Two-color photometry with high temporal resolution of the extremely variable blazar PKS 0537-441
- Autores
- Romero, Gustavo Esteban; Cellone, Sergio Aldo; Combi, Jorge Ariel
- Año de publicación
- 2000
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We report the results of a microvariability monitoring campaign on the southern blazar PKS 0537-441. The source was observed in the V and R optical bands throughout six consecutive nights. Strong variations at both bands, with amplitudes of ∼0.3 mag, were observed on timescales of about 2 days. Smaller fluctuations of ∼0.05 mag on a scale of a couple of hours are superposed on the larger outburst. The spectral index was also variable during the observing period, with an average value of α = -1.6 and changes up to ∼27.5%. The spectrum varies in the sense that it becomes harder when the source is brighter, in accordance with predictions of shock-in-jet models. We discuss our results and the possible origin of the variability in this blazar in light of recent higher frequency observations.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto Argentino de Radioastronomía - Materia
-
Ciencias Astronómicas
BL lacertae objects: individual (PKS 0537-441)
Galaxies: active
Galaxies: photometry - 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:10915/84260
Ver los metadatos del registro completo
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Two-color photometry with high temporal resolution of the extremely variable blazar PKS 0537-441Romero, Gustavo EstebanCellone, Sergio AldoCombi, Jorge ArielCiencias AstronómicasBL lacertae objects: individual (PKS 0537-441)Galaxies: activeGalaxies: photometryWe report the results of a microvariability monitoring campaign on the southern blazar PKS 0537-441. The source was observed in the V and R optical bands throughout six consecutive nights. Strong variations at both bands, with amplitudes of ∼0.3 mag, were observed on timescales of about 2 days. Smaller fluctuations of ∼0.05 mag on a scale of a couple of hours are superposed on the larger outburst. The spectral index was also variable during the observing period, with an average value of α = -1.6 and changes up to ∼27.5%. The spectrum varies in the sense that it becomes harder when the source is brighter, in accordance with predictions of shock-in-jet models. We discuss our results and the possible origin of the variability in this blazar in light of recent higher frequency observations.Facultad de Ciencias Astronómicas y GeofísicasInstituto Argentino de Radioastronomía2000info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf1192-1197http://sedici.unlp.edu.ar/handle/10915/84260enginfo:eu-repo/semantics/altIdentifier/issn/0004-6256info:eu-repo/semantics/altIdentifier/doi/10.1086/301526info: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:UNLP2025-09-29T11:16:19Zoai:sedici.unlp.edu.ar:10915/84260Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:16:20.206SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Two-color photometry with high temporal resolution of the extremely variable blazar PKS 0537-441 |
title |
Two-color photometry with high temporal resolution of the extremely variable blazar PKS 0537-441 |
spellingShingle |
Two-color photometry with high temporal resolution of the extremely variable blazar PKS 0537-441 Romero, Gustavo Esteban Ciencias Astronómicas BL lacertae objects: individual (PKS 0537-441) Galaxies: active Galaxies: photometry |
title_short |
Two-color photometry with high temporal resolution of the extremely variable blazar PKS 0537-441 |
title_full |
Two-color photometry with high temporal resolution of the extremely variable blazar PKS 0537-441 |
title_fullStr |
Two-color photometry with high temporal resolution of the extremely variable blazar PKS 0537-441 |
title_full_unstemmed |
Two-color photometry with high temporal resolution of the extremely variable blazar PKS 0537-441 |
title_sort |
Two-color photometry with high temporal resolution of the extremely variable blazar PKS 0537-441 |
dc.creator.none.fl_str_mv |
Romero, Gustavo Esteban Cellone, Sergio Aldo Combi, Jorge Ariel |
author |
Romero, Gustavo Esteban |
author_facet |
Romero, Gustavo Esteban Cellone, Sergio Aldo Combi, Jorge Ariel |
author_role |
author |
author2 |
Cellone, Sergio Aldo Combi, Jorge Ariel |
author2_role |
author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas BL lacertae objects: individual (PKS 0537-441) Galaxies: active Galaxies: photometry |
topic |
Ciencias Astronómicas BL lacertae objects: individual (PKS 0537-441) Galaxies: active Galaxies: photometry |
dc.description.none.fl_txt_mv |
We report the results of a microvariability monitoring campaign on the southern blazar PKS 0537-441. The source was observed in the V and R optical bands throughout six consecutive nights. Strong variations at both bands, with amplitudes of ∼0.3 mag, were observed on timescales of about 2 days. Smaller fluctuations of ∼0.05 mag on a scale of a couple of hours are superposed on the larger outburst. The spectral index was also variable during the observing period, with an average value of α = -1.6 and changes up to ∼27.5%. The spectrum varies in the sense that it becomes harder when the source is brighter, in accordance with predictions of shock-in-jet models. We discuss our results and the possible origin of the variability in this blazar in light of recent higher frequency observations. Facultad de Ciencias Astronómicas y Geofísicas Instituto Argentino de Radioastronomía |
description |
We report the results of a microvariability monitoring campaign on the southern blazar PKS 0537-441. The source was observed in the V and R optical bands throughout six consecutive nights. Strong variations at both bands, with amplitudes of ∼0.3 mag, were observed on timescales of about 2 days. Smaller fluctuations of ∼0.05 mag on a scale of a couple of hours are superposed on the larger outburst. The spectral index was also variable during the observing period, with an average value of α = -1.6 and changes up to ∼27.5%. The spectrum varies in the sense that it becomes harder when the source is brighter, in accordance with predictions of shock-in-jet models. We discuss our results and the possible origin of the variability in this blazar in light of recent higher frequency observations. |
publishDate |
2000 |
dc.date.none.fl_str_mv |
2000 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo 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://sedici.unlp.edu.ar/handle/10915/84260 |
url |
http://sedici.unlp.edu.ar/handle/10915/84260 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/0004-6256 info:eu-repo/semantics/altIdentifier/doi/10.1086/301526 |
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 1192-1197 |
dc.source.none.fl_str_mv |
reponame:SEDICI (UNLP) instname:Universidad Nacional de La Plata instacron:UNLP |
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SEDICI (UNLP) |
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Universidad Nacional de La Plata |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
repository.mail.fl_str_mv |
alira@sedici.unlp.edu.ar |
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