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<ri:Resource created="2026-05-12T17:02:25Z" status="active" updated="2026-05-19T14:14:26Z" 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>HD 161098 RVs and activity indicators</title><shortName>J/A+A/709/A123</shortName><identifier>ivo://CDS.VizieR/J/A+A/709/A123</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Nari N.</name></creator><creator><name>Suarez Mascareno A.</name></creator><creator><name>Gonzalez Hernandez J.I.</name></creator><creator><name>Stefanov A.K.,Rebolo R.</name></creator><creator><name>Mestre J.M.</name></creator><creator><name>Dumusque X.</name></creator><creator><name>Cretignier M.</name></creator><creator><name>Passegger V.M.,Mignon L.</name></creator><creator><name>Manni F.</name></creator><creator><name>De Amorim R.G.S.B.</name></creator><date role="Updated">2026-05-19T14:14:26Z</date><date role="Created">2026-05-12T17:02:25Z</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>multiple-stars</subject><subject>exoplanets</subject><subject>radial-velocity</subject><subject>visible-astronomy</subject><description>The development of refined instruments and techniques for a detailed analysis of the radial velocities (RVs) of stars other than the Sun allows the presence of planetary signals of amplitude below 1m/s to be investigated. Long-term RV surveys allow the detection of Earth-like and super-Earth-like planets in the habitable zones of Sun-like stars, prime targets for future missions for the atmospheric characterization of exoplanets. We present the analysis of the nearby G8 V-type star HD 161098 (V=7.68mag, d=29.75pc). We searched for terrestrial planets in the habitable zone. We combined historical datasets with new data collected in an ongoing blind search program with HARPS, HARPS-N, and ESPRESSO. We utilized recently developed tools to extract RVs and to deal with the analysis of stellar activity. We performed a joint analysis of RVs and activity indicators to separate the planetary signals from those related to activity. We detected two sub-m/s1 signals that we claim as candidate planets. We are not able to confirm their nature with certainty. Candidate HD 161098 b has an orbital period of 72.578_-0.060_^+0.059^d and a minimum mass of 3.63+/-0.59M_{Earth}_. HD 161098 c has an orbital period of 682.5_-9.9_^+9.5^d and a minimum mass of 7.8_-1.4_^+1.5^M_{Earth}_. If confirmed, candidate HD 161098 c would reside in the optimistic habitable zone of the star. We find a magnetic cycle of 4090_-130_^+140^d period and a rotation period of 28.22_-0.35_^+0.30^d. Our analysis sets the stage for future observing campaigns of the star, finalized for the confirmation of our results. We are entering the sub-m/s era at long orbital periods with a combination of stellar activity treatment and long-term campaigns.</description><source format="bibcode">2026A&amp;A...709A.123N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/709/A123</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</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/709/A123</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/709/A123</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/709/A123</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/709/A123</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/709/A123</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/709/A123</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"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/709/A123/tablee1</name><description>ESPRESSO time series of RV and activity indicators</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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Wilson chromospheric activity index index</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SMW</name><description>Mt. 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