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<ri:Resource created="2025-11-07T14:46:15Z" status="active" updated="2026-07-02T11:52:09Z" 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>Spectra of AF Lep b using SPHERE &amp; GRAVITY from VLT</title><shortName>J/AJ/169/30</shortName><identifier>ivo://CDS.VizieR/J/AJ/169/30</identifier><altIdentifier>doi:10.26093/cds/vizier/be-59-y</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Balmer W.O.</name></creator><creator><name>Franson K.</name></creator><creator><name>Chomez A.</name></creator><creator><name>Pueyo L.</name></creator><creator><name>Stolker T.</name></creator><creator><name>Lacour S.,Nowak M.</name></creator><creator><name>Nasedkin E.</name></creator><creator><name>Bonse M.J.</name></creator><creator><name>Thorngren D.</name></creator><creator><name>Palma-Bifani P.,Molliere P.</name></creator><creator><name>Wang J.J.</name></creator><creator><name>Zhang Z.</name></creator><creator><name>Chavez A.</name></creator><creator><name>Kammerer J.</name></creator><creator><name>Blunt S.,Bowler B.P.</name></creator><creator><name>Bonnefoy M.</name></creator><creator><name>Brandner W.</name></creator><creator><name>Charnay B.</name></creator><creator><name>Chauvin G.</name></creator><creator><name>Henning T.,Lagrange A.-M.</name></creator><creator><name>Pourre N.</name></creator><creator><name>Rickman E.</name></creator><creator><name>De Rosa R.</name></creator><creator><name>Vigan A.,Winterhalder T.</name></creator><date role="Updated">2026-07-02T11:52:09Z</date><date role="Created">2025-11-07T14:46:15Z</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>interferometry</subject><subject>exoplanets</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><description>Direct imaging observations are biased toward wide-separation, massive companions that have degenerate formation histories. Although the majority of exoplanets are expected to form via core accretion, most directly imaged exoplanets have not been convincingly demonstrated to follow this formation pathway. We obtained new interferometric observations of the directly imaged giant planet AF Lep b with the VLTI/GRAVITY instrument. We present three epochs of ~50uas relative astrometry and the K-band spectrum of the planet for the first time at a resolution of R=500. Using only these measurements, spanning less than 2 months, and the Hipparcos-Gaia Catalogue of Accelerations, we are able to significantly constrain the planet's orbit; this bodes well for interferometric observations of planets discovered by Gaia DR4. Including all available measurements of the planet, we infer an effectively circular orbit (e&lt;0.02, 0.07, and 0.13 at 1{sigma}, 2{sigma}, and 3{sigma}, respectively) in spin-orbit alignment with the host and measure a dynamical mass of Mp=3.75+/-0.5MJup. Models of the spectrum of the planet show that it is metal-rich ([M/H]=0.75+/-0.25), with a C/O abundance encompassing the solar value. This ensemble of results shows that the planet is consistent with core accretion formation.</description><source format="bibcode">2025AJ....169...30B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/169/30</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/I/259">I/259 : The Tycho-2 Catalogue (Hog+ 2000)</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/357">I/357 : Gaia DR3 Part 3. 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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>Lambda</name><description>Wavelength</description><unit>um</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Flux</name><description>1D flux</description><unit>1000W.m**-2.nm**-1</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Contrast</name><description>1D contrast</description><ucd>phot.flux;arith.ratio;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/AJ/169/30/fig2b</name><description>GRAVITY spectrum of AF Lep b (Data behind Figure 2)</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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