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<ri:Resource created="2020-08-24T08:54:51Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Opt-NIR light curve of the quasar 3C 273</title><shortName>J/AJ/159/259</shortName><identifier>ivo://CDS.VizieR/J/AJ/159/259</identifier><altIdentifier>doi:10.26093/cds/vizier.51590259</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sobrino Figaredo C.</name></creator><creator><name>Haas M.</name></creator><creator><name>Ramolla M.</name></creator><creator><name>Chini R.</name></creator><creator><name>Blex J.</name></creator><creator><name>Hodapp K.W.,Murphy M.</name></creator><creator><name>Kollatschny W.</name></creator><creator><name>Chelouche D.</name></creator><creator><name>Kaspi S.</name></creator><date role="Updated">2021-04-30T14:16:15Z</date><date role="Created">2020-08-24T08:54:51Z</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>quasars</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>We monitored the z=0.158 quasar 3C273 between 2015 and 2019 in the optical (BVrz) and near-infrared (JHK) with the aim to perform dust reverberation mapping. Accounting for host galaxy and accretion disk contributions, we obtained pure dust light curves in JHK. Cross correlations between the V-band and the dust light curves yield an average rest-frame delay for the hot dust of {tau}cent~410days. This is a factor of two shorter than that expected from the the dust ring radius R_x_~900lt-day reported from interferometric studies. The dust covering factor (CF) is about 8%, much smaller than that predicted from the half covering angle of 45{deg} found for active galactic nuclei (AGNs). We analyze the asymmetric shape of the correlation functions and explore whether an inclined biconical bowl-shaped dust torus geometry could bring these findings ({tau}cent, Rx and CF) into a consistent picture. The hot varying dust emission originates from the edge of the bowl rim with a small covering angle 40{deg}&lt;{theta}&lt;45{deg}, and we see only the near side of the biconus. Such a dust gloriole with R_x_= 900{+/-}200lt-day and an inclination 12{deg} matches the data remarkably well. Comparing the results of 3C273 with literature for less luminous AGN, we find a lag-luminosity relation {tau}{prop}L{alpha} with {alpha}=0.33-0.40, flatter than the widely adopted relation with {alpha}~0.5. We address several explanations for the new lag-luminosity relation.</description><source format="bibcode">2020AJ....159..259S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/159/259</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/349">II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/506/569">J/A+A/506/569 : BEST-II periodic variables in CoRoT LRa02 field (Kabath+,2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AN/333/706">J/AN/333/706 : Bochum survey of the southern Galactic disk (Haas+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/756/73">J/ApJ/756/73 : gri light curves of low-luminosity AGN NGC 4395 (Edri+, 2012)</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/A+A/561/L8">J/A+A/561/L8 : BRJK photometry of Seyfert galaxy WPVS48 (Pozo Nunez+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/213/26">J/ApJS/213/26 : Optical light curves of PHL1811 and 3C273 (Fan+, 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/825/126">J/ApJ/825/126 : SEAMBHs. 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