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<ri:Resource created="2025-11-05T07:55:16Z" status="active" updated="2026-03-02T06:25:50Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>VLT/MUSE images of 5 nearby galaxies</title><shortName>J/A+A/703/A63</shortName><identifier>ivo://CDS.VizieR/J/A+A/703/A63</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Finlez C.</name></creator><creator><name>Treister E.</name></creator><creator><name>Bauer F.</name></creator><creator><name>Koss M.</name></creator><creator><name>Keel W.</name></creator><creator><name>Maksym W.P.</name></creator><creator><name>Sartori L.,Venturi G.</name></creator><creator><name>Ricci C.</name></creator><creator><name>Nagar N.</name></creator><creator><name>Riesco C.</name></creator><creator><name>Diaz Y.</name></creator><creator><name>Parra M.</name></creator><date role="Updated">2026-03-02T06:25:50Z</date><date role="Created">2025-11-05T07:55:16Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>active-galactic-nuclei</subject><subject>galaxies</subject><subject>visible-astronomy</subject><subject>seyfert-galaxies</subject><description>We present a comprehensive study of five nearby active galaxies featuring large (tens of kiloparsecs) extended emission-line regions (EELRs). The study is based on large-format, integral-field spectroscopic observations conducted with the Multi Unit Spectroscopic Explorer (MUSE) at the Very Large Telescope (VLT). The spatially resolved kinematics of the ionized gas and stellar components show signs of rotation, bi-conical outflows, and complex behavior likely associated with past interactions. An analysis of the physical conditions of the EELRs indicates that in these systems the active galactic nucleus (AGN) is the primary ionization source. Using radiative transfer simulations, we compared the ionization state across the EELRs to estimate the required AGN bolometric luminosities at different radial distances. Then, considering the projected light travel time, we reconstructed the inferred AGN luminosity curves. We find that all sources are consistent with a fading trend in intrinsic AGN luminosity by 0.2-3dex over timescales of 40000 to 80000-years, with a time dependence consistent with previous studies of fading AGNs. These results support the hypothesis that most AGNs undergo significant fluctuations in their accretion rates over multiple timescales ranging from 10000 to 1000000-years, as proposed by existing theoretical models. 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