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HIPASS

HIPASS
Survey type astronomical survey Edit this on Wikidata
Observations Parkes Observatory Edit this on Wikidata
Wavelength 21 centimetre Edit this on Wikidata
Website www.atnf.csiro.au/research/multibeam/
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The HI Parkes All Sky Survey (HIPASS) is a large survey for neutral atomic hydrogen (HI). Most of the data was taken between 1997 and 2002 using CSIRO's 64-m Parkes Telescope. HIPASS covered 71% of the sky and identified more than 5000 galaxies; the major galaxy catalogs are: the "HIPASS Bright Galaxy Catalog" (HIPASS BGC), the southern HIPASS catalog (HICAT), and the northern HIPASS catalog (NHICAT) Discoveries include over 5000 galaxies (incl. several new galaxies), the Leading Arm of the Magellanic Stream and a few gas clouds devoid of stars.

HIPASS covers a velocity range of -1,280 to 12,700 km/s. It was the first blind HI survey to cover the entire southern sky and the northern sky up to +25 degr. Technical overview, calibration and imaging (Barnes et al. 2001).

Observations of the southern sky started in February 1997, and were completed in March 2000, consisting of 23020 eight-degree scans of each of 9 minutes duration. HIPASS scanned the entire southern sky five times. The southern HIPASS galaxy catalog (HICAT) contains 4315 HI sources.

Northern HIPASS extended the survey into the northern sky. The entire Virgo Cluster region was observed in Northern HIPASS. NHICAT, the catalogue of the northern extension of HIPASS contains 1002 HI sources.

Observations for HIPASS were taken using the Parkes 21-cmcm Multibeam Receiver. The instrument consists of a focal-plane array of 13 individual receivers arranged in a hexagonal pattern. Built in a collaboration between numerous institutions, it was funded by the Australian Research Council (ARC) and the Australia Telescope National Facility (ATNF) to undertake the HIPASS and ZOA surveys.

HIPASS discovered the Leading Arm of the Magellanic Stream. This is an extension of the Magellanic Stream beyond the Magellanic clouds. The existence of the Leading Arm is predicted by models of a tidal interaction between the Magellanic Clouds and the Milky Way.


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