HIPASS

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HIPASS
Website www.atnf.csiro.au/research/multibeam/
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The H I Parkes All Sky Survey (HIPASS) is a large survey for neutral atomic hydrogen (H I). [1] 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), [2] the southern HIPASS catalog (HICAT), [3] and the northern HIPASS catalog (NHICAT) [4] Discoveries include over 5000 galaxies (incl. several new galaxies), the Leading Arm of the Magellanic Stream and a few gas clouds devoid of stars.

Contents

Survey

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°. Technical overview, calibration and imaging (Barnes et al. 2001).

Southern Sky observations

Observations of the southern sky started in February 1997, and were completed in March 2000, consisting of 23,020 eight-degree scans of each of 9 minutes duration. HIPASS scanned the entire southern sky five times. The southern HIPASS galaxy catalog (HICAT) [3] contains 4315 HI sources.

Northern Sky observations

Northern HIPASS extended the survey into the northern sky. The entire Virgo Cluster region was observed in Northern HIPASS. NHICAT, [4] the catalogue of the northern extension of HIPASS contains 1,002 H I sources.

CHIPASS

Archival data from HIPASS and the HI Zone of Avoidance (HIZOA) survey were reprocessed to make a new 20cm confusion-limited continuum map of the sky south of declination +25°. Its relatively high sensitivity and resolution (compared to other single-dish surveys) and low level of artefacts has made this survey invaluable, particularly for merging with interferometric data such as WALLABY to improve the coverage of extended structure. [5]

Multibeam Receiver

Observations for HIPASS were taken using the Parkes 21-cm Multibeam Receiver. [6] The instrument consists of a focal-plane array of 13 individual receivers arranged in a hexagonal pattern. [6] 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.

Discoveries

Leading arm of Magellanic Stream

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.

HIPASS J0731-69

HIPASS J0731-69 is a cloud of gas devoid of any stars. [7] It is associated with the asymmetric spiral galaxy NGC 2442. [7] It is likely that HIPASS J0731-69 was torn loose from NGC 2442 by a companion. [7]

HIPASS J1712-64

HIPASS J1712-64 is an isolated extragalactic cloud of neutral hydrogen with no associated stars. [8] The cloud is a binary system and is not dense enough to form stars. [8] HIPASS J1712-64 was probably ejected during an interaction between the Magellanic clouds and the Milky way.

New galaxies in the Centaurus A/M83 Group

Ten new galaxies were identified in the Centaurus A/M83 Group, bringing the total (at the time) to 31 galaxies. [9]

See also

Related Research Articles

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<span class="mw-page-title-main">NGC 2552</span> Magellanic Spiral galaxy in the constellation Lynx

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<span class="mw-page-title-main">NGC 2397</span> Galaxy in the constellation Volans

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<span class="mw-page-title-main">NGC 299</span> Open star cluster in the constellation Tucana

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<span class="mw-page-title-main">NGC 376</span> Globular cluster located in the constellation Tucana

NGC 376 is a young open cluster of stars in the southern constellation of Tucana. It was discovered on September 2, 1826, by Scottish astronomer James Dunlop. Dreyer, a Danish/British astronomer, described it as a "globular cluster, bright, small, round." It is irregular in form, with a central spike.

<span class="mw-page-title-main">NGC 3256</span> Peculiar galaxy in the constellation Vela

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<span class="mw-page-title-main">NGC 3175</span> Galaxy in the constellation Antlia

NGC 3175 is a spiral galaxy located in the far eastern part of the southern constellation of Antlia at an approximate distance of 54 million light-years. NGC 3175 was discovered on March 30, 1835 by English astronomer John Herschel, whose notes described it as, "considerably bright, large, much extended NE-SW, very gradually little brighter middle". This galaxy is the namesake of the NGC 3175 group of galaxies, which includes the spiral galaxy NGC 3137.

References

  1. ↑ "HI Parkes All Sky Survey (homepage)".
  2. ↑ Koribalski, B. S.; et al. (2004). "HIPASS Bright Galaxy Catalog". The Astronomical Journal. 128 (1): 16. arXiv: astro-ph/0404436 . Bibcode:2004AJ....128...16K. doi:10.1086/421744. S2CID   16229767.
  3. 1 2 Meyer, M. J.; et al. (2004). "Southern HIPASS catalog". Monthly Notices of the Royal Astronomical Society. 350 (4): 1195. arXiv: astro-ph/0406384 . Bibcode:2004MNRAS.350.1195M. doi: 10.1111/j.1365-2966.2004.07710.x . S2CID   10336076.
  4. 1 2 Wong, O. I.; et al. (2006). "Northern HIPASS Catalog". Monthly Notices of the Royal Astronomical Society. 371 (4): 1855–1864. arXiv: astro-ph/0607491 . Bibcode:2006MNRAS.371.1855W. doi: 10.1111/j.1365-2966.2006.10846.x . S2CID   22014830.
  5. ↑ Calabretta, Mark R.; Staveley-Smith, Lister; Barnes, David G. (2014). "A New 1.4 GHz Radio Continuum Map of the Sky South of Declination +25°". Publications of the Astronomical Society of Australia. 31: e007. arXiv: 1310.2414 . Bibcode:2014PASA...31....7C. doi: 10.1017/pasa.2013.36 . ISSN   1323-3580.
  6. 1 2 "Multibeam Receiver". Archived from the original on 2000-08-19.
  7. 1 2 3 Ryder, S.D.; et al. (July 2001). "HIPASS Detection of an Intergalactic Gas Cloud in the NGC 2442 Group". The Astrophysical Journal. 555 (1): 232–239. arXiv: astro-ph/0103099 . Bibcode:2001ApJ...555..232R. doi:10.1086/321453. S2CID   14455875.
  8. 1 2 Kilborn V.A.; et al. (September 2002). "An Extragalactic H I Cloud with No Optical Counterpart?". The Astronomical Journal. 120 (3): 1342. arXiv: astro-ph/0005267 . Bibcode:2000AJ....120.1342K. doi:10.1086/301542. S2CID   11668655.
  9. ↑ Banks D.G.; et al. (October 1999). "New Galaxies Discovered in the First Blind H I Survey of the Centaurus A Group". The Astrophysical Journal. 524 (2): 612–622. arXiv: astro-ph/9906146 . Bibcode:1999ApJ...524..612B. doi:10.1086/307854. S2CID   118921426.
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