Chemical abundances of Seyfert 2 AGNs, II: N2 metallicity calibration based on SDSS
- Autores
- Carvalho, S.P.; Dors, O. L.; Cardaci, Monica Viviana; Hägele, Guillermo Federico; Krabbe, Nora Cristina; Pérez Montero, E.; Monteiro, A.F.; Armah, M.; Freitas Lemes, P.
- Año de publicación
- 2020
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present a semi-empirical calibration between the metallicity (Z) of Seyfert 2 active galactic nuclei and the N2 = log([N II]λ6584/H a) emission-line intensity ratio. This calibration was derived through the [OIII]λ5007/[O II]λ3727 versus N2 diagram containing observational data and photoionization model results obtained with the CLOUDY code. The observational sample consists of 463 confirmed Seyfert 2 nuclei (redshift z ≤ 0.4) taken from the Sloan Digital Sky Survey DR7 data set. The obtained Z-N2 relation is valid for the range 0.3 ≤ (Z/Z⊙) ≤ 2.0 that corresponds to -0.7 ≤ (N2) ≤ 0.6. The effects of varying the ionization parameter (U), electron density and the slope of the spectral energy distribution on the Z estimations are of the order of the uncertainty produced by the error measurements of N2. This result indicates the large reliability of our Z -N2 calibration. A relation between U and the [OIII]/[O II] line ratio, almost independent of other nebular parameter, was obtained.
Fil: Carvalho, S.P.. Universidade Do Vale Do Paraiba; Brasil
Fil: Dors, O. L.. Universidade Do Vale Do Paraiba; Brasil
Fil: Cardaci, Monica Viviana. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Hägele, Guillermo Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Krabbe, Nora Cristina. Universidade Do Vale Do Paraiba; Brasil
Fil: Pérez Montero, E.. Instituto de Astrofísica de Andalucía; España
Fil: Monteiro, A.F.. Universidade Do Vale Do Paraiba; Brasil
Fil: Armah, M.. Universidade Do Vale Do Paraiba; Brasil
Fil: Freitas Lemes, P.. Universidade Do Vale Do Paraiba; Brasil - Materia
-
GALAXIES: ABUNDANCES
GALAXIES: ACTIVE
GALAXIES: EVOLUTION
GALAXIES: FORMATION
GALAXIES: ISM
GALAXIES: NUCLEI
GALAXIES: SEYFERT - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/144111
Ver los metadatos del registro completo
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oai_identifier_str |
oai:ri.conicet.gov.ar:11336/144111 |
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3498 |
network_name_str |
CONICET Digital (CONICET) |
spelling |
Chemical abundances of Seyfert 2 AGNs, II: N2 metallicity calibration based on SDSSCarvalho, S.P.Dors, O. L.Cardaci, Monica VivianaHägele, Guillermo FedericoKrabbe, Nora CristinaPérez Montero, E.Monteiro, A.F.Armah, M.Freitas Lemes, P.GALAXIES: ABUNDANCESGALAXIES: ACTIVEGALAXIES: EVOLUTIONGALAXIES: FORMATIONGALAXIES: ISMGALAXIES: NUCLEIGALAXIES: SEYFERThttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present a semi-empirical calibration between the metallicity (Z) of Seyfert 2 active galactic nuclei and the N2 = log([N II]λ6584/H a) emission-line intensity ratio. This calibration was derived through the [OIII]λ5007/[O II]λ3727 versus N2 diagram containing observational data and photoionization model results obtained with the CLOUDY code. The observational sample consists of 463 confirmed Seyfert 2 nuclei (redshift z ≤ 0.4) taken from the Sloan Digital Sky Survey DR7 data set. The obtained Z-N2 relation is valid for the range 0.3 ≤ (Z/Z⊙) ≤ 2.0 that corresponds to -0.7 ≤ (N2) ≤ 0.6. The effects of varying the ionization parameter (U), electron density and the slope of the spectral energy distribution on the Z estimations are of the order of the uncertainty produced by the error measurements of N2. This result indicates the large reliability of our Z -N2 calibration. A relation between U and the [OIII]/[O II] line ratio, almost independent of other nebular parameter, was obtained.Fil: Carvalho, S.P.. Universidade Do Vale Do Paraiba; BrasilFil: Dors, O. L.. Universidade Do Vale Do Paraiba; BrasilFil: Cardaci, Monica Viviana. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Hägele, Guillermo Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Krabbe, Nora Cristina. Universidade Do Vale Do Paraiba; BrasilFil: Pérez Montero, E.. Instituto de Astrofísica de Andalucía; EspañaFil: Monteiro, A.F.. Universidade Do Vale Do Paraiba; BrasilFil: Armah, M.. Universidade Do Vale Do Paraiba; BrasilFil: Freitas Lemes, P.. Universidade Do Vale Do Paraiba; BrasilWiley Blackwell Publishing, Inc2020-06info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/144111Carvalho, S.P.; Dors, O. L.; Cardaci, Monica Viviana; Hägele, Guillermo Federico; Krabbe, Nora Cristina; et al.; Chemical abundances of Seyfert 2 AGNs, II: N2 metallicity calibration based on SDSS; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 492; 4; 6-2020; 5675-56830035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1093/MNRAS/STAA193info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/492/4/5675/5721533?redirectedFrom=fulltextinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:40:37Zoai:ri.conicet.gov.ar:11336/144111instacron: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:34982025-09-29 09:40:37.832CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Chemical abundances of Seyfert 2 AGNs, II: N2 metallicity calibration based on SDSS |
title |
Chemical abundances of Seyfert 2 AGNs, II: N2 metallicity calibration based on SDSS |
spellingShingle |
Chemical abundances of Seyfert 2 AGNs, II: N2 metallicity calibration based on SDSS Carvalho, S.P. GALAXIES: ABUNDANCES GALAXIES: ACTIVE GALAXIES: EVOLUTION GALAXIES: FORMATION GALAXIES: ISM GALAXIES: NUCLEI GALAXIES: SEYFERT |
title_short |
Chemical abundances of Seyfert 2 AGNs, II: N2 metallicity calibration based on SDSS |
title_full |
Chemical abundances of Seyfert 2 AGNs, II: N2 metallicity calibration based on SDSS |
title_fullStr |
Chemical abundances of Seyfert 2 AGNs, II: N2 metallicity calibration based on SDSS |
title_full_unstemmed |
Chemical abundances of Seyfert 2 AGNs, II: N2 metallicity calibration based on SDSS |
title_sort |
Chemical abundances of Seyfert 2 AGNs, II: N2 metallicity calibration based on SDSS |
dc.creator.none.fl_str_mv |
Carvalho, S.P. Dors, O. L. Cardaci, Monica Viviana Hägele, Guillermo Federico Krabbe, Nora Cristina Pérez Montero, E. Monteiro, A.F. Armah, M. Freitas Lemes, P. |
author |
Carvalho, S.P. |
author_facet |
Carvalho, S.P. Dors, O. L. Cardaci, Monica Viviana Hägele, Guillermo Federico Krabbe, Nora Cristina Pérez Montero, E. Monteiro, A.F. Armah, M. Freitas Lemes, P. |
author_role |
author |
author2 |
Dors, O. L. Cardaci, Monica Viviana Hägele, Guillermo Federico Krabbe, Nora Cristina Pérez Montero, E. Monteiro, A.F. Armah, M. Freitas Lemes, P. |
author2_role |
author author author author author author author author |
dc.subject.none.fl_str_mv |
GALAXIES: ABUNDANCES GALAXIES: ACTIVE GALAXIES: EVOLUTION GALAXIES: FORMATION GALAXIES: ISM GALAXIES: NUCLEI GALAXIES: SEYFERT |
topic |
GALAXIES: ABUNDANCES GALAXIES: ACTIVE GALAXIES: EVOLUTION GALAXIES: FORMATION GALAXIES: ISM GALAXIES: NUCLEI GALAXIES: SEYFERT |
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 semi-empirical calibration between the metallicity (Z) of Seyfert 2 active galactic nuclei and the N2 = log([N II]λ6584/H a) emission-line intensity ratio. This calibration was derived through the [OIII]λ5007/[O II]λ3727 versus N2 diagram containing observational data and photoionization model results obtained with the CLOUDY code. The observational sample consists of 463 confirmed Seyfert 2 nuclei (redshift z ≤ 0.4) taken from the Sloan Digital Sky Survey DR7 data set. The obtained Z-N2 relation is valid for the range 0.3 ≤ (Z/Z⊙) ≤ 2.0 that corresponds to -0.7 ≤ (N2) ≤ 0.6. The effects of varying the ionization parameter (U), electron density and the slope of the spectral energy distribution on the Z estimations are of the order of the uncertainty produced by the error measurements of N2. This result indicates the large reliability of our Z -N2 calibration. A relation between U and the [OIII]/[O II] line ratio, almost independent of other nebular parameter, was obtained. Fil: Carvalho, S.P.. Universidade Do Vale Do Paraiba; Brasil Fil: Dors, O. L.. Universidade Do Vale Do Paraiba; Brasil Fil: Cardaci, Monica Viviana. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina Fil: Hägele, Guillermo Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina Fil: Krabbe, Nora Cristina. Universidade Do Vale Do Paraiba; Brasil Fil: Pérez Montero, E.. Instituto de Astrofísica de Andalucía; España Fil: Monteiro, A.F.. Universidade Do Vale Do Paraiba; Brasil Fil: Armah, M.. Universidade Do Vale Do Paraiba; Brasil Fil: Freitas Lemes, P.. Universidade Do Vale Do Paraiba; Brasil |
description |
We present a semi-empirical calibration between the metallicity (Z) of Seyfert 2 active galactic nuclei and the N2 = log([N II]λ6584/H a) emission-line intensity ratio. This calibration was derived through the [OIII]λ5007/[O II]λ3727 versus N2 diagram containing observational data and photoionization model results obtained with the CLOUDY code. The observational sample consists of 463 confirmed Seyfert 2 nuclei (redshift z ≤ 0.4) taken from the Sloan Digital Sky Survey DR7 data set. The obtained Z-N2 relation is valid for the range 0.3 ≤ (Z/Z⊙) ≤ 2.0 that corresponds to -0.7 ≤ (N2) ≤ 0.6. The effects of varying the ionization parameter (U), electron density and the slope of the spectral energy distribution on the Z estimations are of the order of the uncertainty produced by the error measurements of N2. This result indicates the large reliability of our Z -N2 calibration. A relation between U and the [OIII]/[O II] line ratio, almost independent of other nebular parameter, was obtained. |
publishDate |
2020 |
dc.date.none.fl_str_mv |
2020-06 |
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/11336/144111 Carvalho, S.P.; Dors, O. L.; Cardaci, Monica Viviana; Hägele, Guillermo Federico; Krabbe, Nora Cristina; et al.; Chemical abundances of Seyfert 2 AGNs, II: N2 metallicity calibration based on SDSS; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 492; 4; 6-2020; 5675-5683 0035-8711 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/144111 |
identifier_str_mv |
Carvalho, S.P.; Dors, O. L.; Cardaci, Monica Viviana; Hägele, Guillermo Federico; Krabbe, Nora Cristina; et al.; Chemical abundances of Seyfert 2 AGNs, II: N2 metallicity calibration based on SDSS; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 492; 4; 6-2020; 5675-5683 0035-8711 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1093/MNRAS/STAA193 info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/492/4/5675/5721533?redirectedFrom=fulltext |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
Wiley Blackwell Publishing, Inc |
publisher.none.fl_str_mv |
Wiley Blackwell Publishing, Inc |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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1844613285170642944 |
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13.070432 |