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<ri:Resource created="2016-05-30T12:07:19Z" 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>MEarth photometry: nearby M-dwarf magnitudes</title><shortName>J/ApJ/818/153</shortName><identifier>ivo://CDS.VizieR/J/ApJ/818/153</identifier><altIdentifier>doi:10.26093/cds/vizier.18180153</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>Newton E.R.</name></creator><date role="Updated">2017-06-12T08:24:56Z</date><date role="Created">2016-05-30T12:07:19Z</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>photometry</subject><subject>metallicity</subject><subject>infrared-sources</subject><subject>surveys</subject><description>The MEarth Project is a photometric survey systematically searching the smallest stars near the Sun for transiting rocky planets. Since 2008, MEarth has taken approximately two million images of 1844 stars suspected to be mid-to-late M dwarfs. We have augmented this survey by taking nightly exposures of photometric standard stars and have utilized this data to photometrically calibrate the MEarth system, identify photometric nights, and obtain an optical magnitude with 1.5% precision for each M dwarf system. Each optical magnitude is an average over many years of data, and therefore should be largely immune to stellar variability and flaring. We combine this with trigonometric distance measurements, spectroscopic metallicity measurements, and 2MASS infrared magnitude measurements in order to derive a color-magnitude-metallicity relation across the mid-to-late M dwarf spectral sequence that can reproduce spectroscopic metallicity determinations to a precision of 0.1 dex. We release optical magnitudes and metallicity estimates for 1567 M dwarfs, many of which did not have an accurate determination of either prior to this work. For an additional 277 stars without a trigonometric parallax, we provide an estimate of the distance, assuming solar neighborhood metallicity. We find that the median metallicity for a volume-limited sample of stars within 20pc of the Sun is [Fe/H]=-0.03+/-0.008, and that 29/565 of these stars have a metallicity of [Fe/H]=-0.5 or lower, similar to the low-metallicity distribution of nearby G dwarfs. When combined with the results of ongoing and future planet surveys targeting these objects, the metallicity estimates presented here will be important for assessing the significance of any putative planet-metallicity correlation.</description><source format="bibcode">2016ApJ...818..153D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/818/153</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/298">I/298 : LSPM-North Catalog (Lepine+ 2005)</relatedResource><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/J/A+A/577/A128">J/A+A/577/A128 : CARMENES input catalog of M dwarfs. 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32595 32596 32602 32623 32627 32643 32658 32679 32686 32699 32707 32708 32712 32749 32753 32761</spatial><spectral>8.650015785639275e-20 1.7003137259100215e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/818/153?format=ascii</footprint><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/818/153/table2</name><description>Nightly photometric coefficients</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>Date</name><description>Observing date</description><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>k2</name><description>[-1.93/13.3] Color coefficient, k2 (1)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>k1</name><description>[-225.5/489.6] Airmass coefficient, k1 (1)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>ZP</name><description>[-80.5/322.6] Zero point, z_i_ (1)</description><unit>mag</unit><ucd>phot.mag;arith.zp</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tel</name><description>MEarth telescope number (tel01-tel08)</description><ucd>meta.number;instr.tel</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column></table><table><name>J/ApJ/818/153/table3</name><description>MEarth magnitudes of Landolt standards</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>Name</name><description>Name of Landolt standard</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>mag</name><description>[9.2/13.3] MEarth magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_mag</name><description>[0.02/0.07] MEarth magnitude error</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Position from SIMBAD (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Position from SIMBAD (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJ/818/153/table5</name><description>Color-magnitude sequence at [Fe/H]=-0.1 and [Fe/H]=0.0</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>Color</name><description>[2.1/3.4] MEarth-2MASS K color index</description><ucd>phot.color;em.opt;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>K1Mag</name><description>[6.4/10] Absolute 2MASS K magnitude for -0.1 metallicity</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>K0Mag</name><description>[5.9/10] Absolute 2MASS K magnitude for 0.0 metallicity</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/ApJ/818/153/table4</name><description>Observed properties of the MEarth targets</description><column><name>SpT</name><description>MK spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>r_F3</name><description>Source for flag 3</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><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>2MASS</name><description>2MASS ID (HHMMSSss+DDMMSSs; J2000)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>LSPM</name><description>LSPM-North ID (JHHMM+DDMMW)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>mag</name><description>[6.6/15.2] MEarth magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_mag</name><description>[0.005/0.2] MEarth magnitude error</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Jmag</name><description>[5.2/12.9] 2MASS J magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Jmag</name><description>? 2MASS J error</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Hmag</name><description>[4.8/12.3] 2MASS H magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Hmag</name><description>? 2MASS H error</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Kmag</name><description>[4.5/11.9] 2MASS Ks magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Kmag</name><description>? 2MASS Ks error</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Plx</name><description>[0.007/0.6]? Trigonometric parallax</description><unit>arcsec</unit><ucd>pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Plx</name><description>[0/0.02]? Trigonometric parallax error</description><unit>arcsec</unit><ucd>stat.error;pos.parallax</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>r_Plx</name><description>Reference for trigonometric parallax</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>r_SpT</name><description>Reference for spectral type</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>FeHsp</name><description>[-0.9/0.9]? Spectroscopic metallicity</description><unit>log(Sun)</unit><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_FeHsp</name><description>[0.1/0.3]? Spectroscopic metallicity error</description><unit>log(Sun)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FeHph</name><description>[-1.1/0.7]? Metallicity from our photometric relation</description><unit>log(Sun)</unit><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DM</name><description>[-0.7/4.8]? Distance modulus (assuming metallicity =-0.1 from this work)</description><ucd>phot.mag.distMod</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F1</name><description>[0/1]? Flag 1 for possible contaminating light (1=True) (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>F2</name><description>[0/1]? Flag 2 for possible contaminating light (1=True) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>F3</name><description>[0/1]? Flag 3 for possible contaminating light (1=True) (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>FirstJD</name><description>Julian date of 1st photometric data point</description><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>LastJD</name><description>Julian date of last photometric data point</description><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ndata</name><description>[14/7752] Total number of data points on photometric nights</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Flag</name><description>[0/1] Flag whether source appears to be over luminous (1=True) (4)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>W15</name><description>Display data from West+, 2015, J/ApJ/812/3, if any</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Positions from 2MASS names (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Positions from 2MASS names (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJ/818/153/table1</name><description>Quantum Efficiency (QE) of the MEarth CCD, and filter throughput</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>lambda</name><description>[650/1000] Wavelength of filter (nanometer)</description><unit>nm</unit><ucd>em.wl;instr.filter</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>QE</name><description>[0.15/0.91] Quantum Efficiency of the MEarth CCD</description><ucd>instr.det.qe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Trans</name><description>[0/1] Transmission of the filter</description><ucd>phys.transmission;instr.filter</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Prod</name><description>[0/0.8] Product</description><ucd>phys.transmission;instr.filter</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>