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The HIPASS H-alpha survey is a project to measure
ionized hydrogen in a sample of 500 galaxies selected
via their 21-cm neutral hydrogen emission.
Our aim is to understand better the global physics
of star formation in galaxies, and to quantify better the
total rate of star formation in the nearby universe.
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Survey Overview
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A brief description of the scientific objectives of the survey.
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The Proposal
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March 2000 NOAO Survey proposal to observe 500 HI-selected
galaxies in H-alpha.
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News and Status
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Survey progress, data releases, etc.
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"First light" image from survey. IC5332.
Red=H alpha, Blue = R band continuum,
Green = H alpha before continuum subtraction
More pretty pictures coming soon.
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Internal Site
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SINGG internal web site.
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