<?xml version='1.0'?><?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?><ri:Resource created="2017-08-28T12:55:00Z" status="active" updated="2025-02-26T11:00:35Z" version="1.2" xmlns:g-colstat="http://dc.g-vo.org/ColStats-1" 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://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/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:CatalogResource"><title>Mars Craters</title><shortName>mars_craters.epn</shortName><identifier>ivo://padc.obspm.planeto/mars_craters/q/epn_core</identifier><curation><publisher>Paris Astronomical Data Centre - Constructor University</publisher><creator><name>Minin, M.</name></creator><date role="Updated">2025-02-26T10:57:20Z</date><contact><name>PADC support team</name><address>77 av. Denfert Rochereau, 75014 Paris, FRANCE</address><email>vo.paris@obspm.fr</email><telephone>0033140512082</telephone></contact></curation><content><subject>solar-system-astronomy</subject><subject>planetary-science</subject><subject>planetary-geology</subject><subject>craters</subject><subject>mars</subject><description> The Mars Crater Catalog by S.J. Robbins was generated from THEMIS
Daytime IR and Viking MDIM 2.1 global mosaics of Mars. Craters were
selected using 5 points along the rim. The table is statistically
complete to the diameter of ~1.0 km. The table contains morphologic
and morphometric data for craters with diameter larger than 3 km. The
Prometheus basin has been excluded from the Catalog due to technical
issues.

Reference: "A New Global Database of Mars Impact Craters ≥1 km: (1)
Database Creation, Properties, and Parameters", S.J. Robbins and B.M.
Hynek, Journal of Geophysical Research - Planets, v.117. (2012) DOI:
10.1029/2011JE003966</description><source>https://doi.org/10.1029/2011JE003966</source><referenceURL>http://voparis-tap-planeto.obspm.fr/tableinfo/mars_craters.epn_core</referenceURL><type>Catalog</type><contentLevel>General</contentLevel><contentLevel>University</contentLevel><contentLevel>Research</contentLevel><relationship><relationshipType>Continues</relationshipType><relatedResource ivo-id="ivo://jacobsuni/mars_craters/q/epn_core">mars craters on server jacobsuni</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://padc.obspm.planeto/tap">PADC TAP Server on voparis-tap-planeto.obspm.fr TAP service</relatedResource></relationship></content><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface role="std" version="1.1" xsi:type="vs:ParamHTTP"><accessURL use="full">http://voparis-tap-planeto.obspm.fr/tap</accessURL></interface></capability><facility>Mars Odyssey Orbiter</facility><instrument>THEMIS Daytime IR</instrument><tableset><schema><name>mars_craters</name><title>Mars Craters</title><description> The Mars Crater Catalog by S.J. Robbins was generated from THEMIS
Daytime IR and Viking MDIM 2.1 global mosaics of Mars. Craters were
selected using 5 points along the rim. The table is statistically
complete to the diameter of ~1.0 km. The table contains morphologic
and morphometric data for craters with diameter larger than 3 km. The
Prometheus basin has been excluded from the Catalog due to technical
issues.

Reference: "A New Global Database of Mars Impact Craters ≥1 km: (1)
Database Creation, Properties, and Parameters", S.J. Robbins and B.M.
Hynek, Journal of Geophysical Research - Planets, v.117. (2012) DOI:
10.1029/2011JE003966</description><table><name>mars_craters.epn_core</name><description> The Mars Crater Catalog by S.J. Robbins was generated from THEMIS
Daytime IR and Viking MDIM 2.1 global mosaics of Mars. Craters were
selected using 5 points along the rim. The table is statistically
complete to the diameter of ~1.0 km. The table contains morphologic
and morphometric data for craters with diameter larger than 3 km. The
Prometheus basin has been excluded from the Catalog due to technical
issues.

Reference: "A New Global Database of Mars Impact Craters ≥1 km: (1)
Database Creation, Properties, and Parameters", S.J. Robbins and B.M.
Hynek, Journal of Geophysical Research - Planets, v.117. (2012) DOI:
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