The incidence of the host galaxy light in the polarized emission of the blazars 1959+650 and 2201+044

Autores
Sosa, Marina; Cellone, Sergio Aldo; Andruchow, Ileana; Von Essen, Carolina
Año de publicación
2014
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
We present a study carried out to determine variations in scales ranging from hours to days, both in the total flux and optical linear polarization in two blazars: 1959+650 and 2201+044. Both blazars are relatively nearby active galactic nuclei, so their host galaxies are well resolved, having accurately measured photometric parameters. This allowed us to apply models that take into account the depolarizing effect introduced by the (un-polarized) light of the galaxy, and, at the same time, to evaluate any spurious variation in polarization time-curves due to variable seeing conditions, that affect differently the (pointlike) core and the (extended) host galaxy. Our results provide information on the optical behaviour of high energy blazars, taking advantage of a scarcely explored technique as optical polarimetry with high-temporal resolution.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Ciencias Astronómicas
blazars
optical polarimetry
optical behaviour
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/165284
Acceder
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network_acronym_str SEDICI
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network_name_str SEDICI (UNLP)
spelling The incidence of the host galaxy light in the polarized emission of the blazars 1959+650 and 2201+044Sosa, MarinaCellone, Sergio AldoAndruchow, IleanaVon Essen, CarolinaCiencias Astronómicasblazarsoptical polarimetryoptical behaviourWe present a study carried out to determine variations in scales ranging from hours to days, both in the total flux and optical linear polarization in two blazars: 1959+650 and 2201+044. Both blazars are relatively nearby active galactic nuclei, so their host galaxies are well resolved, having accurately measured photometric parameters. This allowed us to apply models that take into account the depolarizing effect introduced by the (un-polarized) light of the galaxy, and, at the same time, to evaluate any spurious variation in polarization time-curves due to variable seeing conditions, that affect differently the (pointlike) core and the (extended) host galaxy. Our results provide information on the optical behaviour of high energy blazars, taking advantage of a scarcely explored technique as optical polarimetry with high-temporal resolution.Facultad de Ciencias Astronómicas y Geofísicas2014-04info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionObjeto de conferenciahttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdf227-230http://sedici.unlp.edu.ar/handle/10915/165284enginfo:eu-repo/semantics/altIdentifier/isbn/978-987-24948-2-7info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-22T17:24:45Zoai:sedici.unlp.edu.ar:10915/165284Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 17:24:46.081SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv The incidence of the host galaxy light in the polarized emission of the blazars 1959+650 and 2201+044
title The incidence of the host galaxy light in the polarized emission of the blazars 1959+650 and 2201+044
spellingShingle The incidence of the host galaxy light in the polarized emission of the blazars 1959+650 and 2201+044
Sosa, Marina
Ciencias Astronómicas
blazars
optical polarimetry
optical behaviour
title_short The incidence of the host galaxy light in the polarized emission of the blazars 1959+650 and 2201+044
title_full The incidence of the host galaxy light in the polarized emission of the blazars 1959+650 and 2201+044
title_fullStr The incidence of the host galaxy light in the polarized emission of the blazars 1959+650 and 2201+044
title_full_unstemmed The incidence of the host galaxy light in the polarized emission of the blazars 1959+650 and 2201+044
title_sort The incidence of the host galaxy light in the polarized emission of the blazars 1959+650 and 2201+044
dc.creator.none.fl_str_mv Sosa, Marina
Cellone, Sergio Aldo
Andruchow, Ileana
Von Essen, Carolina
author Sosa, Marina
author_facet Sosa, Marina
Cellone, Sergio Aldo
Andruchow, Ileana
Von Essen, Carolina
author_role author
author2 Cellone, Sergio Aldo
Andruchow, Ileana
Von Essen, Carolina
author2_role author
author
author
dc.subject.none.fl_str_mv Ciencias Astronómicas
blazars
optical polarimetry
optical behaviour
topic Ciencias Astronómicas
blazars
optical polarimetry
optical behaviour
dc.description.none.fl_txt_mv We present a study carried out to determine variations in scales ranging from hours to days, both in the total flux and optical linear polarization in two blazars: 1959+650 and 2201+044. Both blazars are relatively nearby active galactic nuclei, so their host galaxies are well resolved, having accurately measured photometric parameters. This allowed us to apply models that take into account the depolarizing effect introduced by the (un-polarized) light of the galaxy, and, at the same time, to evaluate any spurious variation in polarization time-curves due to variable seeing conditions, that affect differently the (pointlike) core and the (extended) host galaxy. Our results provide information on the optical behaviour of high energy blazars, taking advantage of a scarcely explored technique as optical polarimetry with high-temporal resolution.
Facultad de Ciencias Astronómicas y Geofísicas
description We present a study carried out to determine variations in scales ranging from hours to days, both in the total flux and optical linear polarization in two blazars: 1959+650 and 2201+044. Both blazars are relatively nearby active galactic nuclei, so their host galaxies are well resolved, having accurately measured photometric parameters. This allowed us to apply models that take into account the depolarizing effect introduced by the (un-polarized) light of the galaxy, and, at the same time, to evaluate any spurious variation in polarization time-curves due to variable seeing conditions, that affect differently the (pointlike) core and the (extended) host galaxy. Our results provide information on the optical behaviour of high energy blazars, taking advantage of a scarcely explored technique as optical polarimetry with high-temporal resolution.
publishDate 2014
dc.date.none.fl_str_mv 2014-04
dc.type.none.fl_str_mv info:eu-repo/semantics/conferenceObject
info:eu-repo/semantics/publishedVersion
Objeto de conferencia
http://purl.org/coar/resource_type/c_5794
info:ar-repo/semantics/documentoDeConferencia
format conferenceObject
status_str publishedVersion
dc.identifier.none.fl_str_mv http://sedici.unlp.edu.ar/handle/10915/165284
url http://sedici.unlp.edu.ar/handle/10915/165284
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/isbn/978-987-24948-2-7
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.format.none.fl_str_mv application/pdf
227-230
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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