Multi-Frequency Databases for AGN Investigation—Results and Perspectives

Active Galactic Nuclei (AGNs) are characterized by emission of radiation over more than 10 orders of magnitude in frequency. Therefore, the execution of extensive surveys of the sky, with different types of detectors, is providing the attractive possibility to identify and to investigate the propert...

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Main Authors: Giovanni La Mura, Marco Berton, Sina Chen, Stefano Ciroi, Enrico Congiu, Valentina Cracco, Michele Frezzato, Piero Rafanelli
Format: Article
Language:English
Published: Frontiers Media S.A. 2017-10-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
Online Access:http://journal.frontiersin.org/article/10.3389/fspas.2017.00025/full
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spelling doaj-5772d05210e54a83845f250b1376e0ce2020-11-24T22:07:30ZengFrontiers Media S.A.Frontiers in Astronomy and Space Sciences2296-987X2017-10-01410.3389/fspas.2017.00025301385Multi-Frequency Databases for AGN Investigation—Results and PerspectivesGiovanni La Mura0Marco Berton1Marco Berton2Sina Chen3Stefano Ciroi4Enrico Congiu5Enrico Congiu6Valentina Cracco7Michele Frezzato8Piero Rafanelli9Department of Physics and Astronomy, University of Padua, Padua, ItalyDepartment of Physics and Astronomy, University of Padua, Padua, ItalyAstronomical Observatory of Brera, National Institute for Astrophysics, Milan, ItalyDepartment of Physics and Astronomy, University of Padua, Padua, ItalyDepartment of Physics and Astronomy, University of Padua, Padua, ItalyDepartment of Physics and Astronomy, University of Padua, Padua, ItalyAstronomical Observatory of Brera, National Institute for Astrophysics, Milan, ItalyDepartment of Physics and Astronomy, University of Padua, Padua, ItalyDepartment of Physics and Astronomy, University of Padua, Padua, ItalyDepartment of Physics and Astronomy, University of Padua, Padua, ItalyActive Galactic Nuclei (AGNs) are characterized by emission of radiation over more than 10 orders of magnitude in frequency. Therefore, the execution of extensive surveys of the sky, with different types of detectors, is providing the attractive possibility to identify and to investigate the properties of AGNs on very large statistical samples. Thanks to the large spectroscopic surveys that allow detailed investigation of many of these sources, we have the opportunity to place new constraints on the nature and evolution of AGNs and to investigate their relations with the host systems. In this contribution we present the results that can be obtained by using a new interactive catalog that we developed to investigate the range of AGN spectral energy distributions (SEDs). We present simple SED models based on data collected in the catalog and discuss their relations with optical spectra obtained by follow up observations. We compare our findings with the expectations based on the AGN Unification Model, and we discuss the perspectives of multi-wavelength approaches to address AGN related processes such as black hole accretion and acceleration of relativistic jets.http://journal.frontiersin.org/article/10.3389/fspas.2017.00025/fullgalaxies: activegalaxies: nucleiquasars: emission linesquasars: supermassive black holesgalaxies: jetscatalogs
collection DOAJ
language English
format Article
sources DOAJ
author Giovanni La Mura
Marco Berton
Marco Berton
Sina Chen
Stefano Ciroi
Enrico Congiu
Enrico Congiu
Valentina Cracco
Michele Frezzato
Piero Rafanelli
spellingShingle Giovanni La Mura
Marco Berton
Marco Berton
Sina Chen
Stefano Ciroi
Enrico Congiu
Enrico Congiu
Valentina Cracco
Michele Frezzato
Piero Rafanelli
Multi-Frequency Databases for AGN Investigation—Results and Perspectives
Frontiers in Astronomy and Space Sciences
galaxies: active
galaxies: nuclei
quasars: emission lines
quasars: supermassive black holes
galaxies: jets
catalogs
author_facet Giovanni La Mura
Marco Berton
Marco Berton
Sina Chen
Stefano Ciroi
Enrico Congiu
Enrico Congiu
Valentina Cracco
Michele Frezzato
Piero Rafanelli
author_sort Giovanni La Mura
title Multi-Frequency Databases for AGN Investigation—Results and Perspectives
title_short Multi-Frequency Databases for AGN Investigation—Results and Perspectives
title_full Multi-Frequency Databases for AGN Investigation—Results and Perspectives
title_fullStr Multi-Frequency Databases for AGN Investigation—Results and Perspectives
title_full_unstemmed Multi-Frequency Databases for AGN Investigation—Results and Perspectives
title_sort multi-frequency databases for agn investigation—results and perspectives
publisher Frontiers Media S.A.
series Frontiers in Astronomy and Space Sciences
issn 2296-987X
publishDate 2017-10-01
description Active Galactic Nuclei (AGNs) are characterized by emission of radiation over more than 10 orders of magnitude in frequency. Therefore, the execution of extensive surveys of the sky, with different types of detectors, is providing the attractive possibility to identify and to investigate the properties of AGNs on very large statistical samples. Thanks to the large spectroscopic surveys that allow detailed investigation of many of these sources, we have the opportunity to place new constraints on the nature and evolution of AGNs and to investigate their relations with the host systems. In this contribution we present the results that can be obtained by using a new interactive catalog that we developed to investigate the range of AGN spectral energy distributions (SEDs). We present simple SED models based on data collected in the catalog and discuss their relations with optical spectra obtained by follow up observations. We compare our findings with the expectations based on the AGN Unification Model, and we discuss the perspectives of multi-wavelength approaches to address AGN related processes such as black hole accretion and acceleration of relativistic jets.
topic galaxies: active
galaxies: nuclei
quasars: emission lines
quasars: supermassive black holes
galaxies: jets
catalogs
url http://journal.frontiersin.org/article/10.3389/fspas.2017.00025/full
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