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<ri:Resource created="2026-02-05T09:01:47Z" status="active" updated="2026-03-02T06:25:50Z" 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>Third quadrant bright VPHAS+ photometry</title><shortName>J/MNRAS/545/F213</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/545/F2137</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Drew J.E.</name></creator><creator><name>Greimel R.</name></creator><creator><name>Eisloeffel J.</name></creator><creator><name>Raddi R.</name></creator><creator><name>Wright N.J.</name></creator><date role="Updated">2026-03-02T06:25:50Z</date><date role="Created">2026-02-05T09:01:47Z</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>surveys</subject><subject>galaxy-planes</subject><subject>milky-way-galaxy</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>h-alpha-photometry</subject><description>The southern Galactic plane has been mapped at optical wavelengths and at under 1-arcsec angular resolution by the VST Photometric Halpha Survey of the Galactic plane and bulge (VPHAS+). Ahead of the release of a uniform photometric calibration of the entire survey footprint, we examine the properties of r&lt;19 VPHAS+ point-source photometry in the third Galactic quadrant. Our interim calibration in g, r and i is compared with that of Pan-STARRS, DECaPS-2 and Skymapper, revealing the need for small gri photometric offsets. Corrections to the Halpha and u magnitude scales are determined via comparison with synthetic photometry. VPHAS+ and its northern counterpart, IGAPS, are shown to closely align across the celestial equator. Aided by Gaia DR3, SIMBAD, and specialist catalogues, we explore selections of: A stars; sub-luminous stars; intrinsically-red luminous stars; young stellar objects; emission-line and OB stars. Attention is drawn to stellar variability as a contaminant in selecting emission line objects via (r - Halpha) excess. The (r-i, r-Halpha) plane appears better for this selection than the alternative (g-i, r-Halpha) plane. Using A stars to map extinction, we show that dust obscuration is greater at negative Galactic latitudes. Like the dust, OB and emission line stars are more frequent below the Galactic equator: at heliocentric distances of up to ~7kpc, these stars' distribution fit in with the known warping of the Galactic plane. An overdensity of B stars, several degrees across and potentially in the Outer Arm, is found around (l,b) = (212.0, -0.6).</description><source format="bibcode">2026MNRAS.545f2137D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/545/F2137</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/386">II/386 : VPHAS+ DR3 survey (Drew+, 2025)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/545/F2137</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/545/F2137</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/545/F2137</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/545/F2137</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/545/F2137</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/545/F2137</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/MNRAS/545/F2137/vphasq3b (Photometric catalogue)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/545/F2137/vphasq3b?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/545/F2137/vphasq3b?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/545/F2137/vphasq3b?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>99.72317</ra><dec>1.73218</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>3/336 338 615 621 4/1301 1303 1358 1377 1379-1380 1382 1385 2455 2493 2495 2528 2530 2536 2538 5/5237 5239 5402 5424 5426 5504-5505 5507 5513 5526 5532 5534 5552-5554 9807 9818-9819 9829 9831 9837 9839 9968-9969 9971 9977 9979 9992 9994 10016 10018 10024 10026 10156 10158 6/20804-20805 20807 20813 20815 20837 20945 20947 20980-20981 20983 20989 21578 21600 21602 21700 21708 21710 21746 21752 21754 22024-22025 22027 22060-22061 22063 22096 22098-22099 22110 22132 22134 22140 22149 22151 22193 22196-22197 22220 22224 22240 39263 39267 39270-39271 39315 39321 39347 39701-39703 39708-39709 39711 39733 39735 39741 39743 39880-39881 39883 39905 39907 39946-39947 39950 39972 39974 39980 39982 40068 40070 40076 40078 40100 40102 40108 40110-40111 40504 40506 40592 40594 40600 40602-40603 40628 40630 40636 40638-40639</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/545/F2137?format=ascii</footprint><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/545/F2137/vphasq3b</name><description>Photometric catalogue</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000.0) (RA)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>MainType</name><description>SIMBAD main object class (main_type)</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>SpType</name><description>SIMBAD spectral type (sp_type)</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>VPHAS+</name><description>Display the VPHAS+ data (Drew et al. 2035, Cat. 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