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Australian Square Kilometre Array Pathfinder: Difference between revisions

Coordinates: 26°41′46″S 116°38′13″E / 26.696°S 116.637°E / -26.696; 116.637
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The construction and assembly of the dishes was completed in June 2012.<ref>{{cite web|url=http://www.atnf.csiro.au/projects/askap/news_antenna_18062012.html |title=ASKAP News |publisher=Atnf.csiro.au |date=18 June 2012 |accessdate=18 January 2013}}</ref>
The construction and assembly of the dishes was completed in June 2012.<ref>{{cite web|url=http://www.atnf.csiro.au/projects/askap/news_antenna_18062012.html |title=ASKAP News |publisher=Atnf.csiro.au |date=18 June 2012 |accessdate=18 January 2013}}</ref>


The features that will make ASKAP an unprecedented [[wikt:synoptic|synoptic]] telescope include a wide [[Field of view#Astronomy|field-of-view]], large [[Bandwidth (signal processing)|spectral bandwidth]], extremely fast survey speed, and multiple [[baseline (interferometry)|baseline]]s.<ref>{{cite web |title=Murchison Radio-astronomy Observatory |publisher=CSIRO |accessdate= 13 April 2011 |url=http://www.atnf.csiro.au/projects/askap/site.html}}</ref>
ASKAP was designed as a [[wikt:synoptic|synoptic]] telescope with a wide [[Field of view#Astronomy|field-of-view]], large [[Bandwidth (signal processing)|spectral bandwidth]], fast survey speed, and a large number of simultaneous [[baseline (interferometry)|baseline]]s.<ref>{{cite web |title=Murchison Radio-astronomy Observatory |publisher=CSIRO |accessdate= 13 April 2011 |url=http://www.atnf.csiro.au/projects/askap/site.html}}</ref>


[[File:Installing an ASKAP Phased Array Feed receiver.JPG|thumb|Installation of an advanced [[Phased Array]] Feed (PAF) receiver on an ASKAP antenna. This feed includes 188 individual receivers, to greatly extend the Field of View of an ASKAP 12m dish to 30 square degrees.]]
[[File:Installing an ASKAP Phased Array Feed receiver.JPG|thumb|Installation of an advanced [[Phased Array]] Feed (PAF) receiver on an ASKAP antenna. This feed includes 188 individual receivers, to greatly extend the Field of View of an ASKAP 12m dish to 30 square degrees.]]


ASKAP is located in the [[Murchison (Western Australia)|Murchison]] district in Western Australia, a region that is extremely "radio-quiet" due to the low population density and resultant lack of [[Radio frequency interference|radio interference]] (generated by human activity) that would otherwise interfere with weak [[Astronomical radio source|astronomical signals]].<ref>{{cite news |title=World's biggest radio telescope, Square Kilometre Array |publisher= [[BBC Radio 4]] |accessdate= 13 April 2011 |url=https://www.bbc.co.uk/news/science-environment-12891215/}}</ref>
ASKAP is located in the [[Murchison (Western Australia)|Murchison]] district in Western Australia, a region that is extremely "radio-quiet" due to the low population density and resulting lack of [[Radio frequency interference|radio interference]] (generated by human activity) that would otherwise interfere with weak [[Astronomical radio source|astronomical signals]].<ref>{{cite news |title=World's biggest radio telescope, Square Kilometre Array |publisher= [[BBC Radio 4]] |accessdate= 13 April 2011 |url=https://www.bbc.co.uk/news/science-environment-12891215/}}</ref> The radio quiet location is recognised as a natural resource and protected by the [[Australian Government|Australian Commonwealth]] and [[Government of Western Australia|Western Australia State Government]] through a range of regulatory measures.


Data from ASKAP are transmitted from the MRO to a [[supercomputer]] (acting as a [[radio correlator]]) at the [[Joseph Lade Pawsey|Pawsey]] Supercomputing Centre in [[Perth, Western Australia|Perth]].<ref>{{cite web|title=Pawsey Centre |publisher=iVEC |date=14 June 2012 |url=http://www.ivec.org/ivec-projects/pawsey/ |url-status=dead |archiveurl=https://web.archive.org/web/20130307220253/http://www.ivec.org/ivec-projects/pawsey/ |archivedate=7 March 2013 }}</ref> The data are processed in near-real-time by a [[Instruction pipeline|pipeline processor]] running purpose-built software.<ref>{{cite web |title=ASKAP Science Update, Vol. 5 |publisher= CSIRO |accessdate= 13 April 2011 |url= http://www.atnf.csiro.au/projects/askap/ASKAP_Science_Update_5.pdf }}</ref> All data are made publicly available after quality checks by the ten ASKAP Survey Science Teams.
The unique radio quiet nature is being recognised as a natural resource and is being protected by the [[Australian Government|Australian Commonwealth]] and [[Government of Western Australia|Western Australia State Government]] through a range of protective regulatory measures.

Data from ASKAP will be transmitted from the MRO to a [[supercomputer]] at the [[Joseph Lade Pawsey|Pawsey]] Supercomputing Centre in [[Perth, Western Australia|Perth]]. The data will be converted to images of the sky in near-real-time by a [[Instruction pipeline|pipeline processor]] running the purpose-built ASKAPsoft package.<ref>{{cite web |title=ASKAP Science Update, Vol. 5 |publisher= CSIRO |accessdate= 13 April 2011 |url= http://www.atnf.csiro.au/projects/askap/ASKAP_Science_Update_5.pdf }}</ref> All data will be placed in the public domain after being checked for quality by the ten ASKAP Survey Science Teams. Post processing will be supported by supercomputers operated by iVEC at the Pawsey Centre<ref>{{cite web|title=Pawsey Centre |publisher=iVEC |date=14 June 2012 |url=http://www.ivec.org/ivec-projects/pawsey/ |url-status=dead |archiveurl=https://web.archive.org/web/20130307220253/http://www.ivec.org/ivec-projects/pawsey/ |archivedate=7 March 2013 }}</ref> in Perth, and may also be complemented by '[[theSkyNet]]',<ref>{{cite web
|url=http://www.theskynet.org/about/index
|title=theSkyNet Data
|publisher=International Centre for Radio Astronomy Research
|accessdate=21 December 2011
}}</ref> a "community computing initiative"<ref name=theSkyNet>{{cite web|title=theSkyNet comes alive |url=http://www.ska.gov.au/news/Pages/110929_theskynet.aspx |work=Australia and New Zealand SKA project (anzSKA) |publisher=Australian [[Department of Innovation, Industry, Science and Research]] |accessdate=25 May 2012 |url-status=dead |archiveurl=https://web.archive.org/web/20120321130424/http://www.ska.gov.au/news/Pages/110929_theskynet.aspx |archivedate=21 March 2012 }}</ref> similar to [[Seti@home]].


== Science ==
== Science ==

Revision as of 19:34, 2 June 2020

Australian Square Kilometre Array Pathfinder
Antennas of the ASKAP telescope at the Murchison Radio-astronomy Observatory in Western Australia
Part ofAustralia Telescope National Facility
Murchison Radio-astronomy Observatory
Square Kilometre Array Edit this on Wikidata
Location(s)Western Australia, AUS
Coordinates26°41′46″S 116°38′13″E / 26.696°S 116.637°E / -26.696; 116.637 Edit this at Wikidata
OrganizationCSIRO Edit this on Wikidata
Telescope styleradio interferometer Edit this on Wikidata
Websitewww.atnf.csiro.au/projects/askap/,%20https://www.csiro.au/askap Edit this at Wikidata
Australian Square Kilometre Array Pathfinder is located in Australia
Australian Square Kilometre Array Pathfinder
Location of Australian Square Kilometre Array Pathfinder
  Related media on Commons
[edit on Wikidata]

The Australian Square Kilometre Array Pathfinder (ASKAP) is a radio telescope array located at Murchison Radio-astronomy Observatory (MRO) in the Australian Mid West. It is operated by the Commonwealth Scientific and Industrial Research Organisation (CSIRO) and forms part of the Australia Telescope National Facility.[1] Construction commenced in late 2009 and first light was in October 2012.[2][3]

ASKAP consists of 36 identical parabolic antennas, each 12 metres in diameter, working together as a single astronomical interferometer with a total collecting area of approximately 4,000 square metres. Each antenna is equipped with a phased-array feed, increasing the field of view. This design provides both fast survey speed and high sensitivity.

The facility began as a technology demonstrator for the international Square Kilometre Array (SKA), a planned radio telescope which will be larger and more sensitive.[4] The ASKAP site has been selected as one of the SKA's two central locations.[5]

Description

Development and construction of ASKAP was led by CSIRO Astronomy and Space Science (CASS), in collaboration with scientists and engineers in The Netherlands, Canada and the US, as well as colleagues from Australian universities and industry partners in China.[2]

Design

External videos
video icon Watch a video of the first ASKAP antenna construction at the MRO in January 2010.

The construction and assembly of the dishes was completed in June 2012.[6]

ASKAP was designed as a synoptic telescope with a wide field-of-view, large spectral bandwidth, fast survey speed, and a large number of simultaneous baselines.[7]

Installation of an advanced Phased Array Feed (PAF) receiver on an ASKAP antenna. This feed includes 188 individual receivers, to greatly extend the Field of View of an ASKAP 12m dish to 30 square degrees.

ASKAP is located in the Murchison district in Western Australia, a region that is extremely "radio-quiet" due to the low population density and resulting lack of radio interference (generated by human activity) that would otherwise interfere with weak astronomical signals.[8] The radio quiet location is recognised as a natural resource and protected by the Australian Commonwealth and Western Australia State Government through a range of regulatory measures.

Data from ASKAP are transmitted from the MRO to a supercomputer (acting as a radio correlator) at the Pawsey Supercomputing Centre in Perth.[9] The data are processed in near-real-time by a pipeline processor running purpose-built software.[10] All data are made publicly available after quality checks by the ten ASKAP Survey Science Teams.

Science

The array in 2010

During ASKAP's first five years of operation, at least 75% of its time will be used for large Survey Science Projects. ASKAP is expected to make substantial advances in key areas, including the following:[11]

  1. Galaxy formation and gas evolution in the nearby Universe through extragalactic HI surveys
  2. Evolution, formation and population of galaxies across cosmic time via high resolution, continuum surveys
  3. Characterisation of the radio transient sky through detection and monitoring (including VLBI) of transient and variable sources, and
  4. Evolution of magnetic fields in galaxies over cosmic time through polarisation surveys.

Discoveries

In May 2020, astronomers announced a measurement of the intergalactic medium using six fast radio bursts observed with ASKAP; their results confirm existing measurements of the missing baryon problem.[12][13]

ASKAP Survey Science Projects

In 2009, after an open call for proposals, CSIRO announced that ten major science projects had been selected to use ASKAP.[14] Of the ten projects' authors, 33% were from Australia and New Zealand, 30% from North America, 28% from Europe, and 9% from elsewhere in the world.

The ten ASKAP Survey Science Projects are:

Highest Priority

Slightly Lower Priority

  • COAST: Compact Objects with ASKAP: Surveys and Timing
  • CRAFT: The Commensal Real-time ASKAP Fast Transients survey
  • DINGO: Deep Investigations of Neutral Gas Origins[17]
  • FLASH: The First Large Absorption Survey in HI[18]
  • GASKAP: The Galactic ASKAP Spectral Line Survey[19]
  • POSSUM: Polarization Sky Survey of the Universe's Magnetism[20]
  • VAST: An ASKAP Survey for Variables and Slow Transients[21]
  • VLBI: The High Resolution Components of ASKAP: Meeting the Long Baseline Specifications for the SKA

See also

Wikimedia Commons has media related to Australian Square Kilometre Array Pathfinder.

References

  1. ^ "The Australia Telescope National Facility". CSIRO. Retrieved 13 April 2011.
  2. ^ a b "ASKAP Fast Facts" (PDF). CSIRO. Retrieved 13 April 2011.
  3. ^ Fingas, Jon (5 October 2012). "Australia Square Kilometre Array Pathfinder goes live as the world's quickest radio telescope". Engadget. Retrieved 7 October 2012.
  4. ^ "SKA Factsheet for Journalists" (PDF). SKA Project Development Office (SPDO). Skatelescope.org. Retrieved 13 April 2011.
  5. ^ "Report of the SKA Siting Options Working Group" (PDF). SKA Organisation. Skatelescope.org. 14 June 2012.
  6. ^ "ASKAP News". Atnf.csiro.au. 18 June 2012. Retrieved 18 January 2013.
  7. ^ "Murchison Radio-astronomy Observatory". CSIRO. Retrieved 13 April 2011.
  8. ^ "World's biggest radio telescope, Square Kilometre Array". BBC Radio 4. Retrieved 13 April 2011.
  9. ^ "Pawsey Centre". iVEC. 14 June 2012. Archived from the original on 7 March 2013.
  10. ^ "ASKAP Science Update, Vol. 5" (PDF). CSIRO. Retrieved 13 April 2011.
  11. ^ "ASKAP Science". CSIRO. Retrieved 8 November 2010.
  12. ^ Slezak, Michael; Timms, Penny (27 May 2020). "Half the matter in the universe was missing. Australian scientists just found it". ABC News (on-line). Australian Broadcasting Corporation. Retrieved 27 May 2020.
  13. ^ MacQuart, J.-P.; Prochaska, J. X.; McQuinn, M.; Bannister, K. W.; Bhandari, S.; Day, C. K.; Deller, A. T.; Ekers, R. D.; James, C. W.; Marnoch, L.; Osłowski, S.; Phillips, C.; Ryder, S. D.; Scott, D. R.; Shannon, R. M.; Tejos, N. (2020). "A census of baryons in the Universe from localized fast radio bursts". Nature. 581 (7809): 391–395. arXiv:2005.13161. Bibcode:2020Natur.581..391M. doi:10.1038/s41586-020-2300-2. PMID 32461651.
  14. ^ "CSIRO sets science path for new telescope". CSIRO. Archived from the original on 19 March 2011. Retrieved 13 April 2011.
  15. ^ "EMU: Evolutionary Map of the Universe". Atnf.csiro.au. 7 November 2008. Retrieved 18 January 2013.
  16. ^ "WALLABY – the ASKAP HI All-Sky Survey". Atnf.csiro.au. Retrieved 18 January 2013.
  17. ^ "DINGO". Internal.physics.uwa.edu.au. Retrieved 18 January 2013.
  18. ^ "Sydney Institute for Astronomy – The University of Sydney". Physics.usyd.edu.au. 15 September 2011. Retrieved 18 January 2013.
  19. ^ "GASKAP". Retrieved 18 January 2013.
  20. ^ "ASKAP POSSUM – Home Page". Physics.usyd.edu.au. 24 August 2012. Archived from the original on 12 October 2016. Retrieved 18 January 2013.
  21. ^ "VAST: Variables and Slow Transients: Main – Home Page browse". Physics.usyd.edu.au. Retrieved 18 January 2013.
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