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<ri:Resource created="2024-03-01T09:30:05Z" 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>FITS images of 3C 273 host galaxy</title><shortName>J/A+A/683/L5</shortName><identifier>ivo://CDS.VizieR/J/A+A/683/L5</identifier><altIdentifier>doi:10.26093/cds/vizier.36839005</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ren B.B.</name></creator><creator><name>Fogarty K.</name></creator><creator><name>Debes J.H.</name></creator><creator><name>Meyer E.T.</name></creator><creator><name>Mo Y.</name></creator><creator><name>Mawet D.</name></creator><creator><name>Perrin M.D.,Ogle P.M.</name></creator><creator><name>Sahlmann J.</name></creator><date role="Updated">2024-11-07T20:02:08Z</date><date role="Created">2024-03-01T09:30:05Z</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>galaxies</subject><subject>visible-astronomy</subject><description>The close-in regions of bright quasars' host galaxies have been difficult to image due to the overwhelming light from the quasars. With coronagraphic observations in visible light using the Space Telescope Imaging Spectrograph (STIS) on the Hubble Space Telescope, we removed 3C 273 quasar light using color-matching reference stars. The observations revealed the host galaxy from 60" to 0.2" with nearly full angular coverage. Isophote modeling revealed a new core jet, a core blob, and multiple smaller-scale blobs within 2.5". The blobs could potentially be satellite galaxies or infalling materials towards the central quasar. Using archival STIS data, we constrained the apparent motion of its large scale jets over a 22 yr timeline. 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