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
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/131065

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network_name_str CONICET Digital (CONICET)
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 Técnicas2025-09-29T09:48:23Zoai: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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