Study of Variability in Long-term Multiwavelength Optical Lightcurves of Blazar AO 0235+164
- Autores
- Roy, Abhradeep; Gupta, Alok C.; Chitnis, Varsha R.; Cellone, Sergio Aldo; Raiteri, Claudia M.; Romero, Gustavo Esteban; Wiita, Paul J.; Chatterjee, Anshu; Combi, Jorge Ariel; Liao, Mai; Sarkar, Arkadipta; Villata, Massimo
- Año de publicación
- 2023
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present a long-term and intraday variability study of optical multiwaveband (U BV RI) data from the blazar AO 0235+164 collected by various telescopes for ∼44 yr (1975-2019). The blazar was found to be significantly variable over the years in all wave bands with a variation of about 6 mag between its low and active states. The variations in the different wave bands are highly correlated without any time lag. We did not observe any significant trend in color variation with time, but we observed a bluer-when-brighter trend between the B − I color index and the R magnitude. Optical BV R-band spectral energy distributions always show a convex shape. Significant intraday variability was frequently seen in the quasi-simultaneous observations of AO 0235+164 made on 22 nights in the R and V bands by the CASLEO and CAHA telescopes during 1999-2019. We also estimated a central supermassive black hole mass of 7.9 × 107 M ⊙ by analyzing the broad Mg ii emission line in AO 0235+164's spectrum. We briefly explore the probable physical scenarios responsible for the observed variability.
Fil: Roy, Abhradeep. International Centre Of Theoretical Science. Tata Institute Of Fundamental Research; España
Fil: Gupta, Alok C.. Aryabhatta Research Institute Of Observational Sciences; India. Chinese Academy of Sciences; República de China
Fil: Chitnis, Varsha R.. International Centre Of Theoretical Science. Tata Institute Of Fundamental Research; España
Fil: Cellone, Sergio Aldo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Raiteri, Claudia M.. Istituto Nazionale di Astrofisica; Italia
Fil: Romero, Gustavo Esteban. Universidad Nacional de La Plata; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina
Fil: Wiita, Paul J.. The College Of New Jersey; Estados Unidos
Fil: Chatterjee, Anshu. International Centre Of Theoretical Science. Tata Institute Of Fundamental Research; España
Fil: Combi, Jorge Ariel. Universidad de Jaén; España. Universidad Nacional de La Plata; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Liao, Mai. University Of Science And Technology Of China; China
Fil: Sarkar, Arkadipta. Deutsches Elektronen-synchrotron; Alemania
Fil: Villata, Massimo. Istituto Nazionale di Astrofisica; Italia - Materia
-
Galaxies; Active galaxies
BL Lacertae objects
Quasars - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/227894
Ver los metadatos del registro completo
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Study of Variability in Long-term Multiwavelength Optical Lightcurves of Blazar AO 0235+164Roy, AbhradeepGupta, Alok C.Chitnis, Varsha R.Cellone, Sergio AldoRaiteri, Claudia M.Romero, Gustavo EstebanWiita, Paul J.Chatterjee, AnshuCombi, Jorge ArielLiao, MaiSarkar, ArkadiptaVillata, MassimoGalaxies; Active galaxiesBL Lacertae objectsQuasarshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present a long-term and intraday variability study of optical multiwaveband (U BV RI) data from the blazar AO 0235+164 collected by various telescopes for ∼44 yr (1975-2019). The blazar was found to be significantly variable over the years in all wave bands with a variation of about 6 mag between its low and active states. The variations in the different wave bands are highly correlated without any time lag. We did not observe any significant trend in color variation with time, but we observed a bluer-when-brighter trend between the B − I color index and the R magnitude. Optical BV R-band spectral energy distributions always show a convex shape. Significant intraday variability was frequently seen in the quasi-simultaneous observations of AO 0235+164 made on 22 nights in the R and V bands by the CASLEO and CAHA telescopes during 1999-2019. We also estimated a central supermassive black hole mass of 7.9 × 107 M ⊙ by analyzing the broad Mg ii emission line in AO 0235+164's spectrum. We briefly explore the probable physical scenarios responsible for the observed variability.Fil: Roy, Abhradeep. International Centre Of Theoretical Science. Tata Institute Of Fundamental Research; EspañaFil: Gupta, Alok C.. Aryabhatta Research Institute Of Observational Sciences; India. Chinese Academy of Sciences; República de ChinaFil: Chitnis, Varsha R.. International Centre Of Theoretical Science. Tata Institute Of Fundamental Research; EspañaFil: Cellone, Sergio Aldo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Raiteri, Claudia M.. Istituto Nazionale di Astrofisica; ItaliaFil: Romero, Gustavo Esteban. Universidad Nacional de La Plata; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; ArgentinaFil: Wiita, Paul J.. The College Of New Jersey; Estados UnidosFil: Chatterjee, Anshu. International Centre Of Theoretical Science. Tata Institute Of Fundamental Research; EspañaFil: Combi, Jorge Ariel. Universidad de Jaén; España. Universidad Nacional de La Plata; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Liao, Mai. University Of Science And Technology Of China; ChinaFil: Sarkar, Arkadipta. Deutsches Elektronen-synchrotron; AlemaniaFil: Villata, Massimo. Istituto Nazionale di Astrofisica; ItaliaIOP Publishing2023-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/227894Roy, Abhradeep; Gupta, Alok C.; Chitnis, Varsha R.; Cellone, Sergio Aldo; Raiteri, Claudia M.; et al.; Study of Variability in Long-term Multiwavelength Optical Lightcurves of Blazar AO 0235+164; IOP Publishing; Astrophysical Journal Supplement Series; 265; 1; 3-2023; 14-330067-0049CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4365/acb059info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4365/acb059info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:54:54Zoai:ri.conicet.gov.ar:11336/227894instacron: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:34982025-10-22 11:54:54.882CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Study of Variability in Long-term Multiwavelength Optical Lightcurves of Blazar AO 0235+164 |
| title |
Study of Variability in Long-term Multiwavelength Optical Lightcurves of Blazar AO 0235+164 |
| spellingShingle |
Study of Variability in Long-term Multiwavelength Optical Lightcurves of Blazar AO 0235+164 Roy, Abhradeep Galaxies; Active galaxies BL Lacertae objects Quasars |
| title_short |
Study of Variability in Long-term Multiwavelength Optical Lightcurves of Blazar AO 0235+164 |
| title_full |
Study of Variability in Long-term Multiwavelength Optical Lightcurves of Blazar AO 0235+164 |
| title_fullStr |
Study of Variability in Long-term Multiwavelength Optical Lightcurves of Blazar AO 0235+164 |
| title_full_unstemmed |
Study of Variability in Long-term Multiwavelength Optical Lightcurves of Blazar AO 0235+164 |
| title_sort |
Study of Variability in Long-term Multiwavelength Optical Lightcurves of Blazar AO 0235+164 |
| dc.creator.none.fl_str_mv |
Roy, Abhradeep Gupta, Alok C. Chitnis, Varsha R. Cellone, Sergio Aldo Raiteri, Claudia M. Romero, Gustavo Esteban Wiita, Paul J. Chatterjee, Anshu Combi, Jorge Ariel Liao, Mai Sarkar, Arkadipta Villata, Massimo |
| author |
Roy, Abhradeep |
| author_facet |
Roy, Abhradeep Gupta, Alok C. Chitnis, Varsha R. Cellone, Sergio Aldo Raiteri, Claudia M. Romero, Gustavo Esteban Wiita, Paul J. Chatterjee, Anshu Combi, Jorge Ariel Liao, Mai Sarkar, Arkadipta Villata, Massimo |
| author_role |
author |
| author2 |
Gupta, Alok C. Chitnis, Varsha R. Cellone, Sergio Aldo Raiteri, Claudia M. Romero, Gustavo Esteban Wiita, Paul J. Chatterjee, Anshu Combi, Jorge Ariel Liao, Mai Sarkar, Arkadipta Villata, Massimo |
| author2_role |
author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
Galaxies; Active galaxies BL Lacertae objects Quasars |
| topic |
Galaxies; Active galaxies BL Lacertae objects Quasars |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
We present a long-term and intraday variability study of optical multiwaveband (U BV RI) data from the blazar AO 0235+164 collected by various telescopes for ∼44 yr (1975-2019). The blazar was found to be significantly variable over the years in all wave bands with a variation of about 6 mag between its low and active states. The variations in the different wave bands are highly correlated without any time lag. We did not observe any significant trend in color variation with time, but we observed a bluer-when-brighter trend between the B − I color index and the R magnitude. Optical BV R-band spectral energy distributions always show a convex shape. Significant intraday variability was frequently seen in the quasi-simultaneous observations of AO 0235+164 made on 22 nights in the R and V bands by the CASLEO and CAHA telescopes during 1999-2019. We also estimated a central supermassive black hole mass of 7.9 × 107 M ⊙ by analyzing the broad Mg ii emission line in AO 0235+164's spectrum. We briefly explore the probable physical scenarios responsible for the observed variability. Fil: Roy, Abhradeep. International Centre Of Theoretical Science. Tata Institute Of Fundamental Research; España Fil: Gupta, Alok C.. Aryabhatta Research Institute Of Observational Sciences; India. Chinese Academy of Sciences; República de China Fil: Chitnis, Varsha R.. International Centre Of Theoretical Science. Tata Institute Of Fundamental Research; España Fil: Cellone, Sergio Aldo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Raiteri, Claudia M.. Istituto Nazionale di Astrofisica; Italia Fil: Romero, Gustavo Esteban. Universidad Nacional de La Plata; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina Fil: Wiita, Paul J.. The College Of New Jersey; Estados Unidos Fil: Chatterjee, Anshu. International Centre Of Theoretical Science. Tata Institute Of Fundamental Research; España Fil: Combi, Jorge Ariel. Universidad de Jaén; España. Universidad Nacional de La Plata; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Liao, Mai. University Of Science And Technology Of China; China Fil: Sarkar, Arkadipta. Deutsches Elektronen-synchrotron; Alemania Fil: Villata, Massimo. Istituto Nazionale di Astrofisica; Italia |
| description |
We present a long-term and intraday variability study of optical multiwaveband (U BV RI) data from the blazar AO 0235+164 collected by various telescopes for ∼44 yr (1975-2019). The blazar was found to be significantly variable over the years in all wave bands with a variation of about 6 mag between its low and active states. The variations in the different wave bands are highly correlated without any time lag. We did not observe any significant trend in color variation with time, but we observed a bluer-when-brighter trend between the B − I color index and the R magnitude. Optical BV R-band spectral energy distributions always show a convex shape. Significant intraday variability was frequently seen in the quasi-simultaneous observations of AO 0235+164 made on 22 nights in the R and V bands by the CASLEO and CAHA telescopes during 1999-2019. We also estimated a central supermassive black hole mass of 7.9 × 107 M ⊙ by analyzing the broad Mg ii emission line in AO 0235+164's spectrum. We briefly explore the probable physical scenarios responsible for the observed variability. |
| publishDate |
2023 |
| dc.date.none.fl_str_mv |
2023-03 |
| 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/11336/227894 Roy, Abhradeep; Gupta, Alok C.; Chitnis, Varsha R.; Cellone, Sergio Aldo; Raiteri, Claudia M.; et al.; Study of Variability in Long-term Multiwavelength Optical Lightcurves of Blazar AO 0235+164; IOP Publishing; Astrophysical Journal Supplement Series; 265; 1; 3-2023; 14-33 0067-0049 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/227894 |
| identifier_str_mv |
Roy, Abhradeep; Gupta, Alok C.; Chitnis, Varsha R.; Cellone, Sergio Aldo; Raiteri, Claudia M.; et al.; Study of Variability in Long-term Multiwavelength Optical Lightcurves of Blazar AO 0235+164; IOP Publishing; Astrophysical Journal Supplement Series; 265; 1; 3-2023; 14-33 0067-0049 CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
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info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4365/acb059 info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4365/acb059 |
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openAccess |
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https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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application/pdf application/pdf |
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IOP Publishing |
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IOP Publishing |
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reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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CONICET Digital (CONICET) |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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