Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aj....124..690k&link_type=abstract
The Astronomical Journal, Volume 124, Issue 2, pp. 690-705.
Astronomy and Astrophysics
Astronomy
26
Catalogs, Galaxies: General, Surveys
Scientific paper
The first deep catalog of the H I Parkes All Sky Survey (HIPASS) is presented, covering the south celestial cap (SCC) region. The SCC area is ~2400 deg2 and covers δ<-62°. The average rms noise for the survey is 13 mJy beam-1. Five hundred thirty-six galaxies have been cataloged according to their neutral hydrogen content, including 114 galaxies that have no previous cataloged optical counterpart. This is the largest sample of galaxies from a blind H I survey to date. Most galaxies in optically unobscured regions of sky have a visible optical counterpart; however, there is a small population of low-velocity H I clouds without visible optical counterparts whose origins and significance are unclear. The rms accuracy of the HIPASS positions is found to be 1.9′. The H I mass range of galaxies detected is from ~106 to ~1011 Msolar. There are a large number of late-type spiral galaxies in the SCC sample (66%), compared with 30% for optically selected galaxies from the same region in the NASA Extragalactic Database. The average ratio of H I mass to B luminosity of the sample increases according to optical type, from 1.8 Msolar/Lsolar for early types to 3.2 Msolar/Lsolar for late-type galaxies. The H I-detected galaxies tend to follow the large-scale structure traced by galaxies found in optical surveys. From the number of galaxies detected in this region of sky, we predict the full HIPASS catalog will contain ~5000 galaxies, to a peak flux density limit of ~39 mJy (3 σ), although this may be a conservative estimate as two large voids are present in the region. The H I mass function for this catalog is presented in a subsequent paper.
Banks G. D.
Barnes David G.
Bhathal Ragbir
Boyce Peter J.
de Blok J. G. W.
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