Enhanced astrometry of the rapid ASKAP continuum survey: Mid and high-frequency epochs

Abstract

Accurate radio astrometry is essential for reliable cross-identification of sources across wavelengths, precision localisation of transient events, and the construction of stable all-sky reference catalogues. In this work, we extend our astrometric correction framework for the Rapid Australian Square Kilometre Array Pathfinder (ASKAP) Continuum Survey (RACS) to its mid- and high-frequency epochs (RACS-Mid1 and RACS-High1), building on our previous corrections to the low-frequency surveys. Using a hierarchical cross-matching strategy with high-precision external catalogues, we remove large-scale systematic positional errors that were present in the uncorrected data and significantly reduce the residual scatter across the sky. After correction, the median positional offsets are effectively eliminated, and the 68% confidence interval of the mean residuals of RACS source positions averaged over

1 sq. deg. regions is reduced from

greater than or equivalent to ≳ $\gtrsim$

0.4 double prime 0.4 ″ $0.4''$

to

less than or equivalent to ≲ $\lesssim$

0.18 double prime 0.18 ″ $0.18''$

over most of the survey area for both epochs. Independent validation against multiple external radio astrometric references confirms that individual corrected RACS source positions are accurate to a 1-

sigma σ $\sigma$

confidence level of

tilde ∼ $\sim$

0.25 double prime 0.25 ″ $0.25''$

across the bulk of the sky, with slightly degraded performance within the Galactic plane. While motivated primarily by the need for improved localisation of ASKAP fast radio bursts, these corrections also benefit a wide range of science applications, including transient identification, multiwavelength host association, and studies of Galactic and extragalactic radio populations. Together with our previous work, this establishes RACS as the highest precision arcsecond-resolution all-sky astrometric reference in the southern hemisphere at decimetre wavelengths.