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<ri:Resource created="2014-01-29T09:44:25Z" 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>Ly{alpha} profiles of LAEs at z=3.1</title><shortName>J/ApJ/751/29</shortName><identifier>ivo://CDS.VizieR/J/ApJ/751/29</identifier><altIdentifier>doi:10.26093/cds/vizier.17510029</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Yamada T.</name></creator><creator><name>Matsuda Y.</name></creator><creator><name>Kousai K.</name></creator><creator><name>Hayashino T.</name></creator><creator><name>Morimoto N.</name></creator><creator><name>Umemura M.</name></creator><date role="Updated">2017-12-07T07:27:32Z</date><date role="Created">2014-01-29T09:44:25Z</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>visible-astronomy</subject><subject>redshifted</subject><subject>spectroscopy</subject><subject>apparent-magnitude</subject><description>We present the results of the observations of the Ly{alpha} line profiles of 91 emission-line galaxies at z=3.1 with a spectral resolution of {lambda}/{delta}{lambda}(FWHM){approx}1700 or 180km/s. A significant fraction of ~50% of the observed objects show the characteristic double peaks in their Ly{alpha} profile. The red peak is much stronger than the blue one for most of the cases. The red peaks themselves also show weak but significant asymmetry and their widths are correlated with the velocity separation of the red and the blue peaks. This implies that the peaks are not isolated multiple components with different velocities but parts of a single line that are modified by the absorption and/or scattering by the associated neutral hydrogen gas. The characteristic profile can be naturally explained by scattering in the expanding shell of the neutral hydrogen surrounding the Ly{alpha} emitting region while the attenuation by the intergalactic medium should also be considered. Our results suggest that the star formation in these Ly{alpha} emitters are dominated by young burst-like events that produce the intrinsic Ly{alpha} emission as well as the gas outflow.</description><source format="bibcode">2012ApJ...751...29Y</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/751/29</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/ApJ/744/110">J/ApJ/744/110 : LAE galaxies between 2.1=&lt;z&lt;=3.1 (Ciardullo+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/743/9">J/ApJ/743/9 : z=3.1 LAEs morphological properties (Gronwall+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/736/31">J/ApJ/736/31 : HETDEX pilot survey. II. 1.9&lt;z&lt;3.8 LAEs (Blanc+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/705/639">J/ApJ/705/639 : Sizes of Lyman alpha emitters at z=3.1 (Bond+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/498/13">J/A+A/498/13 : Lyman-{alpha} emitters from redshifts z~2-3 (Nilsson+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/176/301">J/ApJS/176/301 : Subaru/XMM-Newton deep survey IV. (SXDS) (Ouchi+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/58/313">J/PASJ/58/313 : Ly{alpha} emitters in the SUBARU Deep Field (Shimasaku+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/57/165">J/PASJ/57/165 : Ly{alpha} emitters in the SUBARU Deep Field (Taniguchi+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/57/881">J/PASJ/57/881 : Imaging of high-redshift Lyman alpha emitters (Yamada+, 2005)</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/ApJ/751/29</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/751/29</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/751/29</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/751/29</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/751/29</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/751/29</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/ApJ/751/29/table1 (Summary of the observed Lyman{alpha} emitters)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/751/29/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/751/29/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/751/29/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>334.209167</ra><dec>0.463889</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/19033 19036</spatial><spectral>3.9603780926802294e-19 4.0221274315046737e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/751/29?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/751/29/table1</name><description>Summary of the observed Lyman{alpha} emitters</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>LAE</name><description>Galaxy identification (JHHMMSS.s+DDMMSS); &lt;[YMK2012] LAE JHHMMSS.s+DDMMSS&gt; in Simbad</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>ze</name><description>[3/3.2] Redshift measured by the peak of the strongest emission-line component</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FWHM</name><description>[19/1998]? FWHM of the strongest component after correction for the instrumental profile (1)</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lam1</name><description>[4928/5006] The central wavelength of the red peak in the multiple-component Gaussian fitting</description><unit>0.1nm</unit><ucd>em.wl.central;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>lam2</name><description>[4923/4992]? 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