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<ri:Resource created="2013-05-23T14:28:24Z" 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>Extreme emission-line galaxies in CANDELS</title><shortName>J/ApJ/742/111</shortName><identifier>ivo://CDS.VizieR/J/ApJ/742/111</identifier><altIdentifier>doi:10.26093/cds/vizier.17420111</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>van der Wel A.</name></creator><creator><name>Straughn A.N.</name></creator><creator><name>Rix H.-W.</name></creator><creator><name>Finkelstein S.L.</name></creator><creator><name>Koekemoer A.M.,Weiner B.J.</name></creator><creator><name>Wuyts S.</name></creator><creator><name>Bell E.F.</name></creator><creator><name>Faber S.M.</name></creator><creator><name>Trump J.R.</name></creator><creator><name>Koo D.C.,Ferguson H.C.</name></creator><creator><name>Scarlata C.</name></creator><creator><name>Hathi N.P.</name></creator><creator><name>Dunlop J.S.</name></creator><creator><name>Newman J.A.,Dickinson M.</name></creator><creator><name>Jahnke K.</name></creator><creator><name>Salmon B.W.</name></creator><creator><name>de Mello D.F.</name></creator><creator><name>Kocevski D.D.</name></creator><creator><name>Lai K.,Grogin N.A.</name></creator><creator><name>Rodney S.A.</name></creator><creator><name>Guo Y.</name></creator><creator><name>McGrath E.J.</name></creator><creator><name>Lee K.-S.</name></creator><creator><name>Barro G.,Huang K.-H.</name></creator><creator><name>Riess A.G.</name></creator><creator><name>Ashby M.L.N.</name></creator><creator><name>Willner S.P.</name></creator><date role="Updated">2018-02-12T08:45:34Z</date><date role="Created">2013-05-23T14:28:24Z</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>hst-photometry</subject><subject>line-intensities</subject><description>We identify an abundant population of extreme emission-line galaxies (EELGs) at redshift z~1.7 in the Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey imaging from Hubble Space Telescope/Wide Field Camera 3 (HST/WFC3). Sixty-nine EELG candidates are selected by the large contribution of exceptionally bright emission lines to their near-infrared broadband magnitudes. Supported by spectroscopic confirmation of strong [OIII] emission lines - with rest-frame equivalent widths ~1000{AA} - in the four candidates that have HST/WFC3 grism observations, we conclude that these objects are galaxies with ~10^8^M_{sun}_ in stellar mass, undergoing an enormous starburst phase with M_*_/(dM/dt)_*_ of only ~15Myr. These bursts may cause outflows that are strong enough to produce cored dark matter profiles in low-mass galaxies. The individual star formation rates and the comoving number density (3.7x10^-4^Mpc^-3^) can produce in ~4Gyr much of the stellar mass density that is presently contained in 10^8^-10^9^M_{sun}_ dwarf galaxies. Therefore, our observations provide a strong indication that many or even most of the stars in present-day dwarf galaxies formed in strong, short-lived bursts, mostly at z&gt;1.</description><source format="bibcode">2011ApJ...742..111V</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/742/111</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/B/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/261">II/261 : GOODS initial results (Giavalisco+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/203/24">J/ApJS/203/24 : Parameters of galaxies in CANDELS (van der Wel+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/14">J/AJ/141/14 : HST WFC3 ERS : emission-line galaxies (Straughn+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/737/71">J/ApJ/737/71 : The [OIII] emission line in SDSS AGNs (Zhang+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/192/5">J/ApJS/192/5 : ELGs from HETDEX pilot survey (Adams+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/64">J/AJ/141/64 : PEARS emission-line galaxies spectroscopy (Xia+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/138/1022">J/AJ/138/1022 : ELGs from HST PEARS survey (Straughn+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/668/853">J/ApJ/668/853 : Spectroscopy of UltraStrong ELGs (Kakazu+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/365/454">J/MNRAS/365/454 : Emission line analysis of HII galaxies (Hoyos+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/2584">J/AJ/130/2584 : KISS emission-line galaxy candidates. 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