Data

ASKAP Project AS102: WALLABY Pilot Survey DR2 - Mosaicked Data Cubes and Images

The University of Western Australia
Murugeshan, Chandra ; Shen, Austin ; Westmeier, Tobias ; Deg, Nathan ; Spekkens, Kristine ; Huynh, Minh ; Goliath, Sharon ; Venkataraman, Parthasarathy
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ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2FANDS&rft_id=info:doi10.25919/hg66-4v60&rft.title=ASKAP Project AS102: WALLABY Pilot Survey DR2 - Mosaicked Data Cubes and Images&rft.identifier=10.25919/hg66-4v60&rft.publisher=CSIRO Publishing&rft.description=These are full-sensitivity mosaicked data cubes and images of the three fields observed during phase 2 of the WALLABY pilot survey. Mosaics in this collection include: extragalactic spectral-line data cubes and weights cubes. The WALLABY pilot survey DR2 includes observations of three fields in the directions of the NGC 5044 galaxy group, the NGC 4808 galaxy group and the Vela cluster. The NGC 5044 field mosaics cover 120 square degrees and are formed from SBIDs 33879, 34302, 34166, 34275, 31536, 40905, 25701, 25750. The NGC 4808 field mosaics cover 60 square degrees and are formed from SBIDs 33681, 37604. The Vela field mosaics cover 60 square degrees and are formed from SBIDs 33521, 33596. Users of the data are requested to include a reference to the data release paper (Murugeshan et al. 2024, in prep.), the Phase 1 data release paper (Westmeier et al. 2022, PASA, 39, 58), and the WALLABY survey description paper (Koribalski et al. 2020, Ap&SS, 365, 118) in any publication resulting from their analysis.&rft.creator=Murugeshan, Chandra &rft.creator=Shen, Austin &rft.creator=Westmeier, Tobias &rft.creator=Deg, Nathan &rft.creator=Spekkens, Kristine &rft.creator=Huynh, Minh &rft.creator=Goliath, Sharon &rft.creator=Venkataraman, Parthasarathy &rft.date=2024&rft.type=dataset&rft.language=English Access the data

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These are full-sensitivity mosaicked data cubes and images of the three fields observed during phase 2 of the WALLABY pilot survey. Mosaics in this collection include: extragalactic spectral-line data cubes and weights cubes. The WALLABY pilot survey DR2 includes observations of three fields in the directions of the NGC 5044 galaxy group, the NGC 4808 galaxy group and the Vela cluster. The NGC 5044 field mosaics cover 120 square degrees and are formed from SBIDs 33879, 34302, 34166, 34275, 31536, 40905, 25701, 25750. The NGC 4808 field mosaics cover 60 square degrees and are formed from SBIDs 33681, 37604. The Vela field mosaics cover 60 square degrees and are formed from SBIDs 33521, 33596. Users of the data are requested to include a reference to the data release paper (Murugeshan et al. 2024, in prep.), the Phase 1 data release paper (Westmeier et al. 2022, PASA, 39, 58), and the WALLABY survey description paper (Koribalski et al. 2020, Ap&SS, 365, 118) in any publication resulting from their analysis.

Notes

External Organisations
CSIRO Environment; Queen's University Kingston; Royal Military College of Canada; Herzberg Astronomy and Astrophysics Research Centre; University of Toronto
Associated Persons
Austin Shen (Creator); Kristine Spekkens (Creator)Chandra Murugeshan (Creator); Nathan Deg (Creator); Sharon Goliath (Creator); Parthasarathy Venkataraman (Creator)

Issued: 2024-09-11

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Identifiers
ACN 633 798 857