Searches for continuous gravitational waves from nine young supernova remnants
- Autores
- Dominguez, Alfredo Eduardo; Ortega Larcher, Walter Emanuel; Aasi, J.; Abbott, B. P.; Abbott, R.; Abbott, T.; Abernathy, M. R.; Acernese, F.; Ackley, K.; Adams, C.; Adams, T.; Adams, T.; Addesso, P.; Adhikari, R. X.; Adya, V.; Affeldt, C.; Agathos, M.; Agatsuma, K.; Aggarwal, N.; Aguiar, O. D.; Ain, A.; Ajith, P.; Alemic, A.; Allen, B.; Allocca, A.; Amariutei, D.; Anderson, S. B.; Anderson, W. G.; Arai, K.; Araya, M. C.
- Año de publicación
- 2015
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- 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.
Fil: Dominguez, Alfredo Eduardo. Ministerio de Defensa. Fuerza Aerea Argentina; Argentina
Fil: Ortega Larcher, Walter Emanuel. Consejo Nacional de Investigaciones Científicas y Técnicas. Unidad de Investigación y Desarrollo Estrategico Para la Defensa. Subsede Instituto Universitario Aeronautico | Ministerio de Defensa. Unidad de Investigación y Desarrollo Estrategico Para la Defensa. Subsede Instituto Universitario Aeronautico; Argentina
Fil: Aasi, J.. California Institute of Technology; Estados Unidos
Fil: Abbott, B. P.. California Institute of Technology; Estados Unidos
Fil: Abbott, R.. California Institute of Technology; Estados Unidos
Fil: Abbott, T.. State University of Louisiana; Estados Unidos
Fil: Abernathy, M. R.. California Institute of Technology; Estados Unidos
Fil: Acernese, F.. Universita di Salerno; Italia. Istituto Nazionale Di Fisica Nucleare; Italia
Fil: Ackley, K.. University of Florida; Estados Unidos
Fil: Adams, C.. Livingston Observatory; Estados Unidos
Fil: Adams, T.. Cardiff University; Reino Unido. Centre National de la Recherche Scientifique; Francia. Université de Savoie; Francia
Fil: Adams, T.. Centre National de la Recherche Scientifique; Francia. Université de Savoie; Francia
Fil: Addesso, P.. University of Sannio at Benevento; Italia. Istituto Nazionale Di Fisica Nucleare; Italia
Fil: Adhikari, R. X.. California Institute of Technology; Estados Unidos
Fil: Adya, V.. Max Planck Institut für Gravitationsphysik; Alemania
Fil: Affeldt, C.. Max Planck Institut für Gravitationsphysik; Alemania
Fil: Agathos, M.. Nikhef; Países Bajos
Fil: Agatsuma, K.. Nikhef; Países Bajos
Fil: Aggarwal, N.. Massachusetts Institute of Technology; Estados Unidos
Fil: Aguiar, O. D.. Centro de Previsao de Tempo e Estudos Climáticos. Instituto Nacional de Pesquisas Espaciais; Brasil
Fil: Ain, A.. Inter-University Centre for Astronomy and Astrophysics; India
Fil: Ajith, P.. Tata Institute of Fundamental Research; India
Fil: Alemic, A.. Syracuse University; Estados Unidos
Fil: Allen, B.. University of Wisconsin-Milwaukee; Estados Unidos. Max-Planck-Institut für Gravitationsphysik; Alemania
Fil: Allocca, A.. Università degli Studi di Siena; Italia. Istituto Nazionale Di Fisica Nucleare; Italia
Fil: Amariutei, D.. University of Florida; Estados Unidos
Fil: Anderson, S. B.. California Institute of Technology; Estados Unidos
Fil: Anderson, W. G.. University of Wisconsin–Milwaukee; Estados Unidos
Fil: Arai, K.. California Institute of Technology; Estados Unidos
Fil: Araya, M. C.. California Institute of Technology; Estados Unidos - Materia
-
Continuous Gravitational Waves
Search
Supernova Remanent - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/131065
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Searches for continuous gravitational waves from nine young supernova remnantsDominguez, Alfredo EduardoOrtega Larcher, Walter EmanuelAasi, J.Abbott, B. P.Abbott, R.Abbott, T.Abernathy, M. R.Acernese, F.Ackley, K.Adams, C.Adams, T.Adams, T.Addesso, P.Adhikari, R. X.Adya, V.Affeldt, C.Agathos, M.Agatsuma, K.Aggarwal, N.Aguiar, O. D.Ain, A.Ajith, P.Alemic, A.Allen, B.Allocca, A.Amariutei, D.Anderson, S. B.Anderson, W. G.Arai, K.Araya, M. C.Continuous Gravitational WavesSearchSupernova Remanenthttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1science 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.Fil: Dominguez, Alfredo Eduardo. Ministerio de Defensa. Fuerza Aerea Argentina; ArgentinaFil: Ortega Larcher, Walter Emanuel. Consejo Nacional de Investigaciones Científicas y Técnicas. Unidad de Investigación y Desarrollo Estrategico Para la Defensa. Subsede Instituto Universitario Aeronautico | Ministerio de Defensa. Unidad de Investigación y Desarrollo Estrategico Para la Defensa. Subsede Instituto Universitario Aeronautico; ArgentinaFil: Aasi, J.. California Institute of Technology; Estados UnidosFil: Abbott, B. P.. California Institute of Technology; Estados UnidosFil: Abbott, R.. California Institute of Technology; Estados UnidosFil: Abbott, T.. State University of Louisiana; Estados UnidosFil: Abernathy, M. R.. California Institute of Technology; Estados UnidosFil: Acernese, F.. Universita di Salerno; Italia. Istituto Nazionale Di Fisica Nucleare; ItaliaFil: Ackley, K.. University of Florida; Estados UnidosFil: Adams, C.. Livingston Observatory; Estados UnidosFil: Adams, T.. Cardiff University; Reino Unido. Centre National de la Recherche Scientifique; Francia. Université de Savoie; FranciaFil: Adams, T.. Centre National de la Recherche Scientifique; Francia. Université de Savoie; FranciaFil: Addesso, P.. University of Sannio at Benevento; Italia. Istituto Nazionale Di Fisica Nucleare; ItaliaFil: Adhikari, R. X.. California Institute of Technology; Estados UnidosFil: Adya, V.. Max Planck Institut für Gravitationsphysik; AlemaniaFil: Affeldt, C.. Max Planck Institut für Gravitationsphysik; AlemaniaFil: Agathos, M.. Nikhef; Países BajosFil: Agatsuma, K.. Nikhef; Países BajosFil: Aggarwal, N.. Massachusetts Institute of Technology; Estados UnidosFil: Aguiar, O. D.. Centro de Previsao de Tempo e Estudos Climáticos. Instituto Nacional de Pesquisas Espaciais; BrasilFil: Ain, A.. Inter-University Centre for Astronomy and Astrophysics; IndiaFil: Ajith, P.. Tata Institute of Fundamental Research; IndiaFil: Alemic, A.. Syracuse University; Estados UnidosFil: Allen, B.. University of Wisconsin-Milwaukee; Estados Unidos. Max-Planck-Institut für Gravitationsphysik; AlemaniaFil: Allocca, A.. Università degli Studi di Siena; Italia. Istituto Nazionale Di Fisica Nucleare; ItaliaFil: Amariutei, D.. University of Florida; Estados UnidosFil: Anderson, S. B.. California Institute of Technology; Estados UnidosFil: Anderson, W. G.. University of Wisconsin–Milwaukee; Estados UnidosFil: Arai, K.. California Institute of Technology; Estados UnidosFil: Araya, M. C.. California Institute of Technology; Estados UnidosIOP Publishing2015-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/131065Dominguez, 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; 1-160004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/813/1/39info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/813/1/39info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:48:23Zoai:ri.conicet.gov.ar:11336/131065instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:48:24.077CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Searches for continuous gravitational waves from nine young supernova remnants |
title |
Searches for continuous gravitational waves from nine young supernova remnants |
spellingShingle |
Searches for continuous gravitational waves from nine young supernova remnants Dominguez, Alfredo Eduardo Continuous Gravitational Waves Search Supernova Remanent |
title_short |
Searches for continuous gravitational waves from nine young supernova remnants |
title_full |
Searches for continuous gravitational waves from nine young supernova remnants |
title_fullStr |
Searches for continuous gravitational waves from nine young supernova remnants |
title_full_unstemmed |
Searches for continuous gravitational waves from nine young supernova remnants |
title_sort |
Searches for continuous gravitational waves from nine young supernova remnants |
dc.creator.none.fl_str_mv |
Dominguez, Alfredo Eduardo Ortega Larcher, Walter Emanuel Aasi, J. Abbott, B. P. Abbott, R. Abbott, T. Abernathy, M. R. Acernese, F. Ackley, K. Adams, C. Adams, T. Adams, T. Addesso, P. Adhikari, R. X. Adya, V. Affeldt, C. Agathos, M. Agatsuma, K. Aggarwal, N. Aguiar, O. D. Ain, A. Ajith, P. Alemic, A. Allen, B. Allocca, A. Amariutei, D. Anderson, S. B. Anderson, W. G. Arai, K. Araya, M. C. |
author |
Dominguez, Alfredo Eduardo |
author_facet |
Dominguez, Alfredo Eduardo Ortega Larcher, Walter Emanuel Aasi, J. Abbott, B. P. Abbott, R. Abbott, T. Abernathy, M. R. Acernese, F. Ackley, K. Adams, C. Adams, T. Addesso, P. Adhikari, R. X. Adya, V. Affeldt, C. Agathos, M. Agatsuma, K. Aggarwal, N. Aguiar, O. D. Ain, A. Ajith, P. Alemic, A. Allen, B. Allocca, A. Amariutei, D. Anderson, S. B. Anderson, W. G. Arai, K. Araya, M. C. |
author_role |
author |
author2 |
Ortega Larcher, Walter Emanuel Aasi, J. Abbott, B. P. Abbott, R. Abbott, T. Abernathy, M. R. Acernese, F. Ackley, K. Adams, C. Adams, T. Addesso, P. Adhikari, R. X. Adya, V. Affeldt, C. Agathos, M. Agatsuma, K. Aggarwal, N. Aguiar, O. D. Ain, A. Ajith, P. Alemic, A. Allen, B. Allocca, A. Amariutei, D. Anderson, S. B. Anderson, W. G. Arai, K. Araya, M. C. |
author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
dc.subject.none.fl_str_mv |
Continuous Gravitational Waves Search Supernova Remanent |
topic |
Continuous Gravitational Waves Search Supernova Remanent |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
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. Fil: Dominguez, Alfredo Eduardo. Ministerio de Defensa. Fuerza Aerea Argentina; Argentina Fil: Ortega Larcher, Walter Emanuel. Consejo Nacional de Investigaciones Científicas y Técnicas. Unidad de Investigación y Desarrollo Estrategico Para la Defensa. Subsede Instituto Universitario Aeronautico | Ministerio de Defensa. Unidad de Investigación y Desarrollo Estrategico Para la Defensa. Subsede Instituto Universitario Aeronautico; Argentina Fil: Aasi, J.. California Institute of Technology; Estados Unidos Fil: Abbott, B. P.. California Institute of Technology; Estados Unidos Fil: Abbott, R.. California Institute of Technology; Estados Unidos Fil: Abbott, T.. State University of Louisiana; Estados Unidos Fil: Abernathy, M. R.. California Institute of Technology; Estados Unidos Fil: Acernese, F.. Universita di Salerno; Italia. Istituto Nazionale Di Fisica Nucleare; Italia Fil: Ackley, K.. University of Florida; Estados Unidos Fil: Adams, C.. Livingston Observatory; Estados Unidos Fil: Adams, T.. Cardiff University; Reino Unido. Centre National de la Recherche Scientifique; Francia. Université de Savoie; Francia Fil: Adams, T.. Centre National de la Recherche Scientifique; Francia. Université de Savoie; Francia Fil: Addesso, P.. University of Sannio at Benevento; Italia. Istituto Nazionale Di Fisica Nucleare; Italia Fil: Adhikari, R. X.. California Institute of Technology; Estados Unidos Fil: Adya, V.. Max Planck Institut für Gravitationsphysik; Alemania Fil: Affeldt, C.. Max Planck Institut für Gravitationsphysik; Alemania Fil: Agathos, M.. Nikhef; Países Bajos Fil: Agatsuma, K.. Nikhef; Países Bajos Fil: Aggarwal, N.. Massachusetts Institute of Technology; Estados Unidos Fil: Aguiar, O. D.. Centro de Previsao de Tempo e Estudos Climáticos. Instituto Nacional de Pesquisas Espaciais; Brasil Fil: Ain, A.. Inter-University Centre for Astronomy and Astrophysics; India Fil: Ajith, P.. Tata Institute of Fundamental Research; India Fil: Alemic, A.. Syracuse University; Estados Unidos Fil: Allen, B.. University of Wisconsin-Milwaukee; Estados Unidos. Max-Planck-Institut für Gravitationsphysik; Alemania Fil: Allocca, A.. Università degli Studi di Siena; Italia. Istituto Nazionale Di Fisica Nucleare; Italia Fil: Amariutei, D.. University of Florida; Estados Unidos Fil: Anderson, S. B.. California Institute of Technology; Estados Unidos Fil: Anderson, W. G.. University of Wisconsin–Milwaukee; Estados Unidos Fil: Arai, K.. California Institute of Technology; Estados Unidos Fil: Araya, M. C.. California Institute of Technology; Estados Unidos |
description |
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. |
publishDate |
2015 |
dc.date.none.fl_str_mv |
2015-10 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/131065 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 0004-637X CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/131065 |
identifier_str_mv |
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 0004-637X CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/813/1/39 info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/813/1/39 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
IOP Publishing |
publisher.none.fl_str_mv |
IOP Publishing |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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1844613503324782592 |
score |
13.070432 |