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<ri:Resource created="2024-06-17T08:05:50Z" 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>The POKEMON Speckle Survey of nearby M dwarfs. II.</title><shortName>J/AJ/167/56</shortName><identifier>ivo://CDS.VizieR/J/AJ/167/56</identifier><altIdentifier>doi:10.26093/cds/vizier.51670056</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Clark C.A.</name></creator><creator><name>van Belle G.T.</name></creator><creator><name>Horch E.P.</name></creator><creator><name>Lund M.B.</name></creator><creator><name>Ciardi D.R.,von Braun K.</name></creator><creator><name>Winters J.G.</name></creator><creator><name>Everett M.E.</name></creator><creator><name>Hartman Z.D.</name></creator><creator><name>Llama J.</name></creator><date role="Updated">2025-01-15T20:07:21Z</date><date role="Created">2024-06-17T08:05:50Z</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>multiple-stars</subject><subject>visible-astronomy</subject><subject>astrometry</subject><description>Stellar multiplicity is correlated with many stellar properties, yet multiplicity measurements have proven difficult for the M-dwarfs the most common type of star in our galaxy-due to their faintness and the fact that a reasonably complete inventory of later M-dwarfs did not exist until recently. We have therefore carried out the Pervasive Overview of "Kompanions" of Every M-dwarf in Our Neighborhood (POKEMON) survey, which made use of the Differential Speckle Survey Instrument on the 4.3m Lowell Discovery Telescope, along with the NN-EXPLORE Exoplanet Stellar Speckle Imager on the 3.5m WIYN telescope. The POKEMON sample is volume limited from M0V through M9V out to 15pc, with additional brighter targets at larger distances. In total, 1125 targets were observed. New discoveries were presented in the first paper in the series. In this second paper in the series, we present all detected companions, gauge our astrometric and photometric precision, and compare our filtered and filterless speckle observations. We find that the majority (58.9%) of the companions we detect in our speckle images are not resolved in Gaia, demonstrating the need for high-resolution imaging in addition to long-term astrometric monitoring. Additionally, we find that the majority (73.2%) of simulated stellar companions would be detectable by our speckle observations. Specifically within 100au, we find that 70.3% of simulated companions are recovered. Finally, we discuss future directions of the POKEMON survey.</description><source format="bibcode">2024AJ....167...56C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/167/56</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/B/wds">B/wds : The Washington Visual Double Star Catalog (Mason+ 2001-2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/129">I/129 : Parallaxes and Proper Motions near SGP (Murray+ 1986)</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/I/311">I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. 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Gaia RP magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dist</name><description>[1.8/96.1]? Distance</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_Dist</name><description>[1/19]? Reference for Dist (1)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>RUWE</name><description>[0.7/39.1]? Gaia DR3 re-normalized unit weight error</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>IPDFMP</name><description>[0/100] Gaia DR3 ipd_frac_multi_peak</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Comp?</name><description>[N/Y] Companion(s) observed by us? (Y)es or (N)o</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="28*">char</dataType><flag>nullable</flag></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/AJ/167/56/table4</name><description>*Properties of companions detected throughout the POKEMON survey - from erratum published in 2024, AJ, 168, 229</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>2MASS designation (HHMMSSss+DDMMSSs; J2000) or name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>l_Filt</name><description>Limit flag on Filt</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Dmag2</name><description>[2/5.6]? Second companion magnitude difference</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>WDS</name><description>WDS designation (HHMMm+DDMM; J2000)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Epoch</name><description>[17.26/20.11] Year of the measurement; Epoch+2000</description><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Filt</name><description>[562/880] Dmag filter</description><unit>nm</unit><ucd>instr.bandpass</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Dfilt</name><description>[40/50]? Dmag filter width</description><unit>nm</unit><ucd>instr.bandwidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>PA1</name><description>[3/357] Position angle</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Sep1</name><description>[0.078/3.43] Angular separation</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_Dmag1</name><description>Limit flag on Dmag1</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Dmag1</name><description>[0/5.32] Magnitude difference</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PA2</name><description>[15/223]? Second companion position angle</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Sep2</name><description>[1.67/3.6]? Second companion angular separation</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_Dmag2</name><description>Limit flag on Dmag2</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table></schema></tableset></ri:Resource>