Parkes observations for project P885 semester 2024OCTS_01

We propose a reduced even more modest program to continue monitoring 4 of the 6 known radio magnetars, tracking their rotational, flux density, and polarisation properties. The rotational response of 1E 1547.0-5408 to its 2022 'hiccup' in radiative properties is still developing, requiring frequent observations every ~10 days. The cadence and request for Swift J1818.0-1607 is reduced, commensurate with its decreased activity/flux. Observations of XTE J1810-197, and PSR J1622-4950 which ceased emission in 2022, remain at reduced levels. The overall request is 13.5 hours.