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

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.