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<ri:Resource created="2024-05-02T08:40:53Z" status="active" updated="2026-02-10T20:08:25Z" 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>FAST Pulsar Database. I.</title><shortName>J/other/RAA/23.J</shortName><identifier>ivo://CDS.VizieR/J/other/RAA/23.J4002</identifier><altIdentifier>doi:10.26093/cds/vizier/dx/cdkueaac</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wang P.F.</name></creator><creator><name>Han J.L.</name></creator><creator><name>Xu J.</name></creator><creator><name>Wang C.</name></creator><creator><name>Yan Y.</name></creator><creator><name>Jing W.C.</name></creator><creator><name>Su W.Q.</name></creator><creator><name>Zhou D.J.,Wang T.</name></creator><date role="Updated">2026-02-10T20:08:25Z</date><date role="Created">2024-05-02T08:40:53Z</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>pulsars</subject><subject>polarimetry</subject><subject>radio-sources</subject><description>Pulsar polarization profiles form a very basic database for understanding the emission processes in a pulsar magnetosphere. After careful polarization calibration of the 19-beam L-band receiver and verification of beam-offset observation results, we obtain polarization profiles of 682 pulsars from observations by the Five-hundred-meter Aperture Spherical radio Telescope (FAST) during the Galactic Plane Pulsar Snapshot survey and other normal FAST projects. Among them, polarization profiles of about 460 pulsars are observed for the first time. The profiles exhibit diverse features. Some pulsars have a polarization position angle curve with a good S-shaped swing, some with orthogonal modes; some have components with highly linearly polarized components or strong circularly polarized components; some have a very wide profile, coming from an aligned rotator, and some have an interpulse from a perpendicular rotator; some wide profiles are caused by interstellar scattering. We derive geometric parameters for 190 pulsars from the S-shaped position angle curves or with orthogonal modes. We find that the linear and circular polarization or the widths of pulse profiles have various frequency dependencies. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>more</name><description>indicates more informations in table 4 and/or 5</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>PSR</name><description>Pulsar name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType><flag>primary</flag></column><column><name>Per</name><description>Period</description><unit>s</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DM</name><description>dIspersion measure</description><unit>pc.cm**-3</unit><ucd>phys</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Date</name><description>FAST observation date</description><ucd>time.epoch;obs</ucd><flag>nullable</flag></column><column><name>Offset</name><description>? 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Profile width at 10% of the peak intensity</description><unit>deg</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_W10</name><description>? rms uncertainty on W10</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>L/I</name><description>? Degree of linear polarization</description><unit>%</unit><ucd>phys.polarization.linear</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_L/I</name><description>? rms uncertainty on L/I</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>V/I</name><description>? 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PSR</name><description>Pulsar name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>PAsens</name><description>Position angle Swing (1)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>SComp1</name><description>[-+?] Sens of component 1 (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>SComp2</name><description>[-+?] Sens of component 2 (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table><table><name>J/other/RAA/23.J4002/table5</name><description>Geometric Parameters for 190 Pulsars</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>P</name><description>Period</description><unit>s</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>alpha0</name><description>Inclination angle</description><unit>deg</unit><ucd>src.orbital.inclination</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_alpha0</name><description>? Error on alpha0 (lower value)</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_alpha0</name><description>? Error on alpha0 (upper value)</description><unit>deg</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>beta0</name><description>Impact angle</description><unit>deg</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_beta0</name><description>? Error on beta0 (lower value)</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_beta0</name><description>? Error on beta0 (upper value)</description><unit>deg</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>phi0</name><description>Phase where the PA swing has the largest gradient</description><unit>deg</unit><ucd>pos.phaseAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_phi0</name><description>? 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