We request six observations for ASKAP~J1832--0911, a 44-minute Ultra-long period object, with Murriyang ultra-wide-bandwidth low-frequency receiver (UWL). The proposed observation can help us measure and understand different kinds of sub-structures of the pulse over a wide frequency range. The observation can also serve as a pilot observation to develop a method to measure wide pulses with a single-dish telescope. This observation will help us measure the physical parameters of the source and its surrounding environment, and will also help us map the system geometry so that we can model the emission mechanism.