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

Acceder

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spelling	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 Técnicas2025-10-22T11:17:22Zoai: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:34982025-10-22 11:17:23.103CONICET 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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score	12.982451

Searches for continuous gravitational waves from nine young supernova remnants

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