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<ri:Resource created="2012-05-23T12:25:49Z" 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>Isolated neutron stars from Rosat and Swift</title><shortName>J/ApJ/714/1424</shortName><identifier>ivo://CDS.VizieR/J/ApJ/714/1424</identifier><altIdentifier>doi:10.26093/cds/vizier.17141424</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Turner M.L.</name></creator><creator><name>Rutledge R.E.</name></creator><creator><name>Letcavage R.</name></creator><creator><name>Shevchuk A.S.H.</name></creator><creator><name>Fox D.B.</name></creator><date role="Updated">2017-11-06T12:23:26Z</date><date role="Created">2012-05-23T12:25:49Z</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>x-ray-sources</subject><subject>astronomical-object-identification</subject><subject>pulsars</subject><description>Using new and archival observations made with the Swift satellite and other facilities, we examine 147 X-ray sources selected from the ROSAT All-Sky-Survey Bright Source Catalog (RASS/BSC) to produce a new limit on the number of isolated neutron stars (INSs) in the RASS/BSC, the most constraining such limit to date. Independent of X-ray spectrum and variability, the number of INSs is &lt;=48 (90% confidence). Restricting attention to soft (kT_eff_&lt;200eV), non-variable X-ray sources -as in a previous study- yields an all-sky limit of &lt;=31 INSs. In the course of our analysis, we identify five new high-quality INS candidates for targeted follow-up observations. A future all-sky X-ray survey with eROSITA, or another mission with similar capabilities, can be expected to increase the detected population of X-ray-discovered INSs from the 8-50 in the BSC, to (for a disk population) 240-1500, which will enable a more detailed study of neutron star population models.</description><source format="bibcode">2010ApJ...714.1424T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/714/1424</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/IX/10">IX/10 : ROSAT All-Sky Bright Source Catalogue (1RXS) (Voges+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/527/A139">J/A+A/527/A139 : X-ray bursting neutron star atmosphere models (Suleimanov+,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/473/523">J/A+A/473/523 : Spectroscopic monitoring of 3 neutron stars (Van der Meer+,</relatedResource><relatedResource>http://heasarc.gsfc.nasa.gov/cgi-bin/W3Browse/swift.pl : Swift mission archive</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/714/1424</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/714/1424</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/714/1424</mirrorURL></interface></capability><capability><interface 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