113:. All data have been fully observed, and the Hydra field has been calibrated and imaged, leading to the first internal release of data for almost 150 HI detections in the direction of the Hydra cluster. WALLABY science teams are currently analysing the Hydra data, and first science papers are expected in late 2020.
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and L. Staveley-Smith. It was ranked by ASKAP in the top two of ten Survey
Science projects, with Koribalski and Staveley-Smith the principal investigators. Koribalski stepped down in 2019. Currently, Lister Staveley-Smith is the Principal Investigator, Karen Lee-Waddell is the project scientist,
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Several science results have been published from WALLABY Early
Science observations. Highlights include three observations of groups of galaxies, and two detailed studies of nearby galaxies.
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Reynolds, T. N.; Westmeier, T.; Staveley-Smith, L.; Elagali, A.; For, B.-Q.; Kleiner, D.; Koribalski, B. S.; Lee-Waddell, K.; Madrid, J. P.; Popping, A.; Rhee, J. (2019-01-21).
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Lee-Waddell, K.; Koribalski, B. S.; Westmeier, T.; Elagali, A.; For, B.-Q.; Kleiner, D.; Madrid, J. P.; Popping, A.; Reynolds, T. N.; Rhee, J.; Serra, P. (2019-08-21).
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Elagali, A.; Staveley-Smith, L.; Rhee, J.; Wong, O. I.; Bosma, A.; Westmeier, T.; Koribalski, B. S.; Heald, G.; For, B.-Q.; Kleiner, D.; Lee-Waddell, K. (2019-08-01).
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In preparation for the full WALLABY survey, expected to start in 2021, WALLABY conducted a pilot survey in 2020, consisting of three survey fields in the direction of
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Kleiner, D.; Koribalski, B. S.; Serra, P.; Whiting, M. T.; Westmeier, T.; Wong, O. I.; Kamphuis, P.; Popping, A.; Bekiaris, G.; Elagali, A.; For, B.-Q. (2019-10-01).
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For, B.-Q.; Staveley-Smith, L.; Westmeier, T.; Whiting, M.; Oh, S.-H.; Koribalski, B.; Wang, J.; Wong, O. I.; Bekiaris, G.; Cortese, L.; Elagali, A. (2019-11-11).
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a study of the HI properties of galaxies, groups and clusters, including the influence of the environment on galaxy evolution;
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and Tobias
Westmeier is the project manager.. The WALLABY team now has over 150 members.
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131:"The Australian Square Kilometre Array Pathfinder finally hits the big-data highway"
269:"WALLABY early science − V. ASKAP H i imaging of the Lyon Group of Galaxies 351"
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52:/beam in each 4 km/s channel. WALLABY is expected to detect about 500,000
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422:"WALLABY Early Science – IV. ASKAP H i imaging of the nearby galaxy IC 5201"
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20:(WALLABY) is a next-generation survey of the 21 cm radio emission from
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473:"WALLABY early science – III. An H i study of the spiral galaxy NGC 1566"
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32:(ASKAP) telescope, WALLABY will survey three-quarters of the sky over a
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Koribalski, Bärbel S.; Staveley-Smith, L.; Westmeier, T.; Serra, P.;
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with a mean redshift of 0.05, at a mean distance of about 200
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The WALLABY project was proposed in 2009 by a team led by
320:"WALLABY Early Science – II. The NGC 7232 galaxy group"
371:"WALLABY early science – I. The NGC 7162 galaxy group"
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a census of gas-rich galaxies in the vicinity of the
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Schinckel, Antony; Bock, Douglas (16 January 2017).
18:Widefield ASKAP L-band Legacy All-sky Blind surveY
477:Monthly Notices of the Royal Astronomical Society
426:Monthly Notices of the Royal Astronomical Society
375:Monthly Notices of the Royal Astronomical Society
324:Monthly Notices of the Royal Astronomical Society
273:Monthly Notices of the Royal Astronomical Society
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30:Australian Square Kilometer Array Pathfinder
60:. The scientific goals of WALLABY include:
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164:"WALLABY – an SKA Pathfinder H i survey"
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228:"WALLABY Survey – WALLABY Survey Site"
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533:Science and technology in Australia
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168:Astrophysics and Space Science
48:and a sensitivity of 1.6
1:
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198:10.1007/s10509-020-03831-4
162:; Zwaan, M. (2020-07-13).
36:range −90° to +30° to a
40:of 0.26. It will have a
248:"Team – WALLABY Survey"
190:2020Ap&SS.365..118K
28:. It is hosted by the
500:10.1093/mnras/stz1448
449:10.1093/mnras/stz2063
398:10.1093/mnras/sty2930
286:10.1093/mnras/stz2501
89:Early science results
347:10.1093/mnras/stz017
97:WALLABY pilot survey
528:Science experiments
42:angular resolution
24:(HI) in the Local
160:Ryan-Weber, E. V.
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135:The Conversation
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82:B. S. Koribalski
22:neutral hydrogen
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138:. Retrieved
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296:1885/266365
66:Local Group
34:Declination
522:Categories
490:1905.09491
439:1907.12556
388:1810.12466
337:1901.00241
253:2020-10-12
233:2020-10-12
181:2002.07311
174:(7): 118.
140:2020-10-12
117:References
509:0035-8711
458:0035-8711
407:0035-8711
356:0035-8711
305:0035-8711
214:211146706
206:1572-946X
538:Hydrogen
107:NGC 4636
54:galaxies
38:redshift
26:Universe
186:Bibcode
76:History
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46:arcsec
44:of 30
485:arXiv
434:arXiv
383:arXiv
332:arXiv
210:S2CID
176:arXiv
111:Norma
103:Hydra
505:ISSN
454:ISSN
403:ISSN
352:ISSN
301:ISSN
202:ISSN
109:and
16:The
495:doi
481:487
444:doi
430:488
393:doi
379:482
342:doi
328:487
291:hdl
281:doi
277:489
194:doi
172:365
58:Mpc
50:mJy
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