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<ri:Resource created="2021-11-25T15:13:15Z" 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 MIR variability in gamma-ray Seyfert 1 gal.</title><shortName>J/ApJS/255/10</shortName><identifier>ivo://CDS.VizieR/J/ApJS/255/10</identifier><altIdentifier>doi:10.26093/cds/vizier.22550010</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mao L.</name></creator><creator><name>Yi T.</name></creator><date role="Updated">2022-03-10T07:36:58Z</date><date role="Created">2021-11-25T15:13:15Z</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>seyfert-galaxies</subject><subject>infrared-photometry</subject><subject>redshifted</subject><subject>gamma-ray-astronomy</subject><description>Fermi-LAT's detection of {gamma}-rays from narrow-line Seyfert 1 galaxies (NLS1s) has received increasing attention. Understanding these {gamma}-NLS1s is of interest because they have some properties similar to blazars, which are known to show rapid and large-amplitude variability. Based on the largest sample of {gamma}-NLS1s (25 sources), we carried out a systematic search for rapid mid-infrared (MIR, 3.4 and 4.6{mu}m) variability using the multiepoch data of the Wide-field Infrared Survey Explorer (WISE). We also compared a few variability properties between {gamma}-NLS1s and {gamma}-ray blazars. Our main results are as follows. (1) Thirteen {gamma}-NLS1s showed significant (&gt;3{sigma}) rapid variability in at least one of the two MIR bands. The MIR emission of these sources is dominated by the synchrotron emission of relativistic electrons in the jet. (2) The {gamma}-NLS1s with flat radio spectra are more variable than those not detected in {gamma}-rays. (3) The {gamma}-NLS1s tend to show smaller amplitude of variability as well as lower duty cycle relative to {gamma}-ray blazars. (4) The {gamma}-NLS1s tend to show a trend of bluer-when-brighter on both intraday and long timescales, similar to {gamma}-ray blazars. (5) The {gamma}-NLS1s that are more variable on long timescales have larger amplitudes of variability and higher duty cycles on intraday timescales. (6) In the majority of cases, the {gamma}-NLS1s fall in the WISE Gamma-ray Blazar Strip (WGS). However, we noted migrations outside of the WGS due to significant variability.</description><source format="bibcode">2021ApJS..255...10M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/255/10</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/311">II/311 : WISE All-Sky Data Release (Cutri+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</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/ApJS/166/470">J/ApJS/166/470 : SDSS-Spitzer type I QSOs IR photometry (Richards+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/487/475">J/A+A/487/475 : X-ray variability of AGNs in Lockman Hole (Papadakis+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/716/530">J/ApJ/716/530 : Mid-IR variability from the SDWFS (Kozlowski+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/194/29">J/ApJS/194/29 : Observations of blazars at 15GHz (Richards+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/748/68">J/ApJ/748/68 : WISE IR colors of gamma-ray blazars (D'Abrusco+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/748/124">J/ApJ/748/124 : AGN X-ray variability in the 4Ms catalog (Young+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/438/3058">J/MNRAS/438/3058 : 15GHz variability of {gamma}-ray blazars (Richards+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/439/690">J/MNRAS/439/690 : Optical/{gamma}-ray variability in blazars (Hovatta+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/792/30">J/ApJ/792/30 : NEOWISE magnitudes for near-Earth objects (Mainzer+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/795/58">J/ApJ/795/58 : 1H 0323+342 rest frame opt. spectrum with GHAO (Leon+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/573/A76">J/A+A/573/A76 : Multifrequency study of NL Seyfert 1 galaxies (Jarvela+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/810/14">J/ApJ/810/14 : Third catalog of LAT-detected AGNs (3LAC) (Ackermann+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/817/119">J/ApJ/817/119 : Spitzer variability survey of Bootes field (Kozlowski+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/224/26">J/ApJS/224/26 : SEDs of Roma BZCAT blazars (Mao+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/12">J/AJ/152/12 : MOJAVE. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Name of the {gamma}-narrow-line Seyfert 1</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="24*">char</dataType></column><column><name>Nep</name><description>[1/17] Serial number of observational epoch</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>l_V3.4</name><description>Limit flag on V3.4</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>V3.4</name><description>[0/100] WISE 3.4um variability index</description><ucd>meta.code;meta.code.multip</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_V4.6</name><description>Limit flag on V4.6</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>V4.6</name><description>[0/100] WISE 4.6um variability index</description><ucd>meta.code;meta.code.multip</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>delta3.4</name><description>[0] {Delta} metric for WISE 3.4um (always "0")</description><ucd>stat.variance</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>l_delta4.6</name><description>Limit flag for delta4.6</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>delta4.6</name><description>[0] {Delta} metric for WISE 4.6um (always "0")</description><ucd>stat.variance</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>l_sigma3.4</name><description>Limit flag for sigma3.4</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>sigma3.4</name><description>[3/27]? Significance level of W1 band variability</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>l_sigma4.6</name><description>Limit flag for sigma4.6</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>sigma4.6</name><description>[3/19]? Significance level of W2 band variability</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Note</name><description>Note (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column></table></schema></tableset></ri:Resource>