Dataciencia

Colección SciELO Chile

X-ray Properties of Two Complementary Samples of Intermediate Seyfert Galaxies

Indexado

WoS	WOS:001276795100001
Scopus	SCOPUS_ID:85187268583

DOI

10.3390/UNIVERSE10020069

Año

2024

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

We present the X-ray spectral analysis of two complementary sets of intermediate Seyfert galaxies (ISs). Analyzing X-ray data, we estimate the hydrogen abundance (Formula presented.) and test its connection with the [O III] luminosity acquired from optical observations. The results confirm the conclusions drawn in a previous study concerning the lack of a direct correlation between the obscuration measure ((Formula presented.)) and the intrinsic characteristics of the active nuclei ([O III] luminosity). Instead, we validate the existence of a correlation between the Seyfert type and the (Formula presented.) parameter, employing a separation threshold of approximately (Formula presented.) atoms (Formula presented.). Simultaneously, our findings align with prior research, corroborating the relationship between X-ray luminosity and the [O III] luminosity.

Revista

Revista	ISSN
Universe	2218-1997

Métricas Externas

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Disciplinas de Investigación

WOS
Astronomy & Astrophysics
Physics, Particles & Fields

Scopus
Sin Disciplinas

SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional

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Autores - Afiliación

Ord.	Autor	Género	Institución - País
1	Dalla Barba, Benedetta	-	Università degli Studi dell'Insubria - Italia Istituto Nazionale Di Astrofisica, Rome - Italia Univ Insubria - Italia Ist Nazl Astrofis INAF - Italia
2	Foschini, L.	Hombre	Istituto Nazionale Di Astrofisica, Rome - Italia Ist Nazl Astrofis INAF - Italia
3	Berton, M.	Hombre	European Southern Observatory Santiago - Chile Observatorio Europeo Austral - Chile
4	Crepaldi, Luca	-	Università degli Studi di Padova - Italia Univ Padua - Italia
5	Vietri, A.	-	Università degli Studi di Padova - Italia Univ Padua - Italia

Muestra la afiliación y género (detectado) para los co-autores de la publicación.

Financiamiento

Fuente
Universidad Nacional Autónoma de México
University of Illinois at Urbana-Champaign
Ohio State University
Yale University
University of Toronto
University of Arizona
Harvard University
Johns Hopkins University
New Mexico State University
Pennsylvania State University
University of Utah
University of Virginia
Yunnan University
Center for High-Performance Computing at the University of Utah
Carnegie Institution for Science
Max-Planck-Institut fur Astronomie (MPIA Heidelberg)
University of Colorado Boulder
Smithsonian Astrophysical Observatory
Nanjing University
Heidelberg University
Leibniz-Institut fur Astrophysik Potsdam (AIP)
Space Telescope Science Institute (STScI)
Stellar Astrophysics Participation Group
National Astronomical Observatories of China (NAOC)
L'Ecole polytechnique federale de Lausanne (EPFL)
Gotham Participation Group
Max-Planck Institut fur Extraterrestrische Physik (MPE)
Chilean National Time Allocation Committee (CNTAC) ratified researchers

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos

Agradecimiento
SDSS acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. The SDSS web site is www.sdss.org.SDSS is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration, including the Carnegie Institution for Science, Chilean National Time Allocation Committee (CNTAC) ratified researchers, the Gotham Participation Group, Harvard University, Heidelberg University, The Johns Hopkins University, L'Ecole polytechnique federale de Lausanne (EPFL), Leibniz-Institut fur Astrophysik Potsdam (AIP), Max-Planck-Institut fur Astronomie (MPIA Heidelberg), Max-PlanckInstitut fur Extraterrestrische Physik (MPE), Nanjing University, National Astronomical Observatories of China (NAOC), New Mexico State University, The Ohio State University, Pennsylvania State University, Smithsonian Astrophysical Observatory, Space Telescope Science Institute (STScI), the Stellar Astrophysics Participation Group, Universidad Nacional Autonoma de Mexico, University of Arizona, University of Colorado Boulder, University of Illinois at Urbana-Champaign, University of Toronto, University of Utah, University of Virginia, Yale University, and Yunnan University. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France.

Agradecimiento

SDSS acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. The SDSS web site is www.sdss.org.SDSS is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration, including the Carnegie Institution for Science, Chilean National Time Allocation Committee (CNTAC) ratified researchers, the Gotham Participation Group, Harvard University, Heidelberg University, The Johns Hopkins University, L'Ecole polytechnique federale de Lausanne (EPFL), Leibniz-Institut fur Astrophysik Potsdam (AIP), Max-Planck-Institut fur Astronomie (MPIA Heidelberg), Max-PlanckInstitut fur Extraterrestrische Physik (MPE), Nanjing University, National Astronomical Observatories of China (NAOC), New Mexico State University, The Ohio State University, Pennsylvania State University, Smithsonian Astrophysical Observatory, Space Telescope Science Institute (STScI), the Stellar Astrophysics Participation Group, Universidad Nacional Autonoma de Mexico, University of Arizona, University of Colorado Boulder, University of Illinois at Urbana-Champaign, University of Toronto, University of Utah, University of Virginia, Yale University, and Yunnan University. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France.