Ultraviolet/Optical Emission of the Ionized Gas in AGN: Diagnostics of the Ionizing Source and Gas Properties

Spectroscopic studies of active galactic nuclei (AGN) are powerful means of probing the physical properties of the ionized gas within them. In particular, near future observational facilities, such as the James Webb Space Telescope (JWST), will allow detailed statistical studies of rest-frame ultrav...

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Main Authors: Anna Feltre, Stephane Charlot, Marco Mignoli, Angela Bongiorno, Francesco Calura, Jacopo Chevallard, Emma Curtis-Lake, Roberto Gilli, Adele Plat
Format: Article
Language:English
Published: Frontiers Media S.A. 2017-11-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
Online Access:http://journal.frontiersin.org/article/10.3389/fspas.2017.00032/full
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spelling doaj-8b95604e87dd46a89ab43a02d9f635152020-11-24T22:48:03ZengFrontiers Media S.A.Frontiers in Astronomy and Space Sciences2296-987X2017-11-01410.3389/fspas.2017.00032307206Ultraviolet/Optical Emission of the Ionized Gas in AGN: Diagnostics of the Ionizing Source and Gas PropertiesAnna Feltre0Anna Feltre1Stephane Charlot2Marco Mignoli3Angela Bongiorno4Francesco Calura5Jacopo Chevallard6Emma Curtis-Lake7Roberto Gilli8Adele Plat9Univ Lyon, Univ Lyon1, Ens de Lyon, Centre National de la Recherche Scientifique, Centre de Recherche Astrophysique de Lyon UMR5574, Saint-Genis-Laval, FranceSorbonne Universités, UPMC-Centre National de la Recherche Scientifique, UMR7095, Institut d'Astrophysique de Paris, Paris, FranceSorbonne Universités, UPMC-Centre National de la Recherche Scientifique, UMR7095, Institut d'Astrophysique de Paris, Paris, FranceINAF-Osservatorio Astronomico di Bologna, Bologna, ItalyINAF-Osservatorio Astronomico di Roma, Monteporzio Catone, ItalyINAF-Osservatorio Astronomico di Bologna, Bologna, ItalyScientific Support Office, Directorate of Science and Robotic Exploration, European Space Research and Technology Centre (ESTEC), European Space Agency (ESA), Noordwijk, NetherlandsSorbonne Universités, UPMC-Centre National de la Recherche Scientifique, UMR7095, Institut d'Astrophysique de Paris, Paris, FranceINAF-Osservatorio Astronomico di Bologna, Bologna, ItalySorbonne Universités, UPMC-Centre National de la Recherche Scientifique, UMR7095, Institut d'Astrophysique de Paris, Paris, FranceSpectroscopic studies of active galactic nuclei (AGN) are powerful means of probing the physical properties of the ionized gas within them. In particular, near future observational facilities, such as the James Webb Space Telescope (JWST), will allow detailed statistical studies of rest-frame ultraviolet and optical spectral features of the very distant AGN with unprecedented accuracy. In this proceedings, we discuss the various ways of exploiting new dedicated photoionization models of the narrow-line emitting regions (NLR) of AGN for the interpretation of forthcoming revolutionary datasets.http://journal.frontiersin.org/article/10.3389/fspas.2017.00032/fullactive galaxiesemission linesultravioletspectral modelsspectroscopy
collection DOAJ
language English
format Article
sources DOAJ
author Anna Feltre
Anna Feltre
Stephane Charlot
Marco Mignoli
Angela Bongiorno
Francesco Calura
Jacopo Chevallard
Emma Curtis-Lake
Roberto Gilli
Adele Plat
spellingShingle Anna Feltre
Anna Feltre
Stephane Charlot
Marco Mignoli
Angela Bongiorno
Francesco Calura
Jacopo Chevallard
Emma Curtis-Lake
Roberto Gilli
Adele Plat
Ultraviolet/Optical Emission of the Ionized Gas in AGN: Diagnostics of the Ionizing Source and Gas Properties
Frontiers in Astronomy and Space Sciences
active galaxies
emission lines
ultraviolet
spectral models
spectroscopy
author_facet Anna Feltre
Anna Feltre
Stephane Charlot
Marco Mignoli
Angela Bongiorno
Francesco Calura
Jacopo Chevallard
Emma Curtis-Lake
Roberto Gilli
Adele Plat
author_sort Anna Feltre
title Ultraviolet/Optical Emission of the Ionized Gas in AGN: Diagnostics of the Ionizing Source and Gas Properties
title_short Ultraviolet/Optical Emission of the Ionized Gas in AGN: Diagnostics of the Ionizing Source and Gas Properties
title_full Ultraviolet/Optical Emission of the Ionized Gas in AGN: Diagnostics of the Ionizing Source and Gas Properties
title_fullStr Ultraviolet/Optical Emission of the Ionized Gas in AGN: Diagnostics of the Ionizing Source and Gas Properties
title_full_unstemmed Ultraviolet/Optical Emission of the Ionized Gas in AGN: Diagnostics of the Ionizing Source and Gas Properties
title_sort ultraviolet/optical emission of the ionized gas in agn: diagnostics of the ionizing source and gas properties
publisher Frontiers Media S.A.
series Frontiers in Astronomy and Space Sciences
issn 2296-987X
publishDate 2017-11-01
description Spectroscopic studies of active galactic nuclei (AGN) are powerful means of probing the physical properties of the ionized gas within them. In particular, near future observational facilities, such as the James Webb Space Telescope (JWST), will allow detailed statistical studies of rest-frame ultraviolet and optical spectral features of the very distant AGN with unprecedented accuracy. In this proceedings, we discuss the various ways of exploiting new dedicated photoionization models of the narrow-line emitting regions (NLR) of AGN for the interpretation of forthcoming revolutionary datasets.
topic active galaxies
emission lines
ultraviolet
spectral models
spectroscopy
url http://journal.frontiersin.org/article/10.3389/fspas.2017.00032/full
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