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<ri:Resource created="2016-08-04T17:04:39Z" status="active" updated="2025-06-13T15:25:00Z" 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>Parallaxes for 1507 nearby mid-to-late M dwarfs</title><shortName>J/ApJ/784/156</shortName><identifier>ivo://CDS.VizieR/J/ApJ/784/156</identifier><altIdentifier>doi:10.26093/cds/vizier.17840156</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Dittmann J.A.</name></creator><creator><name>Irwin J.M.</name></creator><creator><name>Charbonneau D.</name></creator><creator><name>Berta-Thompson Z.K.</name></creator><date role="Updated">2017-12-18T07:57:23Z</date><date role="Created">2016-08-04T17:04:39Z</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>dwarf-stars</subject><subject>m-stars</subject><subject>stellar-masses</subject><subject>visible-astronomy</subject><subject>trigonometric-parallax</subject><subject>stellar-radii</subject><subject>astronomical-object-identification</subject><description>The MEarth survey is a search for small rocky planets around the smallest, nearest stars to the Sun as identified by high proper motion with red colors. We augmented our planetary search time series with lower cadence astrometric imaging and obtained two million images of approximately 1800 stars suspected to be mid-to-late M dwarfs. We fit an astrometric model to MEarth's images for 1507 stars and obtained trigonometric distance measurements to each star with an average precision of 5mas. Our measurements, combined with the Two Micron All Sky Survey photometry, allowed us to obtain an absolute K_s_ magnitude for each star. In turn, this allows us to better estimate the stellar parameters than those obtained with photometric estimates alone and to better prioritize the targets chosen to monitor at high cadence for planetary transits. The MEarth sample is mostly complete out to a distance of 25pc for stars of type M5.5V and earlier, and mostly complete for later type stars out to 20pc. We find eight stars that are within 10pc of the Sun for which there did not exist a published trigonometric parallax distance estimate. We release with this work a catalog of the trigonometric parallax measurements for 1507 mid-to-late M dwarfs, as well as new estimates of their masses and radii.</description><source format="bibcode">2014ApJ...784..156D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/784/156</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/311">I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/298">I/298 : LSPM-North proper-motion catalog nearby stars (Lepine+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/279">I/279 : Revised Luyten Half-Second Catalogue (Bakos+ 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/239">I/239 : The Hipparcos and Tycho Catalogues (ESA 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/238">I/238 : Yale Trigonometric Parallaxes, Fourth Edition (van Altena+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/70">V/70 : Nearby Stars, Preliminary 3rd Version (Gliese+ 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/98">I/98 : NLTT Catalogue (Luyten, 1979)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/87">I/87 : LHS Catalogue, 2nd Edition (Luyten 1979)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/758/56">J/ApJ/758/56 : Young M dwarfs within 25pc. II. Kinematics (Shkolnik+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/757/112">J/ApJ/757/112 : Stellar diameters. II. K and M-stars (Boyajian+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/754/44">J/ApJ/754/44 : The AstraLux Large M-dwarf Survey (Janson+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/138">J/AJ/142/138 : All-sky catalog of bright M dwarfs (Lepine+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/1680">J/AJ/130/1680 : LSPM-North proper-motion catalog nearby stars (Lepine+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/582/1011">J/ApJ/582/1011 : Revised NLTT Catalog (Salim+, 2003)</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/ApJ/784/156</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/784/156</mirrorURL><mirrorURL title="VizieR at 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>LSPM</name><description>LSPM North Catalog designation (Lepine &amp; Shara 2005, cat. I/298) (JHHMM+DDMMW)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>Gl</name><description>Identifier in Gliese catalog (Gliese et al. 1991, cat. V/70)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>m_Gl</name><description>Component on Gl (A, AB, AC, B, or C)</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>LHS</name><description>Identifier in LHS catalog (1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>NLTT</name><description>[309/58828]? NLTT catalog number (2)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>S03</name><description>Simbad column added by the CDS</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>RAJ2000</name><description>Hour of Right Ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>pmRA</name><description>[-3.9/3.5] Proper motion in RA*cos(DE) ({mu}_RA_*cos(decl.)) from our best fit model</description><unit>arcsec/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pmDE</name><description>[-5.2/10.4] Proper motion in Declination ({mu}_Dec_) from our best fit model</description><unit>arcsec/yr</unit><ucd>pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Date0</name><description>[2008.75/2012.75] Julian epoch of first data point in our fit</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Date1</name><description>[2010.25/2013.5] Julian epoch of last data point in our fit</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>plxrel</name><description>[5.7/546.4] Relative trigonometric parallax</description><unit>mas</unit><ucd>pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pcorr</name><description>[0.8/4.3] Absolute parallax correction (see Section 3.2 for details)</description><unit>mas</unit><ucd>arith.factor</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>plxabs</name><description>[6.9/547.4] Absolute trigonometric parallax</description><unit>mas</unit><ucd>pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_plxabs</name><description>[0/26.7] Error in plxabs</description><unit>mas</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Jmag</name><description>[5.24/12.86] 2MASS J band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Kmag</name><description>[4.02/12.86] 2MASS Ks band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mass</name><description>[0.074/0.792] MEarth estimated mass (3)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rad</name><description>[0.137/0.772] MEarth estimated radius (4)</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Rad</name><description>[0.007/0.039] Error in Rad (5)</description><unit>solRad</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ns</name><description>[7/90] Number of reference stars used in our fit</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Tel</name><description>[1/8] MEarth Telescope number data was taken on (from 1 to 8) (6)</description><ucd>meta.number;instr.tel</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>