Parkes observations for project P1099 semester 2021APRS_02

CU Virginis is the best-studied member of the class of stellar radio transients known as stellar pulsars. Its circularly polarised radio pulses are explained by a model, which has consequences for the frequency-time dependence, polarisation and spectra of the pulses which can be tested using the Parkes ultra-wide-bandwidth receiver system. We propose to perform these tests and to demonstrate that the Parkes telescope can be used to observe transient events on time scales of minutes to hours.