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<ri:Resource created="2022-10-10T07:46:28Z" 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>Properties of 125 M-dwarfs in the southern CVZ</title><shortName>J/AJ/163/257</shortName><identifier>ivo://CDS.VizieR/J/AJ/163/257</identifier><altIdentifier>doi:10.26093/cds/vizier.51630257</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Anthony F.</name></creator><creator><name>Nunez A.</name></creator><creator><name>Agueros M.A.</name></creator><creator><name>Curtis J.L.</name></creator><creator><name>do Nascimento J.-D. Jr,Machado J.M.</name></creator><creator><name>Mann A.W.</name></creator><creator><name>Newton E.R.</name></creator><creator><name>Rampalli R.</name></creator><creator><name>Thao Pa C.</name></creator><creator><name>Wood M.L.</name></creator><date role="Updated">2022-11-09T06:06:53Z</date><date role="Created">2022-10-10T07:46:28Z</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>dwarf-stars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>infrared-astronomy</subject><subject>stellar-masses</subject><description>The evolution of magnetism in late-type dwarfs remains murky, as we can only weakly predict levels of activity for M dwarfs of a given mass and age. We report results from our spectroscopic survey of M dwarfs in the Southern Continuous Viewing Zone (CVZ) of the Transiting Exoplanet Survey Satellite (TESS). As the TESS CVZs overlap with those of the James Webb Space Telescope, our targets constitute a legacy sample for studies of nearby M dwarfs. For 122 stars, we obtained at least one R~2000 optical spectrum with which we measure chromospheric H{alpha} emission, a proxy for magnetic field strength. The fraction of active stars is consistent with what is expected for field M dwarfs; as in previous studies, we find that late-type M dwarfs remain active for longer than their early-type counterparts. While the TESS light curves for ~20% of our targets show modulations consistent with rotation, TESS systematics are not well enough understood for confident measurements of rotation periods (Prot) longer than half the length of an observing sector. We report periods for 12 stars for which we measure Prot&lt;~15days or find confirmation for the TESS-derived Prot in the literature. Our sample of 21 Prot, which includes periods from the literature, is consistent with our targets being spun-down field stars. Finally, we examine the H{alpha}-to- bolometric luminosity distribution for our sample. Two stars are rotating fast enough to be magnetically saturated, but are not, hinting at the possibility that fast rotators may appear inactive in H{alpha}.</description><source format="bibcode">2022AJ....163..257A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/163/257</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/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/38">IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/352">I/352 : Distances to 1.47 billion stars in Gaia EDR3 (Bailer-Jones+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/327/1039">J/A+A/327/1039 : Structure and evolution of low-mass stars (Chabrier+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/331/581">J/A+A/331/581 : Rotation and activity in field M dwarfs (Delfosse+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/426">J/AJ/128/426 : Subdwarfs in the SDSS (West+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/646/297">J/ApJ/646/297 : Spitzer observations of pre-main-sequence stars (Rebull+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/407/465">J/MNRAS/407/465 : Fast-rotating M dwarfs in NGC2516 (Jackson+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/97">J/AJ/141/97 : SDSS DR7 M dwarfs (West+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/743/48">J/ApJ/743/48 : Stars with rotation periods &amp; Xray luminosities (Wright+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/93">J/AJ/144/93 : Close white dwarf + M dwarf binaries (WD+dM) (Morgan+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/143/93">J/AJ/143/93 : Rotational velocities in early-M stars (Reiners+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/795/161">J/ApJ/795/161 : Activity &amp; rotation in Praesepe and the Hyades (Douglas+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/807/45">J/ApJ/807/45 : Potent. habitable planets orbiting M dwarfs (Dressing+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/809/161">J/ApJ/809/161 : X-ray obs. and membership probabilities of M37 (Nunez+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/149/158">J/AJ/149/158 : The BUD sample. 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