The VST/Omegacam Photometric Hα Survey (VPHAS) is imaging the entire Southern Milky Way in visible light at ~1 arcsec angular resolution down to >20th magnitude using the VLT Survey Telescope in Chile.
Survey

VPHAS+ uses VST/OmegaCAM to survey the Southern Galactic Plane and Bulge in u, g, r, i, Hα down to >20th magnitude.

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Science

Our photometry allows a range of rare and short-lived object types to be discovered and characterised.

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Data

VPHAS+ is an ESO Public Survey which provides public data releases.

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Gallery

Our images can be used to construct wide-area mosaics of star-forming regions and extended objects.

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Publications

An overview of VPHAS+ documentation and publications in the literature.

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People

VPHAS+ is an international collaboration, involving institutes mainly from Europe and Chile.

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