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<ri:Resource created="1999-04-07T14:40:22Z" status="active" updated="2025-06-13T15:25:00Z" 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>Hubble Deep Field catalog of color-based redshift</title><shortName>J/AJ/116/2081</shortName><identifier>ivo://CDS.VizieR/J/AJ/116/2081</identifier><altIdentifier>doi:10.26093/cds/vizier.51162081</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wang Y.</name></creator><creator><name>Bahcall N.</name></creator><creator><name>Turner E.L.</name></creator><date role="Updated">2023-04-06T16:50:30Z</date><date role="Created">1999-04-07T14:40:22Z</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>galaxies</subject><subject>photometry</subject><subject>redshifted</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>Wide-band photometry</subject><description>We derive simple empirical color-redshift relations for z&lt;~4 galaxies in the Hubble Deep Field (HDF) using a linear function of three photometric colors (U-B, B-V, V-I). The dispersion between the estimated redshifts and the spectroscopically observed ones is small for relations derived in several separate color regimes; the dispersions range from {sigma}_z_~=0.03 to 0.1 for z&lt;~2 galaxies, and from {sigma}_z_~=0.14 to 0.25 for z&gt;~2 galaxies. We apply the color-redshift relations to the HDF photometric catalog and obtain estimated redshifts that are consistent with those derived from spectral template fitting methods. The advantage of these color-redshift relations is that they are simple and easy to use and do not depend on the assumption of any particular spectral templates; they provide model independent redshift estimates for z&lt;~4 galaxies using only multiband photometry, and they apply to about 90% of all galaxies. We provide a color-based estimated redshift catalog of HDF galaxies to z&lt;~4. We use the estimated redshifts to investigate the redshift distribution of galaxies in the HDF; we find peaks in the redshift distribution that suggest large-scale clustering of galaxies to at least z~1 and that are consistent with those identified in spectroscopic probes of the HDF.</description><source format="bibcode">1998AJ....116.2081W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/116/2081</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/J/A+AS/129/583">J/A+AS/129/583 : Hubble Deep Field surface photometry (Fasano+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/112/1335">J/AJ/112/1335 : Hubble Deep Field observations (Williams+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/112/359">J/AJ/112/359 : Galaxies in the Hubble Deep Field (van den Bergh+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/471/L5">J/ApJ/471/L5 : Redshift clustering in the Hubble Deep Field (Cohen+ 1996)</relatedResource><relatedResource>Table 1: galaxies not used in determining the z_a_ relations</relatedResource><relatedResource>Sawicki: From Sawicki et al. (1997AJ....113....1S)catalog,</relatedResource><relatedResource>x, y: pixel position on v.2 HDF images</relatedResource><relatedResource>z: spectroscopic redshift</relatedResource><relatedResource>za: color-based redshift</relatedResource><relatedResource>ztemp: redshift from spectral template-fitting</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/116/2081</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/116/2081</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/116/2081</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/116/2081</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/116/2081</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/116/2081</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><facility>HST</facility><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/116/2081/table2</name><description>Catalog of color-based redshift estimates</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Sawicki</name><description>Identification number in Sawicki et al. (1997AJ....113....1S) photometric catalog (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>xpos</name><description>x position on v2 HDF image</description><unit>pix</unit><ucd>pos.cartesian.x;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ypos</name><description>y position on v2 HDF image</description><unit>pix</unit><ucd>pos.cartesian.y;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>m814</name><description>m814 (I) magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>m606</name><description>m606 (V) magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>m450</name><description>m450 (B) magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>m300</name><description>m300 (U) magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ztemp</name><description>Photometric redshift from fitting spectral templates by Sawicki et al. 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