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
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/165284
Ver los metadatos del registro completo
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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:UNLP2025-09-29T11:43:50Zoai: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:13292025-09-29 11:43:50.956SEDICI (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 |
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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 |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
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alira@sedici.unlp.edu.ar |
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