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<ri:Resource created="2001-03-23T09:12:42Z" status="active" updated="2025-09-09T14:11:51Z" 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>HST quasar absorption-line key project. VIII.</title><shortName>J/PASP/106/646</shortName><identifier>ivo://CDS.VizieR/J/PASP/106/646</identifier><altIdentifier>doi:10.26093/cds/vizier.61060646</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kirhakos S.</name></creator><creator><name>Sargent W.L.W.</name></creator><creator><name>Schneider D.P.</name></creator><creator><name>Bahcall J.N.</name></creator><creator><name>Jannuzi B.T.,Maoz D.</name></creator><creator><name>Small T.A.</name></creator><date role="Updated">2025-09-09T14:11:51Z</date><date role="Created">2001-03-23T09:12:42Z</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>redshifted</subject><subject>ccd-photometry</subject><description>We present an analysis of CCD images (obtained at the Palomar 1.5m telescope) of more than 100 quasars; many of the objects have been or will be observed in the HST Key Project Quasar Absorption-Line Survey. The data set consists of B, g, and i photometry of 117 quasars and deeper g (limiting magnitude of ~22) images of 101 quasar fields. Positions accurate to ~1", measured with the Space Telescope Science Institute's Astrometric Support Program, are listed for all of the quasars in this study. Positions, magnitudes, and classifications of stars and galaxies located within ~100" of the quasars are given for all of the deep g data. The positions of the stars and galaxies relative to the quasar are accurate to ~0.5". The results presented here can be used to prepare spectroscopic programs designed to obtain redshifts of galaxies in the fields of these quasars.</description><source format="bibcode">1994PASP..106..646K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASP/106/646</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/ApJS/97/1">J/ApJS/97/1 : HST Quasar Absorption Line Key Project. X. 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