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<ri:Resource created="2003-04-26T17:39:40Z" 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>BRI photometry of 3 QSO fields</title><shortName>J/AJ/123/2206</shortName><identifier>ivo://CDS.VizieR/J/AJ/123/2206</identifier><altIdentifier>doi:10.26093/cds/vizier.51232206</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Prochaska J.X.</name></creator><creator><name>Gawiser E.</name></creator><creator><name>Wolfe A.M.</name></creator><creator><name>Quirrenbach A.</name></creator><creator><name>Lanzetta K.M.,Chen H.-W.</name></creator><creator><name>Cooke J.</name></creator><creator><name>Yahata N.</name></creator><date role="Updated">2023-04-06T16:50:47Z</date><date role="Created">2003-04-26T17:39:40Z</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>photometry</subject><description>This paper describes the acquisition and analysis of imaging data for the identification of galaxies associated with z~4 damped Ly{alpha} systems. We present deep BRI images of three fields known to contain four z~4 damped systems. We discuss the reduction and calibration of the data, detail the color criteria used to identify z~4 galaxies, and present a photometric redshift analysis to complement the color selection. We have found no galaxy candidates closer to the QSO than 7" that could be responsible for the damped Ly{alpha} systems. Assuming that at least one of the galaxies is not directly beneath the QSO, we set an upper limit on this damped Ly {alpha} system of L&lt;L^*^_LBG_/4. Finally, we have established a Web site to release these imaging data to the public, at http://kingpin.ucsd.edu/~dlaimg/papers/refern.html . 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