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<ri:Resource created="2008-12-20T21:15:16Z" 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>Spectroscopy of Ultraluminous IR galaxies</title><shortName>J/AJ/132/2596</shortName><identifier>ivo://CDS.VizieR/J/AJ/132/2596</identifier><altIdentifier>doi:10.26093/cds/vizier.51322596</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Darling J.</name></creator><creator><name>Giovanelli R.</name></creator><date role="Updated">2017-06-26T11:50:20Z</date><date role="Created">2008-12-20T21:15:16Z</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>astrophysical-masers</subject><subject>radio-astronomy</subject><subject>redshifted</subject><subject>spectroscopy</subject><description>We investigate the types of nuclear environments that produce OH megamasers (OHMs) with a study of the optical spectra of 40 OHM host galaxies and a control sample of 30 non-masing (ultra)luminous infrared galaxies ([U]LIRGs). The optical spectrophotometry provides spatially resolved spectra of multiple nuclei in a few of these merging systems. Of the 40 OHMs classified, 33% are starbursts, 42% are LINERs, and 25% are Seyfert 2 galaxies; the classification of the non-masing control sample is similar.</description><source format="bibcode">2006AJ....132.2596D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/132/2596</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/II/156">II/156 : IRAS Faint Source Catalog, |b| &gt; 10, Version 2.0 (Moshir+ 1989)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/124/100">J/AJ/124/100 : OH megamasers at z&gt;0.1. 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The H{beta} to H{alpha} flux ratio</description><ucd>phot.flux;em.line.Hbeta;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_OIII</name><description>Limit flag on OIII</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>OIII</name><description>The [OIII] (5007) to H{alpha} flux ratio</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>OI</name><description>The [OI] (6300) to H{alpha} flux ratio</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>N6548</name><description>The [NII] (6548) to H{alpha} flux ratio</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>N6583</name><description>The [NII] (6583) to H{alpha} flux ratio</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>S6716</name><description>? 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Optical heliocentric velocity assumed for the Arecibo OHM survey</description><unit>km/s</unit><ucd>spect.dopplerVeloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_czL</name><description>? The 1{sigma} uncertainty in czL</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>czOH</name><description>? Optical heliocentric velocity centroid of the 1667 MHz OH line</description><unit>km/s</unit><ucd>spect.dopplerVeloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_czOH</name><description>? 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