<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="1997-12-09T17:46:05Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Galilean satellites mutual events in 1997</title><shortName>J/A+A/314/312</shortName><identifier>ivo://CDS.VizieR/J/A+A/314/312</identifier><altIdentifier>doi:10.26093/cds/vizier.33140312</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Arlot J.-E.</name></creator><date role="Updated">2021-02-22T08:30:00Z</date><date role="Created">1997-12-09T17:46:05Z</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>solar-system-planets</subject><subject>occultation</subject><description>This paper provides the predictions of the mutual phenomena of the Galilean satellites which will occur in 1997. Past experiences have shown the interest of the observation of such events very rare, since they occur only every 6 years when the Earth and the Sun pass through the common orbital plane of the Galilean satellites.</description><source format="bibcode">1996A&amp;A...314..312A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/314/312</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/125/399">J/A+AS/125/399 : Mutual phenomena of the Galilean satellites (Arlot+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/383/719">J/A+A/383/719 : Galilean Satellites mutual events 2002-2003 (Arlot, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/383/724">J/A+A/383/724 : 1999-2000 CCD obs. of inner Jovian moons (Kulyk+, 2002)</relatedResource><relatedResource>http://www.bdl.fr : Website</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/A+A/314/312</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/314/312</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/314/312</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/314/312</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/314/312</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/314/312</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/></coverage><tableset><schema><name>default</name><table><name>J/A+A/314/312/table1-9</name><description>*Mutual events: predictions with G-5 ephemeris</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MaxY</name><description>Maximum of magnitude drop (year)</description><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MaxM</name><description>Maximum of magnitude drop (month)</description><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MaxD</name><description>Maximum of magnitude drop (day)</description><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Event</name><description>Type of event (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Maxh</name><description>Maximum of magnitude drop (hour)</description><unit>h</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Maxm</name><description>Maximum of magnitude drop (min)</description><unit>min</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Maxs</name><description>Maximum of magnitude drop (sec)</description><unit>s</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Mag</name><description>? Light flux drop at the time of the minimum of light (2)</description><ucd>phys.composition.massLightRatio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Duration</name><description>? Duration of the event</description><unit>s</unit><ucd>time.duration</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>n_Duration</name><description>? [1] Note on duration (3)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>DistJup</name><description>? Distance of the eclipsed or occulted satellite to the center of Jupiter in Jovian radii in order to know the configuration during the observation</description><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Impact</name><description>Impact parameter i.e. the minimum distance between the satellites during the event (distance to the shadow cone for eclipse)</description><unit>arcsec</unit><ucd>pos.angDistance;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>