<?xml version='1.0'?><?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?><ri:Resource created="2024-11-25T12:00:00Z" status="active" updated="2024-12-05T15:55:05Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:g-colstat="http://dc.g-vo.org/ColStats-1" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vg="http://www.ivoa.net/xml/VORegistry/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://dc.g-vo.org/ColStats-1 http://vo.ari.uni-heidelberg.de/docs/schemata/Colstats.xsd http://www.ivoa.net/xml/RegistryInterface/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/RegistryInterface.xsd http://www.ivoa.net/xml/VORegistry/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VORegistry.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>Galactic X-ray Pulsars</title><shortName>FAI xray pulsars</shortName><identifier>ivo://fai.kz/pulsars/q/scs</identifier><curation><publisher>Fesenkov Astrophysical Institute</publisher><creator><name>FAI NVO Team</name><logo>https://dachs.fai.kz/favicon.png</logo></creator><date role="Updated">2024-12-05T15:55:00Z</date><contact><name>FAI NVO Team</name><address>Observatory 23, 050020 Almaty, Kazakhstan</address><email>vo@fai.kz</email></contact></curation><content><subject>pulsars</subject><description> This catalog contains data on the Galactic population of 82 confirmed
X-ray pulsars in high-mass X-ray binary (HMXB) systems, classified
into 18 persistent and 64 transient sources. Key parameters include
spin periods, spin evolution (local and global trends), orbital
periods, X-ray luminosities, magnetic fields, distances, and detailed
companion star characteristics. The data have been compiled through
cross-matching with recent HMXB catalogs and databases such as Fortin
et al. (2023), Neumann et al. (2023), and Krivonos et al. (2022),
supplemented with literature and SIMBAD database analysis. The catalog
aims to support studies on stellar evolution, accretion processes, and
binary dynamics.</description><source format="bibcode">2023ApJS..268...21K</source><referenceURL>https://dachs.fai.kz/pulsars/q/scs/info</referenceURL><type>service</type><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://fai.kz/tap">FAI archives TAP service</relatedResource></relationship></content><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://dachs.fai.kz/pulsars/q/scs/form</accessURL></interface></capability><capability standardID="ivo://ivoa.net/std/conesearch" xsi:type="cs:ConeSearch"><interface role="std" xsi:type="vs:ParamHTTP"><accessURL use="base">https://dachs.fai.kz/pulsars/q/scs/scs.xml?</accessURL><queryType>GET</queryType><resultType>application/x-votable+xml</resultType><param std="true"><name>RA</name><description>Right Ascension (ICRS decimal)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><dataType xsi:type="vs:SimpleDataType">real</dataType></param><param std="true"><name>DEC</name><description>Declination (ICRS decimal)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><dataType xsi:type="vs:SimpleDataType">real</dataType></param><param std="true"><name>SR</name><description>Search radius</description><unit>deg</unit><dataType xsi:type="vs:SimpleDataType">real</dataType></param><param std="false"><name>Ps</name><description>Spin period of the pulsar</description><unit>s</unit><ucd>time.period.rotation</ucd><dataType arraysize="2" xsi:type="vs:SimpleDataType">real</dataType></param><param std="true"><name>responseformat</name><description>File format requested for output.</description><ucd>meta.code.mime</ucd><dataType arraysize="*" xsi:type="vs:SimpleDataType">char</dataType></param><param std="true"><name>maxrec</name><description>Maximum number of records returned. Pass 0 to retrieve service parameters.</description><dataType xsi:type="vs:SimpleDataType">integer</dataType></param><param std="true"><name>verb</name><description>Exhaustiveness of column selection. VERB=1 only returns the most important columns, VERB=2 selects the columns deemed useful to the average user, VERB=3 returns a table with all available columns.</description><dataType xsi:type="vs:SimpleDataType">integer</dataType></param></interface><maxSR>180</maxSR><maxRecords>100000</maxRecords><verbosity>true</verbosity><testQuery><ra>170.3128</ra><dec>-60.623786</dec><sr>0.001</sr></testQuery></capability><capability standardID="ivo://ivoa.net/std/VOSI#capabilities"><interface role="std" xsi:type="vs:ParamHTTP"><accessURL use="full">https://dachs.fai.kz/pulsars/q/scs/capabilities</accessURL></interface></capability><capability standardID="ivo://ivoa.net/std/VOSI#availability"><interface role="std" xsi:type="vs:ParamHTTP"><accessURL use="full">https://dachs.fai.kz/pulsars/q/scs/availability</accessURL></interface></capability><capability standardID="ivo://ivoa.net/std/VOSI#tables"><interface role="std" version="1.1" xsi:type="vs:ParamHTTP"><accessURL use="full">https://dachs.fai.kz/pulsars/q/scs/tableMetadata</accessURL></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface role="std" version="1.1" xsi:type="vs:ParamHTTP"><accessURL use="full">https://dachs.fai.kz/tap</accessURL></interface></capability><coverage><spatial>6/1196 1796 3035 3149 3308 3632 3687 3728-3729 14057 14251 14410 14437
14452 14664 14677 15305 15367 15476 15639 15683 21690 24325 24451
28831 28875 28896 28925 29115 29461 29504 29529 30239 30244 30257
30262 30271 30331 30400 30417 30598 30618 30625 30629 30719 37363
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X-ray pulsars in high-mass X-ray binary (HMXB) systems, classified
into 18 persistent and 64 transient sources. Key parameters include
spin periods, spin evolution (local and global trends), orbital
periods, X-ray luminosities, magnetic fields, distances, and detailed
companion star characteristics. The data have been compiled through
cross-matching with recent HMXB catalogs and databases such as Fortin
et al. (2023), Neumann et al. (2023), and Krivonos et al. (2022),
supplemented with literature and SIMBAD database analysis. The catalog
aims to support studies on stellar evolution, accretion processes, and
binary dynamics.</description><table><name>pulsars.main</name><description> This catalog contains data on the Galactic population of 82 confirmed
X-ray pulsars in high-mass X-ray binary (HMXB) systems, classified
into 18 persistent and 64 transient sources. Key parameters include
spin periods, spin evolution (local and global trends), orbital
periods, X-ray luminosities, magnetic fields, distances, and detailed
companion star characteristics. The data have been compiled through
cross-matching with recent HMXB catalogs and databases such as Fortin
et al. (2023), Neumann et al. (2023), and Krivonos et al. (2022),
supplemented with literature and SIMBAD database analysis. The catalog
aims to support studies on stellar evolution, accretion processes, and
binary dynamics.</description><nrows>81</nrows><column><name>number</name><description>Catalog number of the object</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>name</name><description>Name of the object</description><ucd>meta.id</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>ra</name><description>The pulsar's ICRS right ascension from SIMBAD</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>indexed</flag><flag>nullable</flag></column><column><name>dec</name><description>The pulsar's ICRS declenation from SIMBAD</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>indexed</flag><flag>nullable</flag></column><column><name>ps</name><description>Spin period of the 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