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<ri:Resource created="2014-11-21T13:07:17Z" 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>Very low-z SDSS galaxies with H{alpha} emission</title><shortName>J/ApJ/765/26</shortName><identifier>ivo://CDS.VizieR/J/ApJ/765/26</identifier><altIdentifier>doi:10.26093/cds/vizier.17650026</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Shim H.</name></creator><creator><name>Chary R.-R.</name></creator><date role="Updated">2017-10-09T13:33:34Z</date><date role="Created">2014-11-21T13:07:17Z</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>line-intensities</subject><subject>redshifted</subject><subject>ultraviolet-astronomy</subject><description>Strong H{alpha} emitters (HAEs) dominate the z~4 Lyman-break galaxy (LBG) population. We have identified local analogs of these HAEs using the Sloan Digital Sky Survey. At z&lt;0.4, only 0.04% of the galaxies are classified as HAEs with H{alpha} equivalent widths (&gt;~500{AA}) comparable to that of z~4 HAEs. Local HAEs have lower stellar mass and lower ultraviolet (UV) luminosity than z~4 HAEs, yet the H{alpha}-to-UV luminosity ratio, as well as their specific star formation rate, is consistent with that of z~4 HAEs, indicating that they are scaled-down versions of high-z star-forming galaxies. Compared to the previously studied local analogs of LBGs selected using rest-frame UV properties, local HAEs show similar UV luminosity surface density, weaker D_n_(4000) break, lower metallicity, and lower stellar mass. This implies that the local HAEs are less evolved galaxies than the traditional Lyman break analogs. In the stacked spectrum, local HAEs show a significant He II{lambda}4686 emission line suggesting a population of hot, massive stars similar to that seen in some Wolf-Rayet galaxies. Low [N II]/[O III] line flux ratios imply that local HAEs are inconsistent with being systems that host bright active galactic nuclei. Instead, it is highly likely that local HAEs are galaxies with an elevated ionization parameter, either due to a high electron density or large escape fraction of hydrogen ionizing photons as in the case of Wolf-Rayet galaxies.</description><source format="bibcode">2013ApJ...765...26S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/765/26</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/311">II/311 : WISE All-Sky Data Release (Cutri+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/312">II/312 : GALEX-DR5 (GR5) sources from AIS and MIS (Bianchi+ 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/421/1043">J/MNRAS/421/1043 : Emission-line galaxies from SDSS DR7 (Shirazi+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/173/441">J/ApJS/173/441 : UV-Luminous galaxies discovered by GALEX (Hoopes+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/655/851">J/ApJ/655/851 : Wolf-Rayet galaxies in the SDSS (Zhang+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/647/128">J/ApJ/647/128 : H{alpha} observations of UV-selected galaxies (Erb, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/161/240">J/ApJS/161/240 : High-ionization emission in metal-deficient BCD (Thuan+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/132/37">J/ApJS/132/37 : Spectroscopy of Southern warm IR galaxies (Kewley+, 2001)</relatedResource><relatedResource>http://www.mpa-garching.mpg.de/SDSS/DR7 : MPA-JHU 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