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<ri:Resource created="2015-09-11T11:27:03Z" 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>327MHz observations of 124 pulsars</title><shortName>J/ApJ/804/23</shortName><identifier>ivo://CDS.VizieR/J/ApJ/804/23</identifier><altIdentifier>doi:10.26093/cds/vizier.18040023</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Krishnakumar M.A.</name></creator><creator><name>Mitra D.</name></creator><creator><name>Naidu A.</name></creator><creator><name>Joshi B.C.</name></creator><creator><name>Manoharan P.K.</name></creator><date role="Updated">2017-06-27T06:38:21Z</date><date role="Created">2015-09-11T11:27:03Z</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>radio-continuum-emission</subject><description>We present the measurements of scatter broadening timescales ({tau}_SC_) for 124 pulsars at 327MHz using the upgraded Ooty Radio Telescope (ORT). These pulsars lie in the dispersion measure range of 37-503pc/cm3 and declination ({delta}) range of -57{deg}&lt;{sigma}&lt;60{deg}. New {tau}_SC_ estimates for 58 pulsars are presented, increasing the sample of all such measurements by about 40% at 327MHz. Using all available {tau}_SC_ measurements in the literature, we investigate the dependence of {tau}_SC_ on dispersion measure. Our measurements, together with previously reported values for {tau}_SC_, affirm that the ionized interstellar medium up to 3kpc is consistent with the Kolmogorov spectrum, while it deviates significantly beyond this distance.</description><source format="bibcode">2015ApJ...804...23K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/804/23</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/VII/189">VII/189 : Catalog of Pulsars (Taylor+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/156">VII/156 : Catalog of 558 Pulsars (Taylor+ 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/763/80">J/ApJ/763/80 : GBT 350MHz survey. 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