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<ri:Resource created="2024-02-02T11:09:37Z" status="active" updated="2026-03-17T20:08:00Z" 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>Radio properties of z&gt;=1 galaxies</title><shortName>J/other/AstBu/78</shortName><identifier>ivo://CDS.VizieR/J/other/AstBu/78.443</identifier><altIdentifier>doi:10.26093/cds/vizier/dv/hikeed</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Khabibullina M.</name></creator><creator><name>Mikhailov A.</name></creator><creator><name>Sotnikova Yu.</name></creator><creator><name>Mufakharov T.</name></creator><creator><name>Mingaliev M.,Kudryashova A.</name></creator><creator><name>Bursov N.</name></creator><creator><name>Stolyarov V.</name></creator><creator><name>Udovitskij R.</name></creator><date role="Updated">2026-03-17T20:08:00Z</date><date role="Created">2024-02-02T11:09:37Z</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>catalogs</subject><subject>radio-galaxies</subject><subject>active-galactic-nuclei</subject><subject>radio-continuum-emission</subject><description>Study of high-redshift radio galaxies (HzRGs) can shed light on the active galactic nuclei (AGNs) evolution in massive elliptical galaxies. The vast majority of observed high-redshift AGNs are quasars, and there are very few radio galaxies at redshifts z&gt;3. We present the radio properties of 173 sources optically identified with radio galaxies at z&gt;1 with flux densities S_1.4_&gt;20mJy. Literature data were collected for compilation of broadband radio spectra, estimation of radio variability, radio luminosity, and radio loudness. Almost 60% of the galaxies have steep or ultra-steep radio spectra; 22% have flat, inverted, upturn, and complex spectral shapes, and 18% have peaked spectra (PS). The majority of the PS sources in the sample (20/31) are megahertz-peaked spectrum sources candidates, i.e. possibly very young and compact radio galaxies. The median values of the variability indices at 11 and 5GHz are V_S11_=0.14 and V_S5_=0.13, which generally indicates a weak or moderate character of the long-term variability of the studied galaxies. The typical radio luminosity and radio loudness are L5 =10^43^-10^44^erg/s and logR=3-4 respectively. We have found less prominent features of the bright compact radio cores for our sample compared to high-redshift quasars at z&gt;3. The variety of the obtained radio properties shows the different conditions for the formation of radio emission sources in galaxies.</description><source format="bibcode">2023AstBu..78..443K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/AstBu/78.443</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>ftp://cats.sao.ru/pub/CATS/RGLIST : CATS Home Page</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/other/AstBu/78.443/table2</name><description>The radio properties of the sample</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>Name</name><description>NVSS name (JHHMM+DDMM, J2000)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>logL5</name><description>? Log of radio luminosity at 5CHz</description><unit>log(1e-07W)</unit><ucd>phys.luminosity;em.radio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_logL5</name><description>? rms (plus) uncertainty on log radio luminosity at 5CHz</description><unit>log(1e-07W)</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logL5</name><description>? rms (minus) uncertainty on log radio luminosity at 5CHz</description><unit>log(1e-07W)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logR1</name><description>? Logarithm of radio loudness, calculated in 1 way</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_logR1</name><description>? rms (plus) uncertainty on logarithm of radio loudness, calculated in 1 way</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logR1</name><description>? rms (minus) uncertainty on logarithm of radio loudness, calculated in 1 way</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logR2</name><description>? Logarithm of radio loudness, calculated in 2 way</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_logR2</name><description>? rms (plus) uncertainty on logarithm of radio loudness, calculated in 2 way</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logR2</name><description>? rms (minus) uncertainty on logarithm of radio loudness, calculated in 2 way</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>alphalow</name><description>? Spectral indices calculated for the frequencies lower than the point where the spectral slope changes its sign from positive to negative</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_alphalow</name><description>? rms uncertainty on {alpha}_low</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>alphahigh</name><description>? Spectral indices calculated for the frequencies higher than the point where the spectral slope changes its sign from negative to positive</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_alphahigh</name><description>? rms uncertainty on {alpha}_high</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SpType</name><description>? Radio spectrum type</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>M5</name><description>? Modulation index</description><ucd>src.var.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>V5</name><description>? Variability index</description><ucd>src.var.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Nobs</name><description>? Number of observations</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>nupeakobs</name><description>? The observed peak frequency in the spectrum</description><ucd>em.freq;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/other/AstBu/78.443/refs</name><description>References</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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