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<ri:Resource created="2016-10-06T14:09:59Z" 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>IDEOS redshift catalogue</title><shortName>J/MNRAS/455/1796</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/455/1796</identifier><altIdentifier>doi:10.26093/cds/vizier.74551796</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hernan-Caballero A.</name></creator><creator><name>Spoon H.W.W.</name></creator><creator><name>Lebouteiller V.</name></creator><creator><name>Rupke D.S.N.,Barry D.P.</name></creator><date role="Updated">2024-08-15T20:16:40Z</date><date role="Created">2016-10-06T14:09:59Z</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>galaxies</subject><subject>infrared-sources</subject><subject>redshifted</subject><description>This is the first of a series of papers on the Infrared Database of Extragalactic Observables from Spitzer (IDEOS). In this work, we describe the identification of optical counterparts of the infrared sources detected in Spitzer Infrared Spectrograph (IRS) observations and the acquisition and validation of redshifts. The IDEOS sample includes all the spectra from the Cornell Atlas of Spitzer/IRS Sources (CASSIS, Lebouteiller et al., 2011ApJS..196....8L, 2015ApJS..218...21L) of galaxies beyond the Local Group. Optical counterparts were identified from correlation of the extraction coordinates with the NASA Extragalactic Database (NED). To confirm the optical association and validate NED redshifts, we measure redshifts with unprecedented accuracy on the IRS spectra ({sigma}({Delta}z/(1+z))~0.0011) by using an improved version of the maximum combined pseudo-likelihood method (MCPL). We perform a multistage verification of redshifts that considers alternate NED redshifts, the MCPL redshift, and visual inspection of the IRS spectrum. The statistics is as follows: the IDEOS sample contains 3361 galaxies at redshift 0&lt;z&lt;6.42 (mean: 0.48, median: 0.14). We confirm the default NED redshift for 2429 sources and identify 124 with incorrect NED redshifts. We obtain IRS-based redshifts for 568 IDEOS sources without optical spectroscopic redshifts, including 228 with no previous redshift measurements. We provide the entire IDEOS redshift catalogue in machine-readable formats. The catalogue condenses our compilation and verification effort, and includes our final evaluation on the most likely redshift for each source, its origin, and reliability estimates.</description><source format="bibcode">2016MNRAS.455.1796H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/455/1796</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>http://cassis.sirtf.com/atlas : CASSIS Home Page</relatedResource><relatedResource>http://ideos.astro.cornell.edu/redshifts.html : IDEOS redshift 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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>AOR_ID</name><description>AOR + Cluster ID</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>RASdeg</name><description>Requested right ascension of Spitzer/IRS observation (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DESdeg</name><description>Requested declination of Spitzer/IRS observation (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>RAJ2000</name><description>Right ascension of CASSIS extracted source (J2000) (1)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination of CASSIS extracted source (J2000) (1)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>NEDname</name><description>NED name of source in zfinal table</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="30*">char</dataType></column><column><name>zfinal</name><description>Final, best redshift for the source</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>r_zfinal</name><description>Origin of best redshift (2)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>q_zfinal</name><description>Verification status for the redshift (3)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>zNED</name><description>Default NED redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>zNEDtype</name><description>Type of default NED redshift (4)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>zMCPL</name><description>Redshift from IRS spectrum (maximum combined pseudo-likelihood method (MCPL) algorithm)</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>gamma</name><description>gamma parameter for zMCPL redshift (5)</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>R</name><description>R parameter for zMCPL redshift (5)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>A</name><description>? Reliability of zMCPL redshift (A=gamma+log10(R)/2)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_A</name><description>[i] i for -infinity</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>P005</name><description>Outlier probability for zMCPL at delta=0.005 threshold, P_0.005_(A) (6)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>P05</name><description>Outlier probability for zMCPL at delta=0.05 threshold, P_0.05_(A) (7)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>zNEDalt</name><description>? 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