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Article: VST Photometric H-alpha Survey of the Southern Galactic Plane and Bulge (VPHAS+)

TitleVST Photometric H-alpha Survey of the Southern Galactic Plane and Bulge (VPHAS+)
Authors
Drew, JEBarentsen, GFabregat, JFarnhill, HMohr-Smith, MWright, NJGonzalez-Solares, EIrwin, MJLewis, JYoldas, AKGreimel, REislöffel, JGroot, PBarlow, MJCorradi, RGänsicke, BTKnigge, CMampaso, AMorris, RNaylor, TParker, QARaddi, RSale, SESteeghs, DUnruh, YCVink, JSWalsh, JRWalton, NAWesson, RZijlstra, A
Issue Date2013
Citation
The Messenger, 2013, v. 154, p. 41-43 How to Cite?
AbstractThe VST Photometric H-alpha survey of the Southern Galactic Plane and Bulge (VPHAS+) is collecting single-epoch Sloan u, g, r, i and H-alpha narrowband photometry, at arcsecond resolution, down to point-source (Vega) magnitudes of ~ 21. The survey footprint encloses the entire southern Galactic Plane within the Galactic latitude range -5° < b < +5°, expanding to b = ±10° in the Galactic Bulge. This brief description of VPHAS+ includes sample data and examples of early science validation.
Persistent Identifierhttp://hdl.handle.net/10722/211195
ISSN
0722-6691

 

DC FieldValueLanguage
dc.contributor.authorDrew, JE-
dc.contributor.authorBarentsen, G-
dc.contributor.authorFabregat, J-
dc.contributor.authorFarnhill, H-
dc.contributor.authorMohr-Smith, M-
dc.contributor.authorWright, NJ-
dc.contributor.authorGonzalez-Solares, E-
dc.contributor.authorIrwin, MJ-
dc.contributor.authorLewis, J-
dc.contributor.authorYoldas, AK-
dc.contributor.authorGreimel, R-
dc.contributor.authorEislöffel, J-
dc.contributor.authorGroot, P-
dc.contributor.authorBarlow, MJ-
dc.contributor.authorCorradi, R-
dc.contributor.authorGänsicke, BT-
dc.contributor.authorKnigge, C-
dc.contributor.authorMampaso, A-
dc.contributor.authorMorris, R-
dc.contributor.authorNaylor, T-
dc.contributor.authorParker, QA-
dc.contributor.authorRaddi, R-
dc.contributor.authorSale, SE-
dc.contributor.authorSteeghs, D-
dc.contributor.authorUnruh, YC-
dc.contributor.authorVink, JS-
dc.contributor.authorWalsh, JR-
dc.contributor.authorWalton, NA-
dc.contributor.authorWesson, R-
dc.contributor.authorZijlstra, A-
dc.date.accessioned2015-07-08T03:22:53Z-
dc.date.available2015-07-08T03:22:53Z-
dc.date.issued2013-
dc.identifier.citationThe Messenger, 2013, v. 154, p. 41-43-
dc.identifier.issn0722-6691-
dc.identifier.urihttp://hdl.handle.net/10722/211195-
dc.description.abstractThe VST Photometric H-alpha survey of the Southern Galactic Plane and Bulge (VPHAS+) is collecting single-epoch Sloan u, g, r, i and H-alpha narrowband photometry, at arcsecond resolution, down to point-source (Vega) magnitudes of ~ 21. The survey footprint encloses the entire southern Galactic Plane within the Galactic latitude range -5° < b < +5°, expanding to b = ±10° in the Galactic Bulge. This brief description of VPHAS+ includes sample data and examples of early science validation.-
dc.languageeng-
dc.relation.ispartofThe Messenger-
dc.titleVST Photometric H-alpha Survey of the Southern Galactic Plane and Bulge (VPHAS+)-
dc.typeArticle-
dc.identifier.emailParker, QA: quentinp@hku.hk-
dc.identifier.authorityParker, QA=rp02017-
dc.identifier.volume154-
dc.identifier.spage41-
dc.identifier.epage43-
dc.identifier.issnl0722-6691-

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