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<ri:Resource created="2025-05-26T10:02:39Z" status="active" updated="2026-03-20T20:03:01Z" 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>RACS VI. RACS-high 1655.5MHz catalogue</title><shortName>J/other/PASA/42.</shortName><identifier>ivo://CDS.VizieR/J/other/PASA/42.38</identifier><altIdentifier>doi:10.26093/cds/vizier/ds/eckdi</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Duchesne S.</name></creator><creator><name>Ross K.</name></creator><creator><name>Thomson A.J.M.</name></creator><creator><name>Lenc E.</name></creator><creator><name>Murphy T.</name></creator><creator><name>Galvin T.J.,Hotan A.W.</name></creator><creator><name>Moss V.A.</name></creator><creator><name>Whiting M.T.</name></creator><date role="Updated">2026-03-20T20:03:01Z</date><date role="Created">2025-05-26T10:02:39Z</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-sources</subject><subject>radio-continuum-emission</subject><subject>galaxy-classification-systems</subject><description>We have conducted a widefield, wideband, snapshot survey using the Australian SKA Pathfinder (ASKAP) referred to as the Rapid ASKAP Continuum Survey (RACS). RACS covers ~90% of the sky, with multiple observing epochs in three frequency bands sampling the ASKAP frequency range of 700-1800MHz. This work contains the catalogues from the third major epoch at 1655.5MHz, RACS-high. From the 1493 images covering the sky up to declination +48 degrees, we present a catalogue of 2677509 radio sources and 3526674 Gaussian components. The catalogue is constructed from images with a median root-mean-square noise of 195uJy/beam and a median angular resolution of 11.8" by 8.1". The overall reliability of the catalogue is estimated to be 99.18%, and we find a decrease in reliability as angular resolution improves. We estimate the brightness scale to be accurate to 10%, and the astrometric accuracy to be within ~0.6" in right ascension and ~0.7" in declination after correction of a systematic declination-dependent offset. All data products from RACS-high, including calibrated visibility datasets, images from individual observations, full- sensitivity mosaics, and the all-sky catalogue are available at the CSIRO ASKAP Science Data Archive: https://doi.org/10.25919/g3jd-av02.</description><source format="bibcode">2025PASA...42...38D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/PASA/42.38</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/other/PASA/38.58">J/other/PASA/38.58 : Rapid ASKAP Continuum Survey. II. RACS cat. (Hale+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/PASA/41.3">J/other/PASA/41.3 : Rapid ASKAP Continuum Survey. 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xsi:type="vs:VOTableType">double</dataType></column><column><name>e_FtotPy</name><description>Uncertainty in the total flux density at 1655.5MHz from PyBDSF fitting (E_Total_flux_PyBDSF)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Ftot</name><description>Quadrature sum of the brightness scale and PyBDSF uncertainties for total flux density at 1655.5MHz (E_Total_flux)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Fpeak</name><description>Peak flux density at 1655.5MHz of the source (Peak_flux)</description><unit>mJy/beam</unit><ucd>phot.flux.density;em.radio.1500-3000MHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_FpeakPy</name><description>Uncertainty in the peak flux density at 1655.5MHz from PyBDSF fitting 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(Peak_flux)</description><unit>mJy/beam</unit><ucd>phot.flux.density;em.radio.1500-3000MHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_FpeakPy</name><description>Uncertainty in the peak flux density from PyBDSF fitting (E_Peak_flux_PyBDSF)</description><unit>mJy/beam</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Min</name><description>Size of the minor axis of the source (Min_axis)</description><unit>arcsec</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>PA</name><description>Position angle of the source, east of north (PA)</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Maj</name><description>Uncertainty in the source major axis (E_Maj_axis)</description><unit>arcsec</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Min</name><description>Uncertainty in the source minor axis (E_Min_axis)</description><unit>arcsec</unit><ucd>stat.error;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_PA</name><description>Uncertainty in the source PA (E_PA)</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>DCMaj</name><description>Deconvolved source major axis (DC_Maj_axis)</description><unit>arcsec</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>DCMin</name><description>Deconvolved source minor axis (DC_Min_axis)</description><unit>arcsec</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>DCPA</name><description>Deconvolved source PA (DC_PA)</description><unit>deg**2</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_DCMaj</name><description>Uncertainty in the deconvolved source major axis (E_DC_Maj_axis)</description><unit>arcsec</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_DCMin</name><description>Uncertainty in the deconvolved source minor axis (E_DC_Min_axis)</description><unit>arcsec</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_DCPA</name><description>Uncertainty in the deconvolved source PA (E_DC_PA)</description><unit>deg**2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Noise</name><description>Local estimate of the root-mean-square noise (Noise)</description><unit>mJy/beam</unit><ucd>instr.det.noise</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tilel</name><description>Direction cosine l of the source with respect to the field centre (Tile_l)</description><unit>deg</unit><ucd>pos.dirCos;obs.field</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Tilem</name><description>Direction cosine m of the source with respect to the field centre (Tile_m)</description><unit>deg</unit><ucd>pos.dirCos;obs.field</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Tilesep</name><description>Angular separation from the field centre (Tile_sep)</description><unit>deg**2</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>PSFMaj</name><description>Major axis FWHM of the PSF for the field (PSF_Maj)</description><unit>arcsec</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PSFMin</name><description>Minor axis FWHM of the PSF for the field (PSF_Min)</description><unit>arcsec</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PSFPA</name><description>PA of the PSF for the field (PSF_PA)</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SCode</name><description>[MS] Source structure classification by PyBDSF, S = single, M = multiple (S_Code)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Flag</name><description>[0/2] Source type flag, 0 = unresolved, 1 = resolved (Flag)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>