SIMBAD references

The Australian Square Kilometre Array Pathfinder (ASKAP) will revolutionize our knowledge of gas-rich galaxies in the Universe. Here we present predictions for two proposed extragalactic ASKAP neutral hydrogen (HI) emission-line surveys, based on semi-analytic models applied to cosmological N-body simulations. The ASKAP HI All-Sky Survey, known as Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY), is a shallow 3 π survey{Ux2028}(z = 0–0.26) which will probe the mass and dynamics of over 6 x 10⁵ galaxies. A much deeper small-area HI survey, called Deep Investigation of Neutral Gas Origins (DINGO), aims to trace the evolution of HI from z = 0 to 0.43, a cosmological volume of 4 x 10⁷Mpc³, detecting potentially 10⁵ galaxies. The high-sensitivity 30 antenna ASKAP core (diameter ∼ 2km) will provide an angular resolution of 30arcsec (at z = 0). Our simulations show that the majority of galaxies detected in WALLABY (87.5per cent) will be resolved. About 5000 galaxies will be well resolved, i.e. more than five beams (2.5arcmin) across the major axis, enabling kinematic studies of their gaseous discs. This number would rise to 1.6 x 10⁵ galaxies if all 36 ASKAP antennas could be used; the additional six antennas provide baselines up to 6km, resulting in an angular resolution of 10arcsec. For DINGO this increased resolution is highly desirable to minimize source confusion, reducing confusion rates from a maximum of 10per cent of sources at the survey edge to 3per cent. We estimate that the sources detected by WALLABY and DINGO will span four orders of magnitude in total halo mass (from 10¹¹ to 10¹⁵M_☉) and nearly seven orders of magnitude in stellar mass (from 10⁵ to 10¹²M_☉), allowing us to investigate the process of galaxy formation across the last four billion years.