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<ri:Resource created="2016-03-30T15:46:53Z" 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>Follow-up spectroscopy of Ly{alpha} 3&lt;z&lt;7 emitters</title><shortName>J/ApJ/815/57</shortName><identifier>ivo://CDS.VizieR/J/ApJ/815/57</identifier><altIdentifier>doi:10.26093/cds/vizier.18150057</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>U V.</name></creator><creator><name>Hemmati S.</name></creator><creator><name>Darvish B.</name></creator><creator><name>Mobasher B.</name></creator><creator><name>Nayyeri H.</name></creator><creator><name>Dickinson M.,Stern D.</name></creator><creator><name>Spinrad H.</name></creator><creator><name>Mallery R.</name></creator><date role="Updated">2017-09-05T14:48:13Z</date><date role="Created">2016-03-30T15:46:53Z</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>spectroscopy</subject><subject>redshifted</subject><subject>galaxy-classification-systems</subject><subject>interstellar-medium</subject><description>We explore the relationship between the spectral shape of the Ly{alpha} emission and the UV morphology of the host galaxy using a sample of 304 Ly{alpha}-emitting BVi-dropouts at 3&lt;z&lt;7 in the Great Observatories Origins Deep Survey and Cosmic Evolution Survey fields. Using our extensive reservoir of high-quality Keck DEIMOS spectra combined with Hubble Space Telescope WFC3 data, we measure the Ly{alpha} line asymmetries for individual galaxies and compare them to axial ratios measured from observed J- and H-band (restframe UV) images. We find that the Ly{alpha} skewness exhibits a large scatter at small elongation (a/b&lt;2), and this scatter decreases as the axial ratio increases. Comparison of this trend to radiative transfer models and various results from the literature suggests that these high-redshift Ly{alpha} emitters are not likely to be intrinsically round and symmetric disks, but they probably host galactic outflows traced by Ly{alpha} emitting clouds. The ionizing sources are centrally located, and the optical depth is a good indicator of the absorption and scattering events on the escape path of Ly{alpha} photons from the source. Our results find no evidence of evolution in Ly{alpha} asymmetry or axial ratio with look-back time.</description><source format="bibcode">2015ApJ...815...57U</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/815/57</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/284">II/284 : COSMOS Multi-Wavelength Photometry Catalog (Capak+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/318">II/318 : GOODS Source Catalogs release r2.0z (Giavalisco+ 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/261">II/261 : GOODS 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