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<ri:Resource created="2022-08-11T09:14:24Z" 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>WISE view of narrow-line Seyfert 1 galaxies</title><shortName>J/MNRAS/483/2362</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/483/2362</identifier><altIdentifier>doi:10.26093/cds/vizier.74832362</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rakshit S.</name></creator><creator><name>Johnson A.</name></creator><creator><name>Stalin C.S.</name></creator><creator><name>Gandhi P.</name></creator><creator><name>Hoenig S.</name></creator><date role="Updated">2024-08-19T20:15:45Z</date><date role="Created">2022-08-11T09:14:24Z</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>galaxies</subject><subject>photometry</subject><subject>seyfert-galaxies</subject><subject>infrared-photometry</subject><subject>infrared-sources</subject><description>We present the colour and flux variability analysis at 3.4{mu}m (W1 band) and 4.6{mu}m (W2 band) of 492 narrow-line Seyfert 1 (NLSy1) galaxies using archival data from the Wide-field Infrared Survey Explorer (WISE). In the WISE colour-colour, (W1-W2) versus (W2-W3) diagram, ~58 per cent of the NLSy1 galaxies of our sample lie in the region occupied by the blazar category of active galactic nuclei (AGNs). The mean W1-W2 colour of candidate variable NLSy1 galaxies is 0.99+/-0.18mag. The average amplitude of variability is 0.11+/-0.07mag in long term (multiyear) with no difference in variability between W1 and W2 bands. The W1-W2 colour of NLSy1 galaxies is anticorrelated with the relative strength of [OIII] to H{beta}, strongly correlated with continuum luminosity, black hole mass, and Eddington ratio. The long-term amplitude of variability shows weak anticorrelation with the FeII strength, continuum luminosity and Eddington ratio. A positive correlation between colour as well as the amplitude of variability with the radio power at 1.4GHz was found for the radio-detected NLSy1 galaxies. This suggests non-thermal synchrotron contribution to the mid-infrared colour and flux variability in radio-detected NLSy1 galaxies.</description><source format="bibcode">2019MNRAS.483.2362R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/483/2362</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/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/792/30">J/ApJ/792/30 : NEOWISE magnitudes for near-Earth objects (Mainzer+, 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