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<ri:Resource created="2025-07-08T08:27:41Z" status="active" updated="2026-07-02T11:44:58Z" 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>Coronographic observations for M dwarfs companions</title><shortName>J/AJ/168/215</shortName><identifier>ivo://CDS.VizieR/J/AJ/168/215</identifier><altIdentifier>doi:10.26093/cds/vizier/be-58-6q</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sanghi A.</name></creator><creator><name>Xuan J.W.</name></creator><creator><name>Wang J.J.</name></creator><creator><name>Mawet D.</name></creator><creator><name>Bowler B.P.</name></creator><creator><name>Ngo H.,Bryan M.L.</name></creator><creator><name>Ruane G.</name></creator><creator><name>Absil O.</name></creator><creator><name>Huby E.</name></creator><date role="Updated">2026-07-02T11:44:58Z</date><date role="Created">2025-07-08T08:27:41Z</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>dwarf-stars</subject><subject>m-stars</subject><subject>infrared-astronomy</subject><subject>visible-astronomy</subject><description>We present Super-RDI, a unique framework for the application of reference star differential imaging (RDI) to Keck/NIRC2 high-contrast imaging observations with the vortex coronagraph. Super-RDI combines frame selection and signal-to-noise ratio (S/N) optimization techniques with a large multiyear reference point-spread function (PSF) library to achieve optimal PSF subtraction at small angular separations. We compile a ~7000 frame reference PSF library based on a set of 288 new Keck/NIRC2 L' sequences of 237 unique targets acquired between 2015 and 2019 as part of two planet-search programs designed for RDI, one focusing on nearby young M dwarfs and the other targeting members of the Taurus star-forming region. For our data set, synthetic companion injection-recovery tests reveal that frame selection with the mean-squared error metric combined with Karhunen-Loeve Image-Processing-based PSF subtraction using 1000-3000 frames and &lt;500 principal components yields the highest average S/N for injected synthetic companions. We uniformly reduce targets in the young M-star survey with both Super-RDI and angular differential imaging (ADI). For the typical parallactic angle rotation of our data set (~10{deg}), Super-RDI performs better than a widely used implementation of ADI-based PSF subtraction at separations &lt;=0.4" (~=5{lambda}/D), gaining an average of 0.25mag in contrast at 0.25" and 0.4mag in contrast at 0.15". This represents a performance improvement in separation space over RDI with single-night reference star observations (~100 frame PSF libraries) applied to a similar Keck/NIRC2 data set in previous work. We recover two known brown dwarf companions and provide detection limits for 155 targets in the young M-star survey. Our results demonstrate that increasing the PSF library size with careful selection of reference frames can improve the performance of RDI with the Keck/NIRC2 vortex coronagraph in L'.</description><source format="bibcode">2024AJ....168..215S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/168/215</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/III/198">III/198 : Palomar/MSU nearby star spectroscopic survey (Hawley+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/237">II/237 : Stellar Photometry in Johnson's 11-color syst. 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