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<ri:Resource created="2025-07-16T09:16:27Z" status="active" updated="2025-08-01T20:03:22Z" 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>LoTSS DR2 visual classifications</title><shortName>J/A+A/699/A338</shortName><identifier>ivo://CDS.VizieR/J/A+A/699/A338</identifier><altIdentifier>doi:10.26093/cds/vizier.36990338</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Horton M.A.</name></creator><creator><name>Hardcastle M.J.</name></creator><creator><name>Miley G.K.</name></creator><creator><name>Tasse C.</name></creator><creator><name>Shimwell T.</name></creator><date role="Updated">2025-08-01T20:03:22Z</date><date role="Created">2025-07-16T09:16:27Z</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-continuum-emission</subject><subject>radio-sources</subject><description>The LOw Frequency ARray Two-metre Sky Survey second data release (LoTSS DR2) covers 27% of the northern sky and contains around four million radio sources. The development of this catalogue involved a large citizen science project (Radio Galaxy Zoo: LOFAR) with more than 116,000 resolved sources going through visual inspection. We took a subset of sources with flux density above 75mJy and an angular size of 90" or greater, giving a total of 9985 sources or ~10% of the visually inspected sources. We classified these by visual inspection in terms of broad source type (e.g., Fanaroff-Riley class I or II, narrow or wide-angle tail, relaxed double), noticeable features (wings, visible jets, banding, filaments etc), environmental features (cluster environment, merger, diffuse emission). Our specific aim was to search for features linked to jet precession, such as a misaligned jet axis, curvature and multiple hotspots. This combination of features and morphology allowed us to detect increasingly fine-grained sub- populations of interesting or unusual sources. We found that 28% of sources showed evidence of one or more precession indicators, which could make them candidates for hosting close binary supermassive black holes. Potential precession signatures occur in sources of all sizes and luminosities in our sample but appear to favour more massive host galaxies. Our work greatly expands the sample size and parameter space of searches for precession signatures in powerful jetted sources. This work also showcases the diversity of large bright radio sources in the LOFAR surveys, whether or not precession indicators are present.</description><source format="bibcode">2025A&amp;A...699A.338H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/699/A338</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+A/622/A1">J/A+A/622/A1 : LOFAR Two-metre Sky Survey DR1 source cat. 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32613 32617-32618 32620 32622-32623 32626 32628-32629 32631 32634-32635 32655-32657 32659 32665-32666 32668 32670 32675 32688 32690-32691 32694-32695 32708-32709 32712 32714-32715 32717-32718 32720-32722 32730-32733 32735-32737 32739-32741 32743-32745 32747-32749 32751-32754 32757 32759-32761 32763</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/699/A338?format=ascii</footprint><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/699/A338/catalog</name><description>Visual classifications and precession indicators for extended radio sources from LoTSS DR2</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>zbest</name><description>? Best estimate of the source redshift (z_best)</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Size</name><description>? Source physical size in kpc (Size)</description><unit>kpc</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Name</name><description>Name of the source from the LoTSS DR2 optical ID catalogue, Cat. J/A+A/678/A151, ILTJHHMMSS.ss+DDMMSS.s (Source_Name)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="22*">char</dataType></column><column><name>L144</name><description>? Source radio luminosity at 144 MHz (L_144)</description><unit>W/Hz</unit><ucd>phys.luminosity;em.radio.100-200MHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logMassmed</name><description>? Base 10 logarithm of source host galaxy stellar mass estimate (Mass_median)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_logMassmed</name><description>[0/1] Mass quality flag (do not use if = 0) (flag_mass)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FRI</name><description>[0/1] Boolean, source is an FRI (fri)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FRII</name><description>[0/1] Boolean, source is an FRII (frii)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Hybrid</name><description>[0/1] Boolean, source is a hybrid as described in the paper (hybrid)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Spiral</name><description>[0/1] Boolean, source is a spiral galaxy (spiral)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Relaxed</name><description>[0/1] Boolean, source is a relaxed double (relaxed)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Cshaped</name><description>[0/1] Boolean, source is c-shaped (cshaped)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Sshaped</name><description>[0/1] Boolean, source is s-shaped (sshaped)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Misalign</name><description>[0/1] Boolean, source is misaligned (misaligned)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Wings</name><description>[0/1] Boolean, source has wings (wings)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Xshaped</name><description>[0/1] Boolean, source is x-shaped (xshaped)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Straight</name><description>[0/1] Boolean, source has a straight jet (straight)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MultHSpot</name><description>[0/1] Boolean, source has multiple hotspots in one or both lobes (multihotspots)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Continuous</name><description>[0/1] Boolean, source has a continuous jet (continuous)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Banding</name><description>[0/1] Boolean, source shows banding structure (banding)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Onesided</name><description>[0/1] Boolean, source is one-sided (onesided)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Restarted</name><description>[0/1] Boolean, source shows signs of having restarted (restarted)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Cluster</name><description>[0/1] Boolean, source is a cluster member (cluster)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Merger</name><description>[0/1] Boolean, source is a merger (merger)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Diffuse</name><description>[0/1] Boolean, source has diffuse structure only (diffuse)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Unknown</name><description>[0/1] Boolean, source classification is unknown (unknown)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FeatureCT</name><description>Total number of features identified (featurecount)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Hasany1</name><description>[0/1] Source has any one precession indicator (hasanyone)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>hasany2</name><description>[0/1] Source has any two precession indicators (hasanytwo)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Hasall</name><description>[0/1] Source has all three precession indicators used in the paper (hasall)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Has1</name><description>[0/1] Source has exactly one precession indicator (has_exactly_1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Has2</name><description>[0/1] Source has exactly two precession indicators (has_exactly_2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SE</name><description>[0/1] Source shows s symmetry and misalignment (se)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MS</name><description>[0/1] Source shows s symmetry and multiple hotspots (ms)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>EM</name><description>[0/1] Source shows multiple hotspots and misalignment (em)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>