aguiar, O. D. | |
dc.creator | Ain, A. | |
dc.creator | Ajith, P. | |
dc.creator | Alemic, A. | |
dc.creator | Allen, B. | |
dc.creator | Allocca, A. | |
dc.creator | Amariutei, D. | |
dc.creator | Anderson, S. B. | |
dc.creator | Anderson, W. G. | |
dc.creator | Arai, K. | |
dc.creator | Araya, M. C. | |
dc.date.accessioned | 2021-04-29T18:54:22Z | |
dc.date.accessioned | 2022-10-15T03:00:42Z | |
dc.date.available | 2021-04-29T18:54:22Z | |
dc.date.available | 2022-10-15T03:00:42Z | |
dc.date.created | 2021-04-29T18:54:22Z | |
dc.date.issued | 2015-10 | |
dc.identifier | Dominguez, Alfredo Eduardo; Ortega Larcher, Walter Emanuel; Aasi, J.; Abbott, B. P.; Abbott, R.; et al.; Searches for continuous gravitational waves from nine young supernova remnants; IOP Publishing; Astrophysical Journal; 813; 1; 10-2015; 1-16 | |
dc.identifier | 0004-637X | |
dc.identifier | http://hdl.handle.net/11336/131065 | |
dc.identifier | CONICET Digital | |
dc.identifier | CONICET | |
dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/4337748 | |
dc.description.abstract | science data run. The targets were nine young supernova remnants not associated with pulsars; eight of the remnants are associated with non-pulsing suspected neutron stars. One target’s parameters are uncertain enough to warrant two searches, for a total of ten. Each search covered a broad band of frequencies and first and second frequency derivatives for a fixed sky direction. The searches coherently integrated data from the two LIGO interferometers over time spans from 5.3–25.3 days using the matched-filtering F-statistic. We found no credible gravitational-wave signals. We set 95% confidence upper limits as strong (low) as 4 × 10−25 on intrinsic strain, 2 × 10−7 on fiducial ellipticity, and 4 × 10−5 on r-mode amplitude. These beat the indirect limits from energy conservation and are within the range of theoretical predictions for neutron-star ellipticities and r-mode amplitudes. | |
dc.language | eng | |
dc.publisher | IOP Publishing | |
dc.relation | info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/813/1/39 | |
dc.relation | info:eu-repo/semantics/altIdentifier/doi/https://dx.doi.org/10.1088/0004-637X/813/1/39 | |
dc.rights | https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ | |
dc.rights | info:eu-repo/semantics/openAccess | |
dc.subject | Continuous Gravitational Waves | |
dc.subject | Search | |
dc.subject | Supernova Remanent | |
dc.title | Searches for continuous gravitational waves from nine young supernova remnants | |
dc.type | info:eu-repo/semantics/article | |
dc.type | info:ar-repo/semantics/artículo | |
dc.type | info:eu-repo/semantics/publishedVersion | |