Host Galaxy and Nuclear Properties of IR-selected AGNs with and without Outflow Signatures
- Autores
- Oio, Gabriel Andrés; Dai, Y. Sophia; Bornancini, Carlos Guillermo; Li, Zi Jian
- Año de publicación
- 2024
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Active galactic nucleus (AGN) driven outflows can have a significant impact on the evolution of the host galaxy. Inthis work, we compare the properties of galaxies that host AGNs with and without outflows. Our sample consists of103 AGNs identified by mid-IR color–color selection and confirmed with optical spectroscopy at a redshift rangeof 0.3 < z < 0.9. We fit the [O III] λ5007 line using spectra from the zCOSMOS survey to identify and study theoccurrence of outflows. We find that ionized outflows are present in ∼25% of our sample, with the largestincidence at the highest [O III] and X-ray luminosity bins. The fastest outflows are found in the more extended andmassive galaxies. We do not observe a difference in the star formation rate of AGNs with outflows compared toAGNs without outflows. From visual inspection and nonparametric morphological studies, we obtain that outflowsare preferentially observed in galaxies with disk-type and elliptical morphologies.
Fil: Oio, Gabriel Andrés. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Chinese Academy of Sciences; República de China
Fil: Dai, Y. Sophia. Chinese Academy of Sciences; República de China
Fil: Bornancini, Carlos Guillermo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Li, Zi Jian. Chinese Academy of Sciences; República de China - Materia
-
Infrared galaxies
Emission line galaxies
Active galactic nuclei
AGN host galaxies - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
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- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/256977
Ver los metadatos del registro completo
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Host Galaxy and Nuclear Properties of IR-selected AGNs with and without Outflow SignaturesOio, Gabriel AndrésDai, Y. SophiaBornancini, Carlos GuillermoLi, Zi JianInfrared galaxiesEmission line galaxiesActive galactic nucleiAGN host galaxieshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Active galactic nucleus (AGN) driven outflows can have a significant impact on the evolution of the host galaxy. Inthis work, we compare the properties of galaxies that host AGNs with and without outflows. Our sample consists of103 AGNs identified by mid-IR color–color selection and confirmed with optical spectroscopy at a redshift rangeof 0.3 < z < 0.9. We fit the [O III] λ5007 line using spectra from the zCOSMOS survey to identify and study theoccurrence of outflows. We find that ionized outflows are present in ∼25% of our sample, with the largestincidence at the highest [O III] and X-ray luminosity bins. The fastest outflows are found in the more extended andmassive galaxies. We do not observe a difference in the star formation rate of AGNs with outflows compared toAGNs without outflows. From visual inspection and nonparametric morphological studies, we obtain that outflowsare preferentially observed in galaxies with disk-type and elliptical morphologies.Fil: Oio, Gabriel Andrés. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Chinese Academy of Sciences; República de ChinaFil: Dai, Y. Sophia. Chinese Academy of Sciences; República de ChinaFil: Bornancini, Carlos Guillermo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Li, Zi Jian. Chinese Academy of Sciences; República de ChinaIOP Publishing2024-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/256977Oio, Gabriel Andrés; Dai, Y. Sophia; Bornancini, Carlos Guillermo; Li, Zi Jian; Host Galaxy and Nuclear Properties of IR-selected AGNs with and without Outflow Signatures; IOP Publishing; Astrophysical Journal; 962; 2; 2-2024; 1-160004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/ad18a5info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ad18a5info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:14:04Zoai:ri.conicet.gov.ar:11336/256977instacron: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 11:14:04.724CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Host Galaxy and Nuclear Properties of IR-selected AGNs with and without Outflow Signatures |
| title |
Host Galaxy and Nuclear Properties of IR-selected AGNs with and without Outflow Signatures |
| spellingShingle |
Host Galaxy and Nuclear Properties of IR-selected AGNs with and without Outflow Signatures Oio, Gabriel Andrés Infrared galaxies Emission line galaxies Active galactic nuclei AGN host galaxies |
| title_short |
Host Galaxy and Nuclear Properties of IR-selected AGNs with and without Outflow Signatures |
| title_full |
Host Galaxy and Nuclear Properties of IR-selected AGNs with and without Outflow Signatures |
| title_fullStr |
Host Galaxy and Nuclear Properties of IR-selected AGNs with and without Outflow Signatures |
| title_full_unstemmed |
Host Galaxy and Nuclear Properties of IR-selected AGNs with and without Outflow Signatures |
| title_sort |
Host Galaxy and Nuclear Properties of IR-selected AGNs with and without Outflow Signatures |
| dc.creator.none.fl_str_mv |
Oio, Gabriel Andrés Dai, Y. Sophia Bornancini, Carlos Guillermo Li, Zi Jian |
| author |
Oio, Gabriel Andrés |
| author_facet |
Oio, Gabriel Andrés Dai, Y. Sophia Bornancini, Carlos Guillermo Li, Zi Jian |
| author_role |
author |
| author2 |
Dai, Y. Sophia Bornancini, Carlos Guillermo Li, Zi Jian |
| author2_role |
author author author |
| dc.subject.none.fl_str_mv |
Infrared galaxies Emission line galaxies Active galactic nuclei AGN host galaxies |
| topic |
Infrared galaxies Emission line galaxies Active galactic nuclei AGN host galaxies |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
Active galactic nucleus (AGN) driven outflows can have a significant impact on the evolution of the host galaxy. Inthis work, we compare the properties of galaxies that host AGNs with and without outflows. Our sample consists of103 AGNs identified by mid-IR color–color selection and confirmed with optical spectroscopy at a redshift rangeof 0.3 < z < 0.9. We fit the [O III] λ5007 line using spectra from the zCOSMOS survey to identify and study theoccurrence of outflows. We find that ionized outflows are present in ∼25% of our sample, with the largestincidence at the highest [O III] and X-ray luminosity bins. The fastest outflows are found in the more extended andmassive galaxies. We do not observe a difference in the star formation rate of AGNs with outflows compared toAGNs without outflows. From visual inspection and nonparametric morphological studies, we obtain that outflowsare preferentially observed in galaxies with disk-type and elliptical morphologies. Fil: Oio, Gabriel Andrés. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Chinese Academy of Sciences; República de China Fil: Dai, Y. Sophia. Chinese Academy of Sciences; República de China Fil: Bornancini, Carlos Guillermo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina Fil: Li, Zi Jian. Chinese Academy of Sciences; República de China |
| description |
Active galactic nucleus (AGN) driven outflows can have a significant impact on the evolution of the host galaxy. Inthis work, we compare the properties of galaxies that host AGNs with and without outflows. Our sample consists of103 AGNs identified by mid-IR color–color selection and confirmed with optical spectroscopy at a redshift rangeof 0.3 < z < 0.9. We fit the [O III] λ5007 line using spectra from the zCOSMOS survey to identify and study theoccurrence of outflows. We find that ionized outflows are present in ∼25% of our sample, with the largestincidence at the highest [O III] and X-ray luminosity bins. The fastest outflows are found in the more extended andmassive galaxies. We do not observe a difference in the star formation rate of AGNs with outflows compared toAGNs without outflows. From visual inspection and nonparametric morphological studies, we obtain that outflowsare preferentially observed in galaxies with disk-type and elliptical morphologies. |
| publishDate |
2024 |
| dc.date.none.fl_str_mv |
2024-02 |
| 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 |
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article |
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publishedVersion |
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http://hdl.handle.net/11336/256977 Oio, Gabriel Andrés; Dai, Y. Sophia; Bornancini, Carlos Guillermo; Li, Zi Jian; Host Galaxy and Nuclear Properties of IR-selected AGNs with and without Outflow Signatures; IOP Publishing; Astrophysical Journal; 962; 2; 2-2024; 1-16 0004-637X CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/256977 |
| identifier_str_mv |
Oio, Gabriel Andrés; Dai, Y. Sophia; Bornancini, Carlos Guillermo; Li, Zi Jian; Host Galaxy and Nuclear Properties of IR-selected AGNs with and without Outflow Signatures; IOP Publishing; Astrophysical Journal; 962; 2; 2-2024; 1-16 0004-637X CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
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eng |
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info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/ad18a5 info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ad18a5 |
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openAccess |
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https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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IOP Publishing |
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IOP Publishing |
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