Extremely violent optical microvariability in blazars: Fact or fiction?
- Autores
- Cellone, Sergio Aldo; Romero, Gustavo Esteban; Araudo, Anabella Teresa
- Año de publicación
- 2006
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Variability amplitudes larger than 1 mag over time-scales of a few tens of minutes have recently been reported in the optical light curves of several blazars. In order to independently verify the real occurrence of such extremely violent events, we undertook an observational study of a selected sample of three blazars: PKS 0048-097, PKS 0754+100 and PKS 1510-089. Possible systematic error sources during data acquisition and reduction were carefully evaluated. We indeed found flux variability at intra-night time-scales in all the three sources, although no extremely violent behaviour, as reported by other authors, was detected. We show that an incorrect choice of the stars used for differential photometry will, under fairly normal conditions, lead to spurious variability with large amplitudes on short time-scales. Wrong results of this kind can be avoided with the use of simple error-control techniques.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
BL Lacertae objects: general
Galaxies: active
Galaxies: photometry - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/83045
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Extremely violent optical microvariability in blazars: Fact or fiction?Cellone, Sergio AldoRomero, Gustavo EstebanAraudo, Anabella TeresaCiencias AstronómicasBL Lacertae objects: generalGalaxies: activeGalaxies: photometryVariability amplitudes larger than 1 mag over time-scales of a few tens of minutes have recently been reported in the optical light curves of several blazars. In order to independently verify the real occurrence of such extremely violent events, we undertook an observational study of a selected sample of three blazars: PKS 0048-097, PKS 0754+100 and PKS 1510-089. Possible systematic error sources during data acquisition and reduction were carefully evaluated. We indeed found flux variability at intra-night time-scales in all the three sources, although no extremely violent behaviour, as reported by other authors, was detected. We show that an incorrect choice of the stars used for differential photometry will, under fairly normal conditions, lead to spurious variability with large amplitudes on short time-scales. Wrong results of this kind can be avoided with the use of simple error-control techniques.Facultad de Ciencias Astronómicas y Geofísicas2006-11-14info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf357-364http://sedici.unlp.edu.ar/handle/10915/83045enginfo:eu-repo/semantics/altIdentifier/issn/0035-8711info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2006.11140.xinfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/4.0/Creative Commons Attribution 4.0 International (CC BY 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:15:45Zoai:sedici.unlp.edu.ar:10915/83045Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:15:45.935SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Extremely violent optical microvariability in blazars: Fact or fiction? |
title |
Extremely violent optical microvariability in blazars: Fact or fiction? |
spellingShingle |
Extremely violent optical microvariability in blazars: Fact or fiction? Cellone, Sergio Aldo Ciencias Astronómicas BL Lacertae objects: general Galaxies: active Galaxies: photometry |
title_short |
Extremely violent optical microvariability in blazars: Fact or fiction? |
title_full |
Extremely violent optical microvariability in blazars: Fact or fiction? |
title_fullStr |
Extremely violent optical microvariability in blazars: Fact or fiction? |
title_full_unstemmed |
Extremely violent optical microvariability in blazars: Fact or fiction? |
title_sort |
Extremely violent optical microvariability in blazars: Fact or fiction? |
dc.creator.none.fl_str_mv |
Cellone, Sergio Aldo Romero, Gustavo Esteban Araudo, Anabella Teresa |
author |
Cellone, Sergio Aldo |
author_facet |
Cellone, Sergio Aldo Romero, Gustavo Esteban Araudo, Anabella Teresa |
author_role |
author |
author2 |
Romero, Gustavo Esteban Araudo, Anabella Teresa |
author2_role |
author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas BL Lacertae objects: general Galaxies: active Galaxies: photometry |
topic |
Ciencias Astronómicas BL Lacertae objects: general Galaxies: active Galaxies: photometry |
dc.description.none.fl_txt_mv |
Variability amplitudes larger than 1 mag over time-scales of a few tens of minutes have recently been reported in the optical light curves of several blazars. In order to independently verify the real occurrence of such extremely violent events, we undertook an observational study of a selected sample of three blazars: PKS 0048-097, PKS 0754+100 and PKS 1510-089. Possible systematic error sources during data acquisition and reduction were carefully evaluated. We indeed found flux variability at intra-night time-scales in all the three sources, although no extremely violent behaviour, as reported by other authors, was detected. We show that an incorrect choice of the stars used for differential photometry will, under fairly normal conditions, lead to spurious variability with large amplitudes on short time-scales. Wrong results of this kind can be avoided with the use of simple error-control techniques. Facultad de Ciencias Astronómicas y Geofísicas |
description |
Variability amplitudes larger than 1 mag over time-scales of a few tens of minutes have recently been reported in the optical light curves of several blazars. In order to independently verify the real occurrence of such extremely violent events, we undertook an observational study of a selected sample of three blazars: PKS 0048-097, PKS 0754+100 and PKS 1510-089. Possible systematic error sources during data acquisition and reduction were carefully evaluated. We indeed found flux variability at intra-night time-scales in all the three sources, although no extremely violent behaviour, as reported by other authors, was detected. We show that an incorrect choice of the stars used for differential photometry will, under fairly normal conditions, lead to spurious variability with large amplitudes on short time-scales. Wrong results of this kind can be avoided with the use of simple error-control techniques. |
publishDate |
2006 |
dc.date.none.fl_str_mv |
2006-11-14 |
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/10915/83045 |
url |
http://sedici.unlp.edu.ar/handle/10915/83045 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/0035-8711 info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2006.11140.x |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/4.0/ Creative Commons Attribution 4.0 International (CC BY 4.0) |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
http://creativecommons.org/licenses/by/4.0/ Creative Commons Attribution 4.0 International (CC BY 4.0) |
dc.format.none.fl_str_mv |
application/pdf 357-364 |
dc.source.none.fl_str_mv |
reponame:SEDICI (UNLP) instname:Universidad Nacional de La Plata instacron: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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