<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2024-11-21T15:55:42Z" 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>Candidate YSOs from JWST ERO obs. of NGC 3324</title><shortName>J/AJ/168/63</shortName><identifier>ivo://CDS.VizieR/J/AJ/168/63</identifier><altIdentifier>doi:10.26093/cds/vizier.51680063</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Crompvoets B.L.</name></creator><creator><name>Di Francesco J.</name></creator><creator><name>Teimoorinia H.</name></creator><creator><name>Preibisch T.</name></creator><date role="Updated">2025-02-18T20:12:43Z</date><date role="Created">2024-11-21T15:55:42Z</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>infrared-photometry</subject><subject>young-stellar-objects</subject><subject>star-forming-regions</subject><description>Among the first observations released to the public from the JWST was a section of the star-forming region NGC 3324 known colloquially as the "Cosmic Cliffs." We build a photometric catalog of the region and test the ability of using the probabilistic random forest machine-learning method to identify its young stellar objects (YSOs). We find 450 candidate YSOs (cYSOs) out of 19497 total objects within the field, 413 of which are cYSOs not found in previous works. These classifications are verified with several different metrics, including recall and precision. Using the obtained probabilities of objects being YSOs, we employ a Monte Carlo approach to determine the surface density of cYSOs in the Cosmic Cliffs, which we find to be largely coincident with column densities derived from Herschel data, up to a column density of 1.37x10^22^cm^-2^. The newly determined number and spatial distribution of YSOs in the Cosmic Cliffs demonstrate that JWST is far more capable of detecting YSOs in dusty regions than Spitzer. Comparisons of the observed colors and brightness of faint cYSOs with those of pre-main-sequence models suggest JWST has detected a significant population of substellar YSOs in the Cosmic Cliffs. The size of this population further suggests previous estimates of star formation efficiencies in molecular clouds have been systematically low.</description><source format="bibcode">2024AJ....168...63C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/168/63</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/ApJS/181/321">J/ApJS/181/321 : Properties of Spitzer c2d dark clouds (Evans+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/184/18">J/ApJS/184/18 : Spitzer survey of young stellar clusters (Gutermuth+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/194/4">J/ApJS/194/4 : Classification of CCCP X-ray sources (Broos+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/539/A143">J/A+A/539/A143 : Nearby B-stars stellar param. and abundances (Nieva+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/549/A67">J/A+A/549/A67 : Embedded YSOs in Carina Nebula complex (Gaczkowski+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/209/31">J/ApJS/209/31 : The MYStIX IR-Excess Source catalog (MIRES) (Povich+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/564/A120">J/A+A/564/A120 : Chandra X-ray observation of Gum 31 (Preibisch+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/220/11">J/ApJS/220/11 : SEDs of Spitzer YSOs in the Gould Belt (Dunham+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/647/A116">J/A+A/647/A116 : YSO candidate catalog from ANN (Cornu+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/507/5106">J/MNRAS/507/5106 : NGC 6822 massive young stellar objects (Kinson+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/254/33">J/ApJS/254/33 : Gal. midplane Spitzer/IRAC cand. YSOs (SPICY) (Kuhn+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/660/A11">J/A+A/660/A11 : Gaia distances to the Carina Nebula Complex (Goeppl+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/517/140">J/MNRAS/517/140 : M33 massive young stellar objects (Kinson+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/165/3">J/AJ/165/3 : SPICY. II. Spectroscopic obs. of 26 YSOs (Kuhn+, 2023)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/168/63</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/168/63</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/168/63</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/168/63</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/168/63</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/168/63</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/AJ/168/63/table3 (Fluxes, J2000 coordinates, and probabilities for sources classified as candidate YSOs)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/168/63/table3?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/168/63/table3?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/168/63/table3?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>159.1862</ra><dec>-58.6801</dec><sr>0.005555555555555556</sr></testQuery></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/AJ/168/63/table4 (Candidate YSOs from other works matched to our candidate YSOs)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/168/63/table4?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/168/63/table4?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/168/63/table4?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>159.217917</ra><dec>-58.635833</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/38018</spatial><spectral>4.0428963483234324e-20 2.46211493093505e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/168/63?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/168/63/table3</name><description>Fluxes, J2000 coordinates, and probabilities for sources classified as candidate YSOs</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Seq</name><description>[0/19496] Sequential object index</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>[159.1/159.31] Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>[-58.7/-58.5] Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>xpix</name><description>[76/14179] X pixel on image (s)</description><unit>pix</unit><ucd>pos.frame</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>ypix</name><description>[65/8373] Y pixel on image (s)</description><unit>pix</unit><ucd>pos.frame</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F090W</name><description>[12.9/28.55]? Flux density in JWST/NIRCam F090W band, Vega magnitudes</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F090W</name><description>[0.01/0.6]? Uncertainty in F090W</description><unit>mag</unit><ucd>stat.error;phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F187N</name><description>[10/25.01]? Flux density in JWST/NIRCam F187N band, Vega magnitudes</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F187N</name><description>[0.01/0.6]? Uncertainty in F187N</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F200W</name><description>[10.5/26.16]? Flux density in JWST/NIRCam F200W band, Vega magnitudes</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F200W</name><description>[0/0.4]? Uncertainty in F200W</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F335M</name><description>[8.15/22.1]? Flux density in JWST/NIRCam F335M band, Vega magnitudes</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F335M</name><description>[0.01/0.6]? Uncertainty in F335M</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PPRFf335m</name><description>Probability of being a YSO based on the PRF model, when the F335M band data are excluded</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>F444W</name><description>[7.7/22.75]? Flux density in JWST/NIRCam F444W band, Vega magnitudes</description><unit>mag</unit><ucd>phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SPICY</name><description>[7423/7481]? SPICY identifier if detected in Kuhn+ 2021, J/ApJS/254/33</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>ClInit</name><description>[0/1]? Initial YSO classification (0=YSO; or 1=contaminant)</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>PPRFf090w</name><description>Probability of being a YSO based on the PRF model, when the F090W band data are excluded</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PRFf090w</name><description>[0/1]? Probability of being a YSO based on the RF model, when the F090W band data are excluded</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PPRFf187n</name><description>[0.0001/1] Probability of being a YSO based on the PRF model, when the F187N band data are excluded</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>PRFf187n</name><description>[0/1]? Probability of being a YSO based on the RF model, when the F187N band data are excluded</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PPRFf200w</name><description>Probability of being a YSO based on the PRF model, when the F200W band data are excluded</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PRFf200w</name><description>[0/1]? Probability of being a YSO based on the RF model, when the F200W band data are excluded</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PRFruns</name><description>[0/1] Fraction of runs where the object is identified as a YSO based on the PRF method (2)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>ClPRF</name><description>[0/1] Final Probabilistic Random Forest YSO classification (0=YSO; or 1=contaminant)</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ProbPRF</name><description>[0/1] PRF Probability of Class</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RFruns</name><description>[0/1] Fraction of runs where the object is identified as a YSO based on the RF method (2)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ClRF</name><description>[0/1]? Final Regular Random Forest YSO classification (0=YSO; or 1=contaminant)</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ProbRF</name><description>[0/1]? RF Probability of Class</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Secure</name><description>Security of classification as YSO or contaminant (3)</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>PRFf335m</name><description>[0/1]? Probability of being a YSO based on the RF model, when the F335M band data are excluded</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PPRFf444w</name><description>Probability of being a YSO based on the PRF model, when the F444W band data are excluded</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PRFf444w</name><description>[0/1]? Probability of being a YSO based on the RF model, when the F444W band data are excluded</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PPRFf470n</name><description>Probability of being a YSO based on the PRF model, when the F470N band data are excluded</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PRFf470n</name><description>[0/1]? Probability of being a YSO based on the RF model, when the F470N band data are excluded</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_F444W</name><description>[0/0.6]? Uncertainty in F444W</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F470N</name><description>[6.7/22.56]? Flux density in JWST/NIRCam F470N band, Vega magnitudes</description><unit>mag</unit><ucd>phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F470N</name><description>[0/0.6]? Uncertainty in F470N</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Survey</name><description>Prior Survey detection (1)</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType" arraysize="26*">char</dataType></column></table><table><name>J/AJ/168/63/table4</name><description>Candidate YSOs from other works matched to our candidate YSOs</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>cYSO</name><description>cYSO position-based name (JHHMMSS.s+DDMMSS)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>Prior</name><description>Previous Works (1)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="39*">char</dataType></column><column><name>Prob</name><description>[0.01/1]? Probability of the object originally selected as the cYSO (within 0.0001{deg} of the position specified in previous works or matched by eye)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Nearby</name><description>[0.64/1]? Nearby Probability (2)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>_RA</name><description>Positions from names (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Positions from names (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">char</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>