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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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 |
work_keys_str_mv |
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