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<ri:Resource created="2022-12-14T12:57:21Z" 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>Gemini-LIGHTS protoplanetary disks</title><shortName>J/AJ/164/109</shortName><identifier>ivo://CDS.VizieR/J/AJ/164/109</identifier><altIdentifier>doi:10.26093/cds/vizier.51640109</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rich E.A.</name></creator><creator><name>Monnier J.D.</name></creator><creator><name>Aarnio A.</name></creator><creator><name>Laws A.S.E.</name></creator><creator><name>Setterholm B.R.,Wilner D.J.</name></creator><creator><name>Calvet N.</name></creator><creator><name>Harries T.</name></creator><creator><name>Miller C.</name></creator><creator><name>Davies C.L.</name></creator><creator><name>Adams F.C.,Andrews S.M.</name></creator><creator><name>Bae J.</name></creator><creator><name>Espaillat C.</name></creator><creator><name>Greenbaum A.Z.</name></creator><creator><name>Hinkley S.</name></creator><creator><name>Kraus S.,Hartmann L.</name></creator><creator><name>Isella A.</name></creator><creator><name>McClure M.</name></creator><creator><name>Oppenheimer R.</name></creator><creator><name>Perez L.M.</name></creator><creator><name>Zhu Z.</name></creator><date role="Updated">2023-08-25T09:53:54Z</date><date role="Created">2022-12-14T12:57:21Z</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>emission-line-stars</subject><subject>pre-main-sequence-stars</subject><subject>polarimetry</subject><subject>infrared-astronomy</subject><description>We present the complete sample of protoplanetary disks from the Gemini- Large Imaging with the Gemini Planet Imager Herbig/T Tauri Survey, which observed bright Herbig Ae/Be stars and T Tauri stars in near-infrared polarized light to search for signatures of disk evolution and ongoing planet formation. The 44 targets were chosen based on their near- and mid-infrared colors, with roughly equal numbers of transitional, pre-transitional, and full disks. Our approach explicitly did not favor well-known, 'famous' disks or those observed by the Atacama Large Millimeter/submillimeter Array, resulting in a less-biased sample suitable to probe the major stages of disk evolution during planet formation. Our optimized data reduction allowed polarized flux as low as 0.002% of the stellar light to be detected, and we report polarized scattered light around 80% of our targets. We detected point-like companions for 47% of the targets, including three brown dwarfs (two confirmed, one new), and a new super-Jupiter-mass candidate around V1295 Aql. We searched for correlations between the polarized flux and system parameters, finding a few clear trends: the presence of a companion drastically reduces the polarized flux levels, far-IR excess correlates with polarized flux for nonbinary systems, and systems hosting disks with ring structures have stellar masses &lt;3M_{sun}_. Our sample also included four hot, dusty "FS CMa" systems, and we detected large-scale (&gt;100au) scattered light around each, signs of extreme youth for these enigmatic systems. 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