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<ri:Resource created="2025-09-26T09:59:10Z" status="active" updated="2026-08-31T14:43:14Z" 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>HeII emitters. {lambda}1640 emission</title><shortName>J/A+A/702/A3</shortName><identifier>ivo://CDS.VizieR/J/A+A/702/A3</identifier><altIdentifier>doi:10.26093/cds/vizier/bc-ny/ld</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gonzalez-Diaz R.</name></creator><creator><name>Vilchez J.M.</name></creator><creator><name>Kehrig C.</name></creator><creator><name>del Moral-Castro I.,Iglesias-Paramo J.</name></creator><date role="Updated">2026-08-31T14:43:14Z</date><date role="Created">2025-09-26T09:59:10Z</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>visible-astronomy</subject><subject>line-intensities</subject><description>The study of high-redshift galaxies provides critical insights into the early stages of cosmic evolution, particularly during the so-called 'cosmic noon', when star formation activity reached its peak. Within this context, the origin of the nebular emission remains an open question. In this work, we conduct a systematic, multi-wavelength investigation of a sample of z~2-4 emitters from the MUSE Hubble Ultra Deep Field surveys, utilising both MUSE and JWST/NIRSpec data and extending the sample presented by previous studies. We derive gas-phase metallicities and key physical properties, including electron densities, temperatures and the production rates of hydrogen- and He^+^-ionising photons. Our results suggest that a combination of factors-such as stellar mass, initial mass function, stellar metallicity, and stellar multiplicity -- likely contributes to the origin of the observed nebular emission. Specifically, for our galaxies with higher gas-phase metallicity (12+log(O/H)&gt;7.55), we find that models for binary population with Salpeter IMF (Mup=100M_{sun}_) and stellar metallicity ~0.001 (i.e., similar to that of the gas) can reproduce the observed ionising conditions. However at lower metallicities, models for binary population with 'top-heavy' initial mass function (Mup=300M_{sun}_) and Z* much lower (10^-4^&lt;Z*&lt;10^-5^) than that of the gas are required to fully account for the observed ionising photon production. These results reinforce that the ionisation keeps challenging current stellar populations, and the ionisation problem persists in the very low metallicity regime.</description><source format="bibcode">2025A&amp;A...702A...3G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/702/A3</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/A+A/670/A4">J/A+A/670/A4 : MUSE Hubble Ultra Deep Field surveys. 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Line flux error of the galaxy ID: 1024</description><unit>1e-23W.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FWHM1024</name><description>? Line FWHM of the galaxy ID: 1024</description><unit>0.1nm</unit><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>F1273</name><description>? Line flux of the galaxy ID: 1273</description><unit>1e-23W.m**-2</unit><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_F1273</name><description>? Line flux error of the galaxy ID: 1273</description><unit>1e-23W.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FWHM1273</name><description>? Line FWHM of the galaxy ID: 1273</description><unit>0.1nm</unit><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>F22</name><description>? Line flux of the galaxy ID: 22</description><unit>1e-23W.m**-2</unit><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_F22</name><description>? Line flux error of the galaxy ID: 22</description><unit>1e-23W.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FWHM22</name><description>? Line FWHM of the galaxy ID: 22</description><unit>0.1nm</unit><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>F1036</name><description>? Line flux of the galaxy ID: 1036</description><unit>1e-23W.m**-2</unit><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_F1036</name><description>? Line flux error of the galaxy ID: 1036</description><unit>1e-23W.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FWHM1036</name><description>? Line FWHM of the galaxy ID: 1036</description><unit>0.1nm</unit><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>F1056</name><description>? Line flux of the galaxy ID: 1056</description><unit>1e-23W.m**-2</unit><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_F1056</name><description>? Line flux error of the galaxy ID: 1056</description><unit>1e-23W.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FWHM1056</name><description>? Line FWHM of the galaxy ID: 1056</description><unit>0.1nm</unit><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>F1051</name><description>? Line flux of the galaxy ID:1051</description><unit>1e-23W.m**-2</unit><ucd>phot.flux;spect.line</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_F1051</name><description>? Line flux error of the galaxy ID:1051</description><unit>1e-23W.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FWHM1051</name><description>? Line FWHM of the galaxy ID:1051</description><unit>0.1nm</unit><ucd>spect.line.width;spect.line</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>F106</name><description>? Line flux of the galaxy ID 106</description><unit>1e-23W.m**-2</unit><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_F106</name><description>? Line flux error of the galaxy ID 106</description><unit>1e-23W.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FWHM106</name><description>? Line FWHM of the galaxy ID 106</description><unit>0.1nm</unit><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>F51</name><description>? Line flux of the galaxy ID: 51</description><unit>1e-23W.m**-2</unit><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_F51</name><description>? Line flux error of the galaxy ID: 51</description><unit>1e-23W.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FWHM51</name><description>? Line flux error of the galaxy ID: 51</description><unit>0.1nm</unit><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>