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<ri:Resource created="2012-02-02T13:18:46Z" status="active" updated="2026-05-19T14:25:37Z" 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>Photometry and spectroscopy in IC 2391</title><shortName>J/ApJ/706/1484</shortName><identifier>ivo://CDS.VizieR/J/ApJ/706/1484</identifier><altIdentifier>doi:10.26093/cds/vizier.17061484</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Boudreault S.</name></creator><creator><name>Bailer-Jones C.A.L.</name></creator><date role="Updated">2026-05-19T14:25:37Z</date><date role="Created">2012-02-02T13:18:46Z</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>open-star-clusters</subject><subject>photometry</subject><subject>spectroscopy</subject><subject>radial-velocity</subject><subject>m-stars</subject><subject>stellar-masses</subject><subject>effective-temperature</subject><subject>stellar-spectral-types</subject><subject>line-intensities</subject><description>We present the stellar and substellar mass function (MF) of the open cluster IC 2391, plus its radial dependence, and use this to put constraints on the formation mechanism of brown dwarfs (BDs). Our multi-band optical and infrared photometric survey with spectroscopic follow-up covers 11deg^2^, making it the largest survey of this cluster to date. From our preliminary spectroscopic follow-up, to confirm BD status and cluster membership, we find that all candidates are M dwarfs (in either the field or the cluster), demonstrating the efficiency of our photometric selection method in avoiding contaminants (e.g., red giants). About half of our photometric candidates for which we have spectra are spectroscopically confirmed as cluster members; two are new spectroscopically confirmed BD members of IC 2391.</description><source format="bibcode">2009ApJ...706.1484B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/706/1484</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/J/A+A/501/553">J/A+A/501/553 : Equivalent widths of IC 2602 + IC 2391 stars (D'Orazi+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/461/509">J/A+A/461/509 : Membership and spectroscopy of IC 2391 (Platais+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/468/151">J/A+A/468/151 : Nearby open clusters radii and masses (Piskunov+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/430/287">J/A+A/430/287 : XMM observations of IC 2391 stars (Marino+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/355/959">J/MNRAS/355/959 : Proper motions of IC 2391 possible members (Dodd+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/372/862">J/A+A/372/862 : Lithium abundances in IC 2602 and IC 2391 (Randich+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/134/103">J/ApJS/134/103 : Low-mass members of IC 2391 (Barrado y Navascues+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/345/471">J/A+A/345/471 : Memberships of open clusters (Robichon+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/126/357">J/A+AS/126/357 : Members 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