<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2021-10-28T09:11:41Z" 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>COSMOS2015 dataset machine learning photo-z</title><shortName>J/MNRAS/507/5034</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/507/5034</identifier><altIdentifier>doi:10.26093/cds/vizier.75075034</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Razim O.</name></creator><creator><name>Cavuoti S.</name></creator><creator><name>Brescia M.</name></creator><creator><name>Riccio G.</name></creator><creator><name>Salvato M.</name></creator><creator><name>Longo G.</name></creator><date role="Updated">2024-08-21T20:18:36Z</date><date role="Created">2021-10-28T09:11:41Z</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>astronomical-models</subject><subject>redshifted</subject><subject>galaxies</subject><subject>catalogs</subject><description>In order to answer the open questions of modern cosmology and galaxy evolution theory, robust algorithms for calculating photometric redshifts (photo-z) for very large samples of galaxies are needed. Correct estimation of the various photo-z algorithms' performance requires attention to both the performance metrics and the data used for the estimation. In this work, we use the supervised machine learning algorithm MLPQNA (Multi-Layer Perceptron with Quasi-Newton Algorithm) to calculate photometric redshifts for the galaxies in the COSMOS2015 catalogue and the unsupervised Self-Organizing Maps (SOM) to determine the reliability of the resulting estimates. We find that for z_spec_&lt;1.2, MLPQNA photo-z predictions are on the same level of quality as spectral energy distribution fitting photo-z. We show that the SOM successfully detects unreliable zspec that cause biases in the estimation of the photo-z algorithms' performance. Additionally, we use SOM to select the objects with reliable photo-z predictions. Our cleaning procedures allow us to extract the subset of objects for which the quality of the final photo-z catalogues is improved by a factor of 2, compared to the overall statistics.</description><source format="bibcode">2021MNRAS.507.5034R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/507/5034</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/224/24">J/ApJS/224/24 : The COSMOS2015 catalog (Laigle+, 2016)</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/MNRAS/507/5034</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/507/5034</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/507/5034</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/507/5034</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/507/5034</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/507/5034</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/MNRAS/507/5034/mlphotoz (COSMOS2015 machine learning photometric redshifts with reliability indicators derived with SOM)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/507/5034/mlphotoz?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/507/5034/mlphotoz?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/507/5034/mlphotoz?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>149.93295632</ra><dec>1.61800327</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/6814 6/27245 27247 27344</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/507/5034?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/507/5034/mlphotoz</name><description>COSMOS2015 machine learning photometric redshifts with reliability indicators derived with SOM</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>RAJ2000</name><description>[149.41/150.79] Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>[1.61/2.82] Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>Seq</name><description>Object ID in the original COSMOS2015 catalog, Laigle et al., 2016, Cat. J/ApJS/224/24)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>dataset</name><description>[Run Test Train] A flag indicating whether the object was included in the train, test or run samples during MLPQNA training</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>zphMl</name><description>[0.02/1.47] Photometric redshift obtained with MLPQNA (photoZ_ML)</description><ucd>src.redshift.phot;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>zphMlCoeff</name><description>? In-cell outlier coefficient for ML photo-z (photoZ_ML_outlCoeff) (1)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>zphSED</name><description>[0.0/4.72] SED fitting photometric redshift derived from the COSMOS2015 (photoZ_SED)</description><ucd>src.redshift.phot;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>zphSEDCoeff</name><description>? In-cell outlier coefficient for SED fitting photo-z (photoZ_SED_outlCoeff) (1)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>resML-SED</name><description>[-1.11/0.75] Residuals between ML and SED fitting photo-z calculated as resid=(z_SED-z_ML)/(1+z_SED) (residML_SED)</description><ucd>stat.fit.residual;stat.fit;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>zspCoeff</name><description>? In-cell outlier coefficient for spec-z (specZ_outlCoeff) (1)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>tMO</name><description>Occupation of the SOM cell, to which this object belongs, by the train dataset (trainMapOccupation)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>