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<ri:Resource created="2023-11-15T13:01:12Z" status="active" updated="2025-05-19T09:50:00Z" 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-state quasars with CRTS</title><shortName>J/MNRAS/491/4925</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/491/4925</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Graham M.J.</name></creator><creator><name>Ross N.P.</name></creator><creator><name>Stern D.</name></creator><creator><name>Drake A.J.</name></creator><creator><name>McKernan B.</name></creator><creator><name>Ford K.E.S.,Djorgovski S.G.</name></creator><creator><name>Mahabal A.A.</name></creator><creator><name>Glikman E.</name></creator><creator><name>Larson S.</name></creator><creator><name>Christensen E.</name></creator><date role="Updated">2024-03-01T14:34:30Z</date><date role="Created">2023-11-15T13:01:12Z</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>black-holes</subject><subject>quasars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>infrared-photometry</subject><description>We present the results of a systematic search for quasars in the Catalina Real-time Transient Survey exhibiting both strong photometric variability and spectroscopic variability over a decadal baseline. We identify 111 sources with specific patterns of optical and mid-infrared photometric behaviour and a defined spectroscopic change. These 'changing-state' quasars (CSQs) form a higher luminosity sample to complement existing sets of 'changing-look' AGNs and quasars in the literature. The CSQs (by selection) exhibit larger photometric variability than the changing-look quasars (CLQs). The spectroscopic variability is marginally stronger in the CSQs than CLQs as defined by the change in H{beta}/[OIII] ratio. We find 48 sources with declining H{beta} flux and 63 sources with increasing H{beta} flux, and discover 8 sources with z&gt;0.8, further extending the redshift arm. Our CSQ sample compares to the literature CLQ objects in similar distributions of H{beta} flux ratios and differential Eddington ratios between high (bright) and low (dim) states. Taken as a whole, we find that this population of extreme varying quasars is associated with changes in the Eddington ratio and the time-scales imply cooling/heating fronts propagating through the disc.</description><source format="bibcode">2020MNRAS.491.4925G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/491/4925</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/J/ApJ/696/870">J/ApJ/696/870 : Catalina Real-time Transient Survey (CRTS)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/154">V/154 : Sloan Digital Sky Surveys (SDSS), 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