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<ri:Resource created="2003-02-16T18:27:01Z" 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>The Hamburg/SAO Survey for BCGs. I.</title><shortName>J/A+A/397/463</shortName><identifier>ivo://CDS.VizieR/J/A+A/397/463</identifier><altIdentifier>doi:10.26093/cds/vizier.33970463</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ugryumov A.V.</name></creator><creator><name>Engels D.</name></creator><creator><name>Pustilnik S.A. Kniazev A.Y.</name></creator><creator><name>Pramsky A.G.,Hagen H.-J.</name></creator><date role="Updated">2003-02-16T17:28:16Z</date><date role="Created">2003-02-16T18:27:01Z</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>spectroscopy</subject><subject>radial-velocity</subject><description>We present the description and the first results of a new project devoted to the search for extremely metal-deficient blue compact/HII-galaxies (BCGs) and to the creation of a well selected large BCG sample with strong emission lines. Such galaxies should be suitable for reliable determination of their oxygen abundance through the measurement of the faint [OIII]4363{AA} line. The goals of the project are two-fold: a) to discover a significant number of new extremely metal-poor galaxies (Z&lt;=1/20Z_{sun}_), and b) to study the metallicity distribution of local BCGs. Selection of candidates for follow-up slit spectroscopy is performed on the database of objective prism spectra of the Hamburg Quasar Survey. The sky region is limited by {delta}&gt;=0{deg} and b^II^&lt;=-30{deg}. In this paper we present the results of the follow-up spectroscopy conducted with the Russian 6m telescope. The list of observed candidates contained 52 objects, of which 46 were confirmed as strong-lined BCGs (EW([OIII]5007&gt;=100{AA}). The remaining five lower excitation ELGs include three BCGs, and two galaxies classified as SBN (Starburst Nucleus) and DANS (Dwarf Amorphous Nucleus Starburst). One object is identified as a quasar with a strong Ly_alpha emission line near {lambda}=5000{AA} (z~3). We provide a list with coordinates, measured radial velocities, B-magnitudes, equivalent widths EW([OIII]5007) and EW(H{beta}) and for the 46 strong-lined BCGs the derived oxygen abundances 12+log(O/H). The abundances range between 7.42 and 8.4 (corresponding to metallicities between 1/30 and 1/3Z_{sun}_). The sample contains four galaxies with Z&lt;=1/20Z_{sun}_, of which three are new discoveries. This demonstrates the high efficiency of the new project to find extremely metal-deficient galaxies. The radial velocities of the strong-lined ELGs range between 500 and 19000km/s with a median value of ~6400km/s. The typical B-magnitudes of the galaxies presented are 17.0mag-18.0mag.</description><source format="bibcode">2003A&amp;A...397..463U</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/397/463</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/A+AS/135/511">J/A+AS/135/511 : The Hamburg/SAO Survey for ELGs. I. (Ugryumov+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/137/299">J/A+AS/137/299 : The Hamburg/SAO Survey for ELGs. II. (Pustilnik+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/142/417">J/A+AS/142/417 : The Hamburg/SAO Survey for ELGs. III. (Hopp+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/366/771">J/A+A/366/771 : The Hamburg/SAO Survey for ELGs. IV (Kniazev+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/374/907">J/A+A/374/907 : The Hamburg/SAO Survey for ELGs. V. 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