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<ri:Resource created="2009-10-28T21:19:56Z" 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>Diffuse ionized gas database DIGEDA</title><shortName>J/other/RMxAA/45</shortName><identifier>ivo://CDS.VizieR/J/other/RMxAA/45.261</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Flores-Fajardo N.</name></creator><creator><name>Morisset C.</name></creator><creator><name>Binette L.</name></creator><date role="Updated">2017-10-18T08:23:56Z</date><date role="Created">2009-10-28T21:19:56Z</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>h-ii-regions</subject><subject>interstellar-medium</subject><description>Studies of the Diffuse Ionized Gas (DIG) have progressed without providing so far any strict criterion to distinguish DIGs from HII regions. In this work, we compile the emission line measurements of 29 galaxies that are available in the scientific literature, thereby setting up the first DIG database DIGEDA. Making use of this database, we proceeded to analyze global properties of the DIG using the [NII]6583/Halpha, [OI]6300/Halpha, [OIII]5007/Hbeta and [SII]6716/Halpha lines ratios, including the Halpha emission measure. This analysis leads us to conclude that the [NII]/Halpha ratio provides an objective criterion for distinguishing whether an emission region is DIG or an HII region, while the EM(Halpha) is a useful quantity only when the galaxies are considered individually. Finally, we find that the emission regions of Irr galaxies classified as DIG in the literature appear in fact to be much more similar to HII regions than to the DIGs of spiral galaxies.</description><source format="bibcode">2009RMxAA..45..261F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/RMxAA/45.261</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/ApJS/165/307">J/ApJS/165/307 : Ionization in neutral gas galaxies survey. I. (Meurer+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/661/801">J/ApJ/661/801 : Ionization in neutral gas galaxies survey. III. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>GalID</name><description>Integer number that relates uniquely the galaxy's name to its source catalog (1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>primary</flag></column><column><name>Galaxy</name><description>The NED catalog name of each galaxy in DIGEDA</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000.0)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000.0)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>MType</name><description>Galaxy morphology in NED catalog</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>i</name><description>? The inclination angle for each galaxy</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>NED</name><description>Simbad column added by the CDS</description><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/other/RMxAA/45.261/digeda</name><description>DIG and HII regions spectroscopic observations database</description><column><name>I4363</name><description>? OIII 4363 line intensity (2)</description><ucd>spect.line.intensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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OIII 4959 line intensity (2)</description><ucd>spect.line.intensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>I5007</name><description>? OIII 5007 line intensity (2)</description><ucd>spect.line.intensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>I5876</name><description>? HeI 5876 line intensity (2)</description><ucd>spect.line.intensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>I6300</name><description>? OI 6300 line intensity (2)</description><ucd>spect.line.intensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>I6548</name><description>? NII 6548 line intensity (2)</description><ucd>spect.line.intensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>IHa</name><description>? Halpha 6563 line intensity (2)</description><ucd>spect.line.intensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>I6583</name><description>? NII 6583 line intensity (2)</description><ucd>spect.line.intensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>I6716</name><description>? SII 6716 line intensity (2)</description><ucd>spect.line.intensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>I6731</name><description>? SII 6731 line intensity (2)</description><ucd>spect.line.intensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>I16+31</name><description>? SII 6716+6731 line intensity (2)</description><ucd>spect.line.intensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Te</name><description>? 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