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<ri:Resource created="2003-03-29T10:46:19Z" 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>Neutron stars in NGC 5139</title><shortName>J/ApJ/578/405</shortName><identifier>ivo://CDS.VizieR/J/ApJ/578/405</identifier><altIdentifier>doi:10.26093/cds/vizier.15780405</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rutledge R.E.</name></creator><creator><name>Bildsten L.</name></creator><creator><name>Brown E.F.</name></creator><creator><name>Pavlov G.G.</name></creator><creator><name>Zavlin V.E.</name></creator><date role="Updated">2003-03-29T09:46:43Z</date><date role="Created">2003-03-29T10:46:19Z</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>globular-star-clusters</subject><subject>pulsars</subject><subject>x-ray-sources</subject><description>The Chandra/ACIS-I detectors observed NGC 5139 in imaging mode for two continuous periods (2000 January 24 02:15-09:46 and January 25 04:33-17:24 TT) for a total exposure of ~68.6ks. We combined the two observations and analyzed them as one. We searched for point sources using CELLDETECT, using only the 0.1-2.5keV energy range, excluding regions less than 16 pixels from the detector edges and keeping only sources with signal-to-noise ratio (S/N)&gt;5.0. 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