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<ri:Resource created="2026-03-06T08:01:25Z" status="active" updated="2026-03-06T07:11:29Z" 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>LOFAR Two-metre Sky Survey (LoTSS) DR3</title><shortName>J/A+A/707/A198</shortName><identifier>ivo://CDS.VizieR/J/A+A/707/A198</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Shimwell T.W.</name></creator><creator><name>Hardcastle M.J.</name></creator><creator><name>Tasse C.</name></creator><creator><name>Drabent A.</name></creator><creator><name>Botteon A.,Williams W.L.</name></creator><creator><name>Best P.N.</name></creator><creator><name>Roettgering H.J.A.</name></creator><creator><name>Brueggen M.</name></creator><creator><name>Brunetti G.,Callingham J.R.</name></creator><creator><name>Chyzy K.T.</name></creator><creator><name>Conway J.E.</name></creator><creator><name>De Gasperin F.</name></creator><creator><name>Haverkorn M.,Horellou C.</name></creator><creator><name>Jackson N.</name></creator><creator><name>Miley G.K.</name></creator><creator><name>Morabito L.K.</name></creator><creator><name>Morganti R.,O'Sullivan S.P.</name></creator><creator><name>Schwarz D.J.</name></creator><creator><name>Smith D.J.B.</name></creator><creator><name>van Weeren R.J.,Vedantham H.K.</name></creator><creator><name>White G.J.</name></creator><creator><name>Ahmadi A.</name></creator><creator><name>Alegre L.</name></creator><creator><name>Arias M.</name></creator><creator><name>Asabere B.,Bahr-Kalus B.</name></creator><creator><name>Barkus B.</name></creator><creator><name>Bilicki M.</name></creator><creator><name>Boehme L.</name></creator><creator><name>Brentjens M.,Brienza M.</name></creator><creator><name>Bomans D.J.</name></creator><creator><name>Bonafede A.</name></creator><creator><name>Bonato M.</name></creator><creator><name>Bonnassieux E.,Boxelaar J.M.</name></creator><creator><name>Camera S.</name></creator><creator><name>Cassano R.</name></creator><creator><name>Chilufya J.</name></creator><creator><name>Cianfaglione M.,Croston J.H.</name></creator><creator><name>Cuciti V.</name></creator><creator><name>Dabhade P.</name></creator><creator><name>De Rubeis E.</name></creator><creator><name>de Jong J.M.G.H.J.,Dallacasa D.</name></creator><creator><name>Dettmar R.J.</name></creator><creator><name>Duncan K.J.</name></creator><creator><name>Di Gennaro G.</name></creator><creator><name>Edler H.W.,Groeneveld C.</name></creator><creator><name>Guerkan G.</name></creator><creator><name>Hajduk M.</name></creator><creator><name>Hale C.L.</name></creator><creator><name>Heesen V.</name></creator><creator><name>Hoang D.N.,Hoeft M.</name></creator><creator><name>Holties H.</name></creator><creator><name>Horton M.A.</name></creator><creator><name>Iacobelli M.</name></creator><creator><name>Jamrozy M.</name></creator><creator><name>Jarvis M.J.,Jelic V.</name></creator><creator><name>Kadler M.</name></creator><creator><name>Kondapally R.</name></creator><creator><name>Kunert-Bajraszewska M.</name></creator><creator><name>Loose M.,Magliocchetti M.</name></creator><creator><name>Malek K.</name></creator><creator><name>Manzano C.</name></creator><creator><name>McKean J.P.</name></creator><creator><name>Mevius M.</name></creator><creator><name>Mingo B.,Miskolczi A.</name></creator><creator><name>Misra A.</name></creator><creator><name>Moldon J.</name></creator><creator><name>Nair D.G.</name></creator><creator><name>Nakoneczny S.J.</name></creator><creator><name>Orru E.,Pashapour-Ahmadabadi M.</name></creator><creator><name>Pasini T.</name></creator><creator><name>Petley J.</name></creator><creator><name>Pierce J.C.S.</name></creator><creator><name>Prandoni I.,Rafferty D.</name></creator><creator><name>Rajpurohit K.</name></creator><creator><name>Riseley C.J.</name></creator><creator><name>Roberts I.D.</name></creator><creator><name>Sethi S.,Shulevski A.</name></creator><creator><name>Stein M.</name></creator><creator><name>Stuardi C.</name></creator><creator><name>Sweijen F.</name></creator><creator><name>ter Veen S.</name></creator><creator><name>Timmerman R.,Vaccari M.</name></creator><creator><name>Wijnholds S.</name></creator><date role="Updated">2026-03-06T07:11:29Z</date><date role="Created">2026-03-06T08:01:25Z</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>surveys</subject><subject>radio-continuum-emission</subject><description>We present the third data release of the LOFAR Two-metre Sky Survey (LoTSS-DR3). The survey images cover 88% of the northern sky and were created from 12950 hrs of data (18.6 PB) accumulated over 10.5 years. Producing the images took 20 million core hours of processing through direction-independent and direction-dependent calibration pipelines that correct for instrumental effects as well as spatially and temporally varying ionospheric distortions. In our 120-168MHz continuum mosaic images with an angular resolution of 600 (900 below declination 10{deg}) we catalogue 13667877 sources, formed from 16,943,656 Gaussian components. The scatter in the astrometric precision approximately follows the expected noise-like behaviour but with an additional systematic component of at least 0.2400 that is likely due to calibration imperfections. The random flux density scale error is 6%, while the systematic offset was previously shown to be within 2%. The median sensitivity of our mosaics is 92mJy/beam, improving to 68mJy/beam at high observing elevations, but degrading to 183mJy/beam at the celestial equator due to station area projection effects. Completeness simulations, accounting for realistic source models, time- and bandwidth-smearing effects, and astrometric errors, indicate that we detect more than 95% of compact sources with integrated flux densities exceeding 9 times the local root mean square (RMS) noise. However, the recovered source counts in a particular integrated flux density bin do not match the injected counts until flux densities exceed 45 times the local RMS noise. The Euclidean-normalised differential source counts derived from the survey constrain the radio source population over five orders of magnitude and are in good agreement with previous deep and wide-area surveys. All data products are publicly available, including catalogues, individual-field Stokes I, Q, U, and V images, mosaicked Stokes I images, and uv data with associated direction-dependent calibration solutions.</description><source format="bibcode">2026A&amp;A...707A.198S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/707/A198</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 catalog (Shimwell+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/659/A1">J/A+A/659/A1 : 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Deconvolved FWHM of the major axis of the source</description><unit>arcsec</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_DCMaj</name><description>? Uncertainty in deconvolved FWHM of the major axis</description><unit>arcsec</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>DCMin</name><description>? Deconvolved FWHM of the minor axis of the source</description><unit>arcsec</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_DCMin</name><description>? Uncertainty in deconvolved FWHM of the minor axis</description><unit>arcsec</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PA</name><description>[]? Fitted position angle of the major axis of the source measured east of north</description><unit>deg</unit><ucd>pos.posAng;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_PA</name><description>? Uncertainty in fitted position angle of the major axis of the source</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>DCPA</name><description>? Deconvolved position angle of the major axis of the source measured east of north</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_DCPA</name><description>? Uncertainty in deconvolved position angle of the major axis of the source</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Islrms</name><description>RMS Average background RMS value of the island in which the source is located</description><unit>mJy/beam</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>IslFTot</name><description>Integrated Stokes I flux density of the island in which the source is located</description><unit>mJy</unit><ucd>phot.flux.density;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_IslFTot</name><description>Uncertainty in integrated Stokes I flux density of the island</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SCode</name><description>Source classification code (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>HEALPIX</name><description>HEALPix pixel index of the source position, computed at NSIDE = 16</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Res</name><description>The angular resolution of the mosaic image from which the source was extracted</description><ucd>pos.angResolution</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>