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<ri:Resource created="2022-10-21T07:22:23Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Absolute &amp; relative astrometry for {epsilon} Indi B</title><shortName>J/AJ/163/288</shortName><identifier>ivo://CDS.VizieR/J/AJ/163/288</identifier><altIdentifier>doi:10.26093/cds/vizier.51630288</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chen M.</name></creator><creator><name>Li Y.</name></creator><creator><name>Brandt T.D.</name></creator><creator><name>Dupuy T.J.</name></creator><creator><name>Cardoso C.V.</name></creator><creator><name>McCaughrean M.J.</name></creator><date role="Updated">2024-02-13T12:07:35Z</date><date role="Created">2022-10-21T07:22:23Z</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>exoplanets</subject><subject>multiple-stars</subject><subject>dwarf-stars</subject><subject>astrometry</subject><subject>infrared-photometry</subject><description>We report individual dynamical masses of 66.92{+/-}0.36 MJup and 53.25{+/-}0.29MJup for the binary brown dwarfs {epsilon} Indi Ba and Bb, measured from long-term (~10yr) relative orbit monitoring and absolute astrometry monitoring data on the Very Large Telescope (VLT). Relative astrometry with NACO fully constrains the Keplerian orbit of the binary pair, while absolute astrometry with FORS2 measures the system's parallax and mass ratio. We find a parallax consistent with the Hipparcos and Gaia values for {epsilon} Indi A, and a mass ratio for {epsilon} Indi Ba to Bb precise to better than 0.2%. {epsilon} Indi Ba and Bb have spectral types T1-1.5 and T6, respectively. With an age of 3.5_-1.0_^+0.8^Gyr from {epsilon} Indi A's activity, these brown dwarfs provide some of the most precise benchmarks for substellar cooling models. Assuming coevality, the very different luminosities of the two brown dwarfs and our moderate mass ratio imply a steep mass-luminosity relationship (L{prop}M^5.37{+/-}0.08^) that can be explained by a slowed cooling rate in the L/T transition, as previously observed for other L/T binaries. Finally, we present a periodogram analysis of the near-infrared photometric data, but find no definitive evidence of periodic signals with a coherent phase.</description><source format="bibcode">2022AJ....163..288C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/163/288</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/B/pastel">B/pastel : The PASTEL catalogue (Soubiran+, 2016-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IX/10">IX/10 : ROSAT All-Sky Bright Source Catalogue (1RXS) (Voges+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/259">I/259 : The Tycho-2 Catalogue (Hog+ 2000)</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/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/348/897">J/A+A/348/897 : Ages of main-sequence stars (Lachaume+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/161">J/AJ/132/161 : NStars project; The southern sample. 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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>Obs</name><description>[2005/2016] Astrometry date, year</description><ucd>time.epoch</ucd></column><column><name>Nframes</name><description>[1/30] Number of frames</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Band</name><description>[I] Band</description><ucd>instr.bandpass</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Texp</name><description>[20/600] Total integration</description><unit>s</unit><ucd>time</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/AJ/163/288/table3</name><description>Relative astrometry results</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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