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<ri:Resource created="2019-11-19T07:58:53Z" 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>Adaptative optic images of WISE YSO candidates</title><shortName>J/ApJ/868/43</shortName><identifier>ivo://CDS.VizieR/J/ApJ/868/43</identifier><altIdentifier>doi:10.26093/cds/vizier.18680043</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Silverberg S.M.</name></creator><creator><name>Kuchner M.J.</name></creator><creator><name>Wisniewski J.P.</name></creator><creator><name>Bans A.S.</name></creator><creator><name>Debes J.H.,Kenyon S.J.</name></creator><creator><name>Baranec C.</name></creator><creator><name>Riddle R.</name></creator><creator><name>Law N.</name></creator><creator><name>Teske J.K.</name></creator><creator><name>Burns-Kaurin E.,Bosch M.K.D.</name></creator><creator><name>Cernohous T.</name></creator><creator><name>Doll K.</name></creator><creator><name>Durantini Luca H.A.</name></creator><creator><name>Hyogo M.,Hamilton J.</name></creator><creator><name>Finnemann J.J.S.</name></creator><creator><name>Lau L. (The Disk Detective Collaboration)</name></creator><date role="Updated">2024-09-05T15:16:07Z</date><date role="Created">2019-11-19T07:58:53Z</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>young-stellar-objects</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>effective-temperature</subject><subject>stellar-distance</subject><description>The Disk Detective citizen science project aims to find new stars with excess 22{mu}m emission from circumstellar dust in the AllWISE data release from the Wide-field Infrared Survey Explorer. We evaluated 261 Disk Detective objects of interest with imaging with the Robo-AO adaptive optics instrument on the 1.5m telescope at Palomar Observatory and with RetroCam on the 2.5m du Pont Telescope at Las Campanas Observatory to search for background objects at 0.15"-12" separations from each target. Our analysis of these data leads us to reject 7% of targets. Combining this result with statistics from our online image classification efforts implies that at most 7.9%+/-0.2% of AllWISE-selected infrared excesses are good disk candidates. Applying our false-positive rates to other surveys, we find that the infrared excess searches of McDonald+ (2012, J/MNRAS/427/343 and 2017, J/MNRAS/471/770) and Marton+ (2016, J/MNRAS/458/3479) all have false-positive rates &gt;70%. Moreover, we find that all 13 disk candidates in Theissen &amp; West (2014, J/ApJ/794/146) with W4 signal-to-noise ratio &gt;3 are false positives. We present 244 disk candidates that have survived vetting by follow-up imaging. Of these, 213 are newly identified disk systems. Twelve of these are candidate members of comoving pairs based on Gaia astrometry, supporting the hypothesis that warm dust is associated with binary systems. We also note the discovery of 22{mu}m excess around two known members of the Scorpius-Centaurus association, and we identify known disk host WISEAJ164540.79-310226.6 as a likely Sco-Cen member. Thirty of these disk candidates are closer than ~125pc (including 26 debris disks), making them good targets for both direct-imaging exoplanet searches.</description><source format="bibcode">2018ApJ...868...43S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/868/43</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/I/259">I/259 : The Tycho-2 Catalogue (Hog+ 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/332">II/332 : c2d Spitzer final data release (DR4) (Evans+, 2003)</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/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/101/117">J/ApJS/101/117 : UBVRIJHKLMNQ photometry in Taurus-Auriga (Kenyon+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/313/43">J/MNRAS/313/43 : OB association members in ACT+TRC Cat. 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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>Zoo</name><description>Zooniverse identifier</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Teff</name><description>[3400/14853] Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Teff</name><description>[31/180] Lower uncertainty in Teff</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>E_Teff</name><description>[32/179] Upper uncertainty in Teff</description><unit>K</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>f_Tdisk</name><description>Limit flag on Tdisk</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Tdisk</name><description>[1/685] Disk temperature</description><unit>K</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Tdisk</name><description>[2/113]? Lower uncertainty in Tdisk</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>E_Tdisk</name><description>[5/125]? Upper uncertainty in Tdisk</description><unit>K</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>l_LIR/L*</name><description>Limit flag on LIR/L*</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>LIR/L*</name><description>[2.5e-05/9.9] IR to stellar luminosity ratio</description><ucd>phys.luminosity;em.IR;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_LIR/L*</name><description>[2e-06/1.5]? 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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>Zoo</name><description>Zooniverse identifier</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Teff</name><description>[2500/12460] Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Teff</name><description>[12/208] Lower uncertainty in Teff</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>E_Teff</name><description>[51/326] Upper uncertainty in Teff</description><unit>K</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>alpha</name><description>[-2.6/0.8]? Spectral index of disk</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_alpha</name><description>[0.01/0.03]? Lower uncertainty in alpha</description><ucd>stat.error;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_alpha</name><description>[0.01/0.03]? Upper uncertainty in alpha</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Tdisk</name><description>[127/1897] Disk temperature</description><unit>K</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Tdisk</name><description>[0.04/102] Lower uncertainty in Tdisk</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_Tdisk</name><description>[0.04/135] Upper uncertainty in Tdisk</description><unit>K</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>LIR/L*</name><description>[0.0002/2.2] IR to stellar luminosity ratio</description><ucd>phys.luminosity;em.IR;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_LIR/L*</name><description>[1e-05/0.1] Lower uncertainty in LIR/L*</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>E_LIR/L*</name><description>[2e-05/0.3] Upper uncertainty in LIR/L*</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>