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We present the HIPASS Bright Galaxy Catalog (BGC), which contains the 1000 H I brightest galaxies in the southern sky as obtained from the H I Parkes All-Sky Survey (HIPASS). The selection of the brightest sources is based on their H I peak flux density (S peak ≳ 116 mJy) as measured from the spatially integrated HIPASS spectrum. The derived H I masses range from ∼10 7 to 4 × 10 10 M⊙. While the BGC (z 10°. Therefore, the BGC yields no evidence for a population of "free-floating" intergalactic H I clouds without associated optical counterparts. HIPASS provides a clear view of the local large-scale structure. The dominant features in the sky distribution of the BGC are the Supergalactic Plane and the Local Void. In addition, one can clearly see the Centaurus Wall, which connects via the Hydra and Antlia Clusters to the Puppis Filament. Some previously hardly noticable galaxy groups stand out quite distinctly in the H I sky distribution. Several new structures, including some not behind the Milky Way, are seen for the first time.
Koribalski et al. (Thu,) studied this question.