Uso de las líneas de neón en el estudio de las componentes presentes en SEDs de AGNs radio silenciosos

ilustraciones a color, diagramas, fotografías

Autores:
Bernal Salinas, Jonhatan Herney
Tipo de recurso:
Fecha de publicación:
2024
Institución:
Universidad Nacional de Colombia
Repositorio:
Universidad Nacional de Colombia
Idioma:
spa
OAI Identifier:
oai:repositorio.unal.edu.co:unal/86517
Acceso en línea:
https://repositorio.unal.edu.co/handle/unal/86517
https://repositorio.unal.edu.co/
Palabra clave:
520 - Astronomía y ciencias afines
Núcleos galácticos activos
Distribución de energía espectral
Active galactic nuclei
Spectral energy distribution
Técnicas: fotométrica
Análisis de datos
Métodos: estadístico
Bases de datos astronómicos: varios
Galaxias: fotometría
Galaxias: Seyfert
Data analysis
Methods: statistical
Techniques: photometric
Astronomical data bases: miscellaneous
Galaxies: photometry
Galaxies: Seyfert
Observatorio virtual
Virtual observatory
Rights
openAccess
License
Atribución-NoComercial 4.0 Internacional
id UNACIONAL2_d6a8ccfb387367e25ec0e4b2585a4742
oai_identifier_str oai:repositorio.unal.edu.co:unal/86517
network_acronym_str UNACIONAL2
network_name_str Universidad Nacional de Colombia
repository_id_str
dc.title.spa.fl_str_mv Uso de las líneas de neón en el estudio de las componentes presentes en SEDs de AGNs radio silenciosos
dc.title.translated.eng.fl_str_mv Use of neon lines in the study of the components present in SEDs of radio silent AGNs
title Uso de las líneas de neón en el estudio de las componentes presentes en SEDs de AGNs radio silenciosos
spellingShingle Uso de las líneas de neón en el estudio de las componentes presentes en SEDs de AGNs radio silenciosos
520 - Astronomía y ciencias afines
Núcleos galácticos activos
Distribución de energía espectral
Active galactic nuclei
Spectral energy distribution
Técnicas: fotométrica
Análisis de datos
Métodos: estadístico
Bases de datos astronómicos: varios
Galaxias: fotometría
Galaxias: Seyfert
Data analysis
Methods: statistical
Techniques: photometric
Astronomical data bases: miscellaneous
Galaxies: photometry
Galaxies: Seyfert
Observatorio virtual
Virtual observatory
title_short Uso de las líneas de neón en el estudio de las componentes presentes en SEDs de AGNs radio silenciosos
title_full Uso de las líneas de neón en el estudio de las componentes presentes en SEDs de AGNs radio silenciosos
title_fullStr Uso de las líneas de neón en el estudio de las componentes presentes en SEDs de AGNs radio silenciosos
title_full_unstemmed Uso de las líneas de neón en el estudio de las componentes presentes en SEDs de AGNs radio silenciosos
title_sort Uso de las líneas de neón en el estudio de las componentes presentes en SEDs de AGNs radio silenciosos
dc.creator.fl_str_mv Bernal Salinas, Jonhatan Herney
dc.contributor.advisor.none.fl_str_mv Higuera Garzón, Mario Armando
Ramos Padilla, Andres Felipe
dc.contributor.author.none.fl_str_mv Bernal Salinas, Jonhatan Herney
dc.contributor.researchgroup.spa.fl_str_mv Astronomía, Astrofísica y Cosmologia
dc.contributor.orcid.spa.fl_str_mv Bernal-Salinas, Jonhatan-H [0000000178180687]
dc.contributor.cvlac.spa.fl_str_mv Bernal-Salinas, Jonhatan-H [0002207112]
dc.subject.ddc.spa.fl_str_mv 520 - Astronomía y ciencias afines
topic 520 - Astronomía y ciencias afines
Núcleos galácticos activos
Distribución de energía espectral
Active galactic nuclei
Spectral energy distribution
Técnicas: fotométrica
Análisis de datos
Métodos: estadístico
Bases de datos astronómicos: varios
Galaxias: fotometría
Galaxias: Seyfert
Data analysis
Methods: statistical
Techniques: photometric
Astronomical data bases: miscellaneous
Galaxies: photometry
Galaxies: Seyfert
Observatorio virtual
Virtual observatory
dc.subject.lemb.spa.fl_str_mv Núcleos galácticos activos
Distribución de energía espectral
dc.subject.lemb.eng.fl_str_mv Active galactic nuclei
Spectral energy distribution
dc.subject.proposal.spa.fl_str_mv Técnicas: fotométrica
Análisis de datos
Métodos: estadístico
Bases de datos astronómicos: varios
Galaxias: fotometría
dc.subject.proposal.eng.fl_str_mv Galaxias: Seyfert
Data analysis
Methods: statistical
Techniques: photometric
Astronomical data bases: miscellaneous
Galaxies: photometry
Galaxies: Seyfert
dc.subject.wikidata.spa.fl_str_mv Observatorio virtual
dc.subject.wikidata.eng.fl_str_mv Virtual observatory
description ilustraciones a color, diagramas, fotografías
publishDate 2024
dc.date.accessioned.none.fl_str_mv 2024-07-17T14:25:47Z
dc.date.available.none.fl_str_mv 2024-07-17T14:25:47Z
dc.date.issued.none.fl_str_mv 2024
dc.type.spa.fl_str_mv Trabajo de grado - Maestría
dc.type.driver.spa.fl_str_mv info:eu-repo/semantics/masterThesis
dc.type.version.spa.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.coarversion.spa.fl_str_mv http://purl.org/coar/version/c_970fb48d4fbd8a85
dc.type.content.spa.fl_str_mv Text
dc.type.redcol.spa.fl_str_mv http://purl.org/redcol/resource_type/TM
status_str publishedVersion
dc.identifier.uri.none.fl_str_mv https://repositorio.unal.edu.co/handle/unal/86517
dc.identifier.instname.spa.fl_str_mv Universidad Nacional de Colombia
dc.identifier.reponame.spa.fl_str_mv Repositorio Institucional Universidad Nacional de Colombia
dc.identifier.repourl.spa.fl_str_mv https://repositorio.unal.edu.co/
url https://repositorio.unal.edu.co/handle/unal/86517
https://repositorio.unal.edu.co/
identifier_str_mv Universidad Nacional de Colombia
Repositorio Institucional Universidad Nacional de Colombia
dc.language.iso.spa.fl_str_mv spa
language spa
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spelling Atribución-NoComercial 4.0 Internacionalhttp://creativecommons.org/licenses/by-nc/4.0/info:eu-repo/semantics/openAccesshttp://purl.org/coar/access_right/c_abf2Higuera Garzón, Mario Armandoa12f46c538561a02747286f0cf279f63600Ramos Padilla, Andres Felipe468b4a489e0776f68c760600371ac75f600Bernal Salinas, Jonhatan Herney813db54dd1fbeda21199ba157408bb33Astronomía, Astrofísica y CosmologiaBernal-Salinas, Jonhatan-H [0000000178180687]Bernal-Salinas, Jonhatan-H [0002207112]2024-07-17T14:25:47Z2024-07-17T14:25:47Z2024https://repositorio.unal.edu.co/handle/unal/86517Universidad Nacional de ColombiaRepositorio Institucional Universidad Nacional de Colombiahttps://repositorio.unal.edu.co/ilustraciones a color, diagramas, fotografíasLa línea de emisión de [Ne V] en infrarrojo, ha mostrado ser un relevante indicador de la actividad de un AGN por su alto potencial de ionización. Así mismo el análisis de la razón [Ne V]/[Ne II], ha permitido distinguir entre ambientes estelares y AGNs. Con base en lo anterior, este trabajo buscó verificar a partir de una muestra de AGNs radio silenciosos (galaxias Seyfert y QSO) tomada de la base de datos del CDS y su servicio SIMBAD, que las estimaciones de la fracción del AGN (fAGN ) provenientes de CIGALE, coinciden con los trazadores de líneas de Neón en el infrarrojo. De las tablas fotométricas del NED, se filtraron las galaxias que contienen datos en las líneas [Ne II]12.8µm, [Ne V]14.3µm y [Ne III]15.5µm. Se compararon las razones de [Ne V]/[Ne II], [Ne V]/[Ne III] y [Ne III]/[Ne II] con diferentes propiedades físicas estimados del modelamiento y ajuste de las distribuciones espectrales de energía (SEDs). Se encontró que la correlación entre fAGN y la razón [Ne V]/[Ne II] es fuerte en las galaxias clasificadas como Seyfert 1 en la muestra inicial, pero débil en las clasificadas como Seyfert 2. Este mismo patrón se presenta al clasificar las galaxias por su ángulo de visión (i) al toroide y la luminosidad del disco del AGN (Ldisc AGN ) (Texto tomado de la fuente).The emision line of [Ne V] in infrared has proven to be a relevant indicator of the activity of an AGN due to its high ionization potential. Likewise, the analysis of the ratio [Ne V]/[Ne II], has allowed to distinguish between stellar environments and AGNs. Based on the above, this work sought to verify from a sample of radio quiet AGNs (Seyfert galaxies and QSOs) taken from the CDS database and its service SIMBAD, that the estimates of the AGN fraction (fAGN ) coming from CIGALE, coincide with the Neon line tracers in the infrared. From the NED photometric tables, galaxies containing data on the lines [Ne II]12.8µm, [Ne V]14.3µm and [Ne III]15.5µm were filtered. [Ne V]/[Ne II], [Ne V]/[Ne III] and [Ne III]/[Ne II] ratios were compared with different physical parameters estimated from modeling and fitting of spectral energy dsitributions (SEDs). It was found that the correlation between fAGN and the [Ne V]/[Ne II] ratio is strong in galaxies classified as Seyfert 1 in the initial sample, but weak in those classified as Seyfert 2. This same pattern occurs by classifying galaxies by their viewing angle (i) to the torus and the luminosity of the AGN disk (Ldisc AGN ).MaestríaMagíster en Ciencias - AstronomíaNúcleos Activos de Galaxia87 páginasapplication/pdfspaUniversidad Nacional de ColombiaBogotá - Ciencias - Maestría en Ciencias - AstronomíaFacultad de CienciasBogotá, ColombiaUniversidad Nacional de Colombia - Sede Bogotá520 - Astronomía y ciencias afinesNúcleos galácticos activosDistribución de energía espectralActive galactic nucleiSpectral energy distributionTécnicas: fotométricaAnálisis de datosMétodos: estadísticoBases de datos astronómicos: variosGalaxias: fotometríaGalaxias: SeyfertData analysisMethods: statisticalTechniques: photometricAstronomical data bases: miscellaneousGalaxies: photometryGalaxies: SeyfertObservatorio virtualVirtual observatoryUso de las líneas de neón en el estudio de las componentes presentes en SEDs de AGNs radio silenciososUse of neon lines in the study of the components present in SEDs of radio silent AGNsTrabajo de grado - Maestríainfo:eu-repo/semantics/masterThesisinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/version/c_970fb48d4fbd8a85Texthttp://purl.org/redcol/resource_type/TMAbel, N. & Satyapal, S.: , 2008; [Ne V] Emission in Optically Classified Starbursts; The Astrophysical Journal; 678 (2): 686–692; doi:10.1086/529013; URL http://dx.doi.org/10.1086/529013.Andrae, R.; Schulze-Hartung, T. & Melchior, P.: , 2010; Dos and don’ts of reduced chi-squared.Antonucci, R.: , 1993; Unified models for active galactic nuclei and quasars; Annual Rev. 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