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<ri:Resource created="2024-09-25T13:24:53Z" 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>Stellar properties &amp; RV variability for M-dwarfs</title><shortName>J/AJ/166/11</shortName><identifier>ivo://CDS.VizieR/J/AJ/166/11</identifier><altIdentifier>doi:10.26093/cds/vizier.51660011</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pass E.K.</name></creator><creator><name>Winters J.G.</name></creator><creator><name>Charbonneau D.</name></creator><creator><name>Irwin J.M.</name></creator><creator><name>Latham D.W.,Berlind P.</name></creator><creator><name>Calkins M.L.</name></creator><creator><name>Esquerdo G.A.</name></creator><creator><name>Mink J.</name></creator><date role="Updated">2025-01-24T20:10:48Z</date><date role="Created">2024-09-25T13:24:53Z</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>m-stars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>radial-velocity</subject><subject>surveys</subject><description>Cold Jovian planets play an important role in sculpting the dynamical environment in which inner terrestrial planets form. The core accretion model predicts that giant planets cannot form around low-mass M-dwarfs, although this idea has been challenged by recent planet discoveries. Here, we investigate the occurrence rate of giant planets around low-mass (0.1-0.3M{sun}) M-dwarfs. We monitor a volume-complete, inactive sample of 200 such stars located within 15pc, collecting four high-resolution spectra of each M-dwarf over six years and performing intensive follow-up monitoring of two candidate radial velocity variables. We use TRES on the 1.5m telescope at the Fred Lawrence Whipple Observatory and CHIRON on the Cerro Tololo Inter-American Observatory 1.5m telescope for our primary campaign, and MAROON-X on Gemini-North for high-precision follow up. We place a 95% confidence upper limit of 1.5% (68% confidence limit of 0.57%) on the occurrence of MP sini&gt;1MJ giant planets out to the water snow line and provide additional constraints on the giant planet population as a function of MP sini and period. Beyond the snow line (100K&lt;Teq&lt;150K), we place 95% confidence upper limits of 1.5%, 1.7%, and 4.4% (68% confidence limits of 0.58%, 0.66%, and 1.7%) for 3MJ&lt;MP sini&lt;10MJ, 0.8MJ&lt;MP sini&lt;3MJ, and 0.3 MJ&lt;MP sini&lt;0.8 MJ giant planets, respectively; i.e., Jupiter analogs are rare around low-mass M-dwarfs. In contrast, surveys of Sun-like stars have found that their giant planets are most common at these Jupiter-like instellations.</description><source format="bibcode">2023AJ....166...11P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/166/11</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/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/407/1157">J/A+A/407/1157 : UVES sky atlas (Hanuschik+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/622/1102">J/ApJ/622/1102 : The planet-metallicity correlation. 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