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<ri:Resource created="2024-11-08T16:45:42Z" status="active" updated="2025-06-13T15:25:00Z" 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>Changing-look AGN. I. Main sequence transition</title><shortName>J/ApJS/272/13</shortName><identifier>ivo://CDS.VizieR/J/ApJS/272/13</identifier><altIdentifier>doi:10.26093/cds/vizier.22720013</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Panda S.</name></creator><creator><name>Sniegowska M.</name></creator><date role="Updated">2025-02-13T20:13:51Z</date><date role="Created">2024-11-08T16:45:42Z</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>visible-astronomy</subject><subject>spectroscopy</subject><subject>redshifted</subject><subject>line-intensities</subject><subject>black-holes</subject><description>This paper is the first in a series of papers that prepare and analyze spectral and other properties for a database of already-discovered changing-look active galactic nuclei (CL AGNs). Here we focus on the spectral fitting and analysis of broad emission lines in a sample of 93 CL AGNs collected from the literature with existing Sloan Digital Sky Survey (SDSS)/Baryon Oscillation Spectroscopic Survey (BOSS)/extended-BOSS spectroscopy where the H{beta} emission-line profile does not completely disappear in any epochs. Additionally, we have gathered older/newer spectral epochs from all the available SDSS data releases to make the database more complete. We use PyQSOFit and perform a homogeneous spectral decomposition of all of our SDSS spectra and tabulate the AGN continuum and emission-line properties per epoch per source, chronologically. This further allows us to categorize the sources in our sample as Turn-On or Turn-Off and subsequently check for repeated occurrences of such phases. We then estimate the black hole mass (M_BH_) and the Eddington ratio ({lambda}_Edd_) per epoch per source where the required parameters are available and well estimated. We demonstrate the movement of the source in the M_BH_-{lambda}_Edd_ plane, allowing us to check for systematic changes in the source's fundamental properties. We then track their transition along the optical plane of the Eigenvector 1 schema and categorize sources that either stay within the same population (A or B) or make an interpopulation movement as a function of spectral epoch. We also test the Balmer decrement (H{alpha}/H{beta}) of a subset of our sample of CL AGNs as a function of time and AGN luminosity.</description><source format="bibcode">2024ApJS..272...13P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/272/13</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/V/154">V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/289">VII/289 : SDSS quasar catalog, sixteenth data release (DR16Q) (Lyke+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/613/682">J/ApJ/613/682 : AGN central masses (Peterson+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/422/925">J/A+A/422/925 : Profile variability in lines of NGC 5548 (Shapovalova+ 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/166/470">J/ApJS/166/470 : SDSS-Spitzer type I QSOs IR photometry (Richards+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/166/128">J/ApJS/166/128 : Narrow line Seyfert 1 galaxies from SDSS-DR3 (Zhou+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/383/581">J/MNRAS/383/581 : Broad-line Balmer decrements in blue AGN (Dong+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/486/99">J/A+A/486/99 : Long-term sp. variability of NGC 4151 (Shapovalova+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/189/15">J/ApJS/189/15 : FeII emission in a sample of AGN spectra (Kovacevic+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/788/159">J/ApJ/788/159 : 17 Seyfert 1 galaxies light curves (Koshida+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/217/26">J/ApJS/217/26 : Lick AGN monitoring 2011: light curves (Barth+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/806/128">J/ApJ/806/128 : Space telescope RM project. 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