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<ri:Resource created="2023-02-09T13:59:37Z" status="active" updated="2025-05-19T09:50:00Z" 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>Arecibo polarimetric single-pulse survey</title><shortName>J/MNRAS/489/1543</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/489/1543</identifier><altIdentifier>doi:10.26093/cds/vizier.74891543</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Olszanski T.E.E.</name></creator><creator><name>Mitra D.</name></creator><creator><name>Rankin J.M.</name></creator><date role="Updated">2024-08-20T20:12:32Z</date><date role="Created">2023-02-09T13:59:37Z</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>pulsars</subject><subject>polarimetry</subject><subject>radio-spectroscopy</subject><description>We report on an Arecibo 4.5-GHz polarimetric single-pulse survey of the brightest pulsars at high frequency within its sky. The high-frequency profiles are accompanied by a collection of both previously published and unpublished high quality 1.4- and 0.33-GHz observations. Here our analyses and discussion primarily involve the average and statistical properties of the 46 pulsars polarimetric pulse sequences, profile classification and frequency evolution, and polarimetric profiles and peak-occurrence histograms. In most cases both the fractional linear polarization and profile widths decrease with frequency as expected, but there are some exceptions. Similarly, we were able to review and/or extend the profile classifications for this population of pulsars and work out their beaming characteristics quantitatively showing that almost all show properties compatible with the core/double-cone emission beam model. 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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>Name</name><description>Pulsar name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>P</name><description>Pulsar rotational 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.dispMeasure;instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RM</name><description>Rotation measure</description><unit>rad.m**2</unit><ucd>phys.polarization.rotMeasure</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>MJDP</name><description>? 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Binning on the P band</description><ucd>instr.setup</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>MJDL</name><description>Modified Julian date of the L band observation</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NpL</name><description>Number of pulses on the L band</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>BinsL</name><description>Binning on the L band</description><ucd>instr.setup</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MJDC</name><description>Modified Julian date of the C band observation</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NpC</name><description>Number of pulses on the C band</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>BinsC</name><description>Binning on the C band</description><ucd>instr.setup</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><table><name>J/MNRAS/489/1543/table2</name><description>Pulsar parameters</description><column><name>Name</name><description>Pulsar name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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Absolute fractional circular polarization in the P band</description><unit>%</unit><ucd>phys.polarization.circular</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_VabsP</name><description>? 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