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<ri:Resource created="2026-06-03T13:36:27Z" status="active" updated="2026-06-15T00:00:00Z" 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>MIPAPS. II. Pa{alpha} emission-line sources</title><shortName>J/ApJS/279/55</shortName><identifier>ivo://CDS.VizieR/J/ApJS/279/55</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kim I.-J.</name></creator><creator><name>Pyo J.</name></creator><creator><name>Seon K.-I.</name></creator><creator><name>Jeong W.-S.</name></creator><creator><name>Nakagawa T.</name></creator><creator><name>Matsumoto T.</name></creator><date role="Updated">2026-06-03T13:00:27Z</date><date role="Created">2026-06-03T13:36:27Z</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>galaxy-planes</subject><subject>milky-way-galaxy</subject><subject>h-ii-regions</subject><subject>infrared-photometry</subject><subject>interstellar-medium</subject><subject>surveys</subject><description>Using data from the MIRIS Pa{alpha} Galactic Plane Survey (MIPAPS), we present a Pa{alpha} 1.87{mu}m line image of the entire Galactic plane within the latitude range of -3{deg}&lt;~b&lt;~+3{deg}, revealing numerous Pa{alpha} features. Based on the MIPAPS Pa{alpha} image and the Wide-field Infrared Survey Explorer (WISE) HII region catalog, we compile a catalog of 1489 Pa{alpha} emission-line sources in the Galactic plane within 90{deg}&lt;~l&lt;~330{deg}. By comparing our Pa{alpha} images with H{alpha} images constructed from the IPHAS and VPHAS+ survey data, we demonstrate the advantages of Pa{alpha} line observations. We identify 902 Pa{alpha} sources associated with HII regions, and newly confirm 619 HII region candidates as definitive HII regions through Pa{alpha} or H{alpha} detections. We also identify 261 extended and 326 pointlike Pa{alpha} sources not included in the WISE catalog, most of which have H{alpha} counterparts in the IPHAS or VPHAS+ images. A search of the SIMBAD database indicates that these sources originate from diverse object types. By measuring Pa{alpha} and H{alpha} fluxes, we estimate the E(B-V) color excesses derived from extended emissions for 138 Pa{alpha} sources, showing good agreement with values obtained from spectrophotometry of ionizing stars in previous studies. Furthermore, we calculate total Lyman continuum luminosities for 42 Pa{alpha} sources, providing constraints on the distances to HII regions and the spectral types of their ionizing stars. These results highlight the scientific potential of Pa{alpha} line observations and the benefits of combining multiple hydrogen recombination lines in exploring ionized regions.</description><source format="bibcode">2025ApJS..279...55K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/279/55</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/VII/233">VII/233 : 2MASS All-Sky Extended Source Catalog (XSC) (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/321">II/321 : IPHAS DR2 Source Catalogue (Barentsen+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/386">II/386 : VPHAS+ DR3 survey (Drew+, 2025)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/397/133">J/A+A/397/133 : Star-forming complexes in the Galaxy (Russeil+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/470/161">J/A+A/470/161 : UBV phot. of HII regions exciting stars (Russeil+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/480/409">J/A+A/480/409 : IPHAS symbiotic stars candidates (Corradi+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/384/1277">J/MNRAS/384/1277 : H{alpha} emission line sources from IPHAS (Witham+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/504/291">J/A+A/504/291 : Candidate Planetary Nebulae in IPHAS cat. 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The 1{sigma} uncertainty on E (B-V)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>_Glon</name><description>Positions from MIPAPS names (longitude part)</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>_Glat</name><description>Positions from MIPAPS names (latitude part)</description><unit>deg</unit><ucd>pos.galactic.lat</ucd></column></table><table><name>J/ApJS/279/55/table4</name><description>WISE HII region sources with No MIPAPS Pa{alpha} detection</description><column><name>_RA.icrs</name><description>Right ascension (ICRS) (computed by VizieR, not part of the original data. 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